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id="toc-Specific_bands-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-Dynamics" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Dynamics"> <div class="vector-toc-text"> 4 Dynamics </div> </a> <button aria-controls="toc-Dynamics-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> Toggle Dynamics subsection </button> <ul id="toc-Dynamics-sublist" class="vector-toc-list"> <li id="toc-Shallow_models" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Shallow_models"> <div class="vector-toc-text"> 4.1 Shallow models </div> </a> <ul id="toc-Shallow_models-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Deep_models" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Deep_models"> <div class="vector-toc-text"> 4.2 Deep models </div> </a> <ul id="toc-Deep_models-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Internal_heat" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Internal_heat"> <div class="vector-toc-text"> 4.3 Internal heat </div> </a> <ul id="toc-Internal_heat-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-Discrete_features" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Discrete_features"> <div class="vector-toc-text"> 5 Discrete features </div> </a> <button aria-controls="toc-Discrete_features-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> Toggle Discrete features subsection </button> <ul id="toc-Discrete_features-sublist" class="vector-toc-list"> <li id="toc-Vortices" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Vortices"> <div class="vector-toc-text"> 5.1 Vortices </div> </a> <ul id="toc-Vortices-sublist" class="vector-toc-list"> <li id="toc-Great_Red_Spot" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#Great_Red_Spot"> <div class="vector-toc-text"> 5.1.1 Great Red Spot </div> </a> <ul id="toc-Great_Red_Spot-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Oval_BA" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#Oval_BA"> <div class="vector-toc-text"> 5.1.2 Oval BA </div> </a> <ul id="toc-Oval_BA-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-Storms_and_lightning" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Storms_and_lightning"> <div class="vector-toc-text"> 5.2 Storms and lightning </div> </a> <ul id="toc-Storms_and_lightning-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Circumpolar_cyclones" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Circumpolar_cyclones"> <div class="vector-toc-text"> 5.3 Circumpolar cyclones </div> </a> <ul id="toc-Circumpolar_cyclones-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Disturbances" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Disturbances"> <div class="vector-toc-text"> 5.4 Disturbances </div> </a> <ul id="toc-Disturbances-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Hot_spots" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Hot_spots"> <div class="vector-toc-text"> 5.5 Hot spots </div> </a> <ul id="toc-Hot_spots-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-The_possibility_of_life" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#The_possibility_of_life"> <div class="vector-toc-text"> 5.6 The possibility of life </div> </a> <ul id="toc-The_possibility_of_life-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-Observational_history" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Observational_history"> <div class="vector-toc-text"> 6 Observational history </div> </a> <button aria-controls="toc-Observational_history-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> Toggle Observational history subsection </button> <ul id="toc-Observational_history-sublist" class="vector-toc-list"> <li id="toc-Great_Red_Spot_studies" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Great_Red_Spot_studies"> <div class="vector-toc-text"> 6.1 Great Red Spot studies </div> </a> <ul id="toc-Great_Red_Spot_studies-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-White_ovals" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#White_ovals"> <div class="vector-toc-text"> 6.2 White ovals </div> </a> <ul id="toc-White_ovals-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-See_also" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#See_also"> <div class="vector-toc-text"> 7 See also </div> </a> <ul id="toc-See_also-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Notes" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Notes"> <div class="vector-toc-text"> 8 Notes </div> </a> <ul id="toc-Notes-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-References" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#References"> <div class="vector-toc-text"> 9 References </div> </a> <ul id="toc-References-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Cited_sources" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Cited_sources"> <div class="vector-toc-text"> 10 Cited sources </div> </a> <ul id="toc-Cited_sources-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Further_reading" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Further_reading"> <div class="vector-toc-text"> 11 Further reading </div> </a> <ul id="toc-Further_reading-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-External_links" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#External_links"> <div class="vector-toc-text"> 12 External links </div> </a> <ul id="toc-External_links-sublist" class="vector-toc-list"> </ul> </li> </ul> </div> </div> </nav> </div> </div> <div class="mw-content-container"> <main id="content" class="mw-body"> <header class="mw-body-header vector-page-titlebar"> <nav aria-label="Contents" class="vector-toc-landmark"> <div id="vector-page-titlebar-toc" class="vector-dropdown vector-page-titlebar-toc vector-button-flush-left" > <input type="checkbox" id="vector-page-titlebar-toc-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-vector-page-titlebar-toc" class="vector-dropdown-checkbox " aria-label="Toggle the table of contents" > <label id="vector-page-titlebar-toc-label" for="vector-page-titlebar-toc-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--icon-only " aria-hidden="true" > Toggle the table of contents </label> <div class="vector-dropdown-content"> <div id="vector-page-titlebar-toc-unpinned-container" class="vector-unpinned-container"> </div> </div> </div> </nav> <h1 id="firstHeading" class="firstHeading mw-first-heading">Atmosphere of Jupiter</h1> <div id="p-lang-btn" class="vector-dropdown mw-portlet mw-portlet-lang" > <input type="checkbox" id="p-lang-btn-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-p-lang-btn" class="vector-dropdown-checkbox 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Available in 27 languages" > <label id="p-lang-btn-label" for="p-lang-btn-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--action-progressive mw-portlet-lang-heading-27" aria-hidden="true" > 27 languages </label> <div class="vector-dropdown-content"> <div class="vector-menu-content"> <ul class="vector-menu-content-list"> <li class="interlanguage-link interwiki-ar mw-list-item"><a href="https://ar.wikipedia.org/wiki/%D8%BA%D9%84%D8%A7%D9%81_%D8%A7%D9%84%D9%85%D8%B4%D8%AA%D8%B1%D9%8A_%D8%A7%D9%84%D8%AC%D9%88%D9%8A" title="غلاف المشتري الجوي – Arabic" lang="ar" hreflang="ar" data-title="غلاف المشتري الجوي" data-language-autonym="العربية" data-language-local-name="Arabic" class="interlanguage-link-target">العربية</a></li><li class="interlanguage-link interwiki-bn mw-list-item"><a href="https://bn.wikipedia.org/wiki/%E0%A6%AC%E0%A7%83%E0%A6%B9%E0%A6%B8%E0%A7%8D%E0%A6%AA%E0%A6%A4%E0%A6%BF%E0%A6%B0_%E0%A6%AC%E0%A6%BE%E0%A6%AF%E0%A6%BC%E0%A7%81%E0%A6%AE%E0%A6%A3%E0%A7%8D%E0%A6%A1%E0%A6%B2" title="বৃহস্পতির বায়ুমণ্ডল – Bangla" lang="bn" hreflang="bn" data-title="বৃহস্পতির বায়ুমণ্ডল" data-language-autonym="বাংলা" data-language-local-name="Bangla" class="interlanguage-link-target">বাংলা</a></li><li class="interlanguage-link interwiki-be mw-list-item"><a href="https://be.wikipedia.org/wiki/%D0%90%D1%82%D0%BC%D0%B0%D1%81%D1%84%D0%B5%D1%80%D0%B0_%D0%AE%D0%BF%D1%96%D1%82%D1%8D%D1%80%D0%B0" title="Атмасфера Юпітэра – Belarusian" lang="be" hreflang="be" data-title="Атмасфера Юпітэра" data-language-autonym="Беларуская" data-language-local-name="Belarusian" class="interlanguage-link-target">Беларуская</a></li><li class="interlanguage-link interwiki-ca mw-list-item"><a href="https://ca.wikipedia.org/wiki/Atmosfera_de_J%C3%BApiter" title="Atmosfera de Júpiter – Catalan" lang="ca" hreflang="ca" data-title="Atmosfera de Júpiter" data-language-autonym="Català" data-language-local-name="Catalan" class="interlanguage-link-target">Català</a></li><li class="interlanguage-link interwiki-da mw-list-item"><a href="https://da.wikipedia.org/wiki/Jupiters_atmosf%C3%A6re" title="Jupiters atmosfære – Danish" lang="da" hreflang="da" data-title="Jupiters atmosfære" data-language-autonym="Dansk" data-language-local-name="Danish" class="interlanguage-link-target">Dansk</a></li><li class="interlanguage-link interwiki-es mw-list-item"><a href="https://es.wikipedia.org/wiki/Atm%C3%B3sfera_de_J%C3%BApiter" title="Atmósfera de Júpiter – Spanish" lang="es" hreflang="es" data-title="Atmósfera de Júpiter" data-language-autonym="Español" data-language-local-name="Spanish" class="interlanguage-link-target">Español</a></li><li class="interlanguage-link interwiki-fa mw-list-item"><a href="https://fa.wikipedia.org/wiki/%D8%AC%D9%88_%D9%85%D8%B4%D8%AA%D8%B1%DB%8C" title="جو مشتری – Persian" lang="fa" hreflang="fa" data-title="جو مشتری" data-language-autonym="فارسی" data-language-local-name="Persian" class="interlanguage-link-target">فارسی</a></li><li class="interlanguage-link interwiki-fr mw-list-item"><a href="https://fr.wikipedia.org/wiki/Atmosph%C3%A8re_de_Jupiter" title="Atmosphère de Jupiter – French" lang="fr" hreflang="fr" data-title="Atmosphère de Jupiter" data-language-autonym="Français" data-language-local-name="French" class="interlanguage-link-target">Français</a></li><li class="interlanguage-link interwiki-ko mw-list-item"><a href="https://ko.wikipedia.org/wiki/%EB%AA%A9%EC%84%B1%EC%9D%98_%EB%8C%80%EA%B8%B0" title="목성의 대기 – Korean" lang="ko" hreflang="ko" data-title="목성의 대기" data-language-autonym="한국어" data-language-local-name="Korean" class="interlanguage-link-target">한국어</a></li><li class="interlanguage-link interwiki-hi mw-list-item"><a href="https://hi.wikipedia.org/wiki/%E0%A4%AC%E0%A5%83%E0%A4%B9%E0%A4%B8%E0%A5%8D%E0%A4%AA%E0%A4%A4%E0%A4%BF_%E0%A4%95%E0%A4%BE_%E0%A4%B5%E0%A4%BE%E0%A4%AF%E0%A5%81%E0%A4%AE%E0%A4%82%E0%A4%A1%E0%A4%B2" title="बृहस्पति का वायुमंडल – Hindi" lang="hi" hreflang="hi" data-title="बृहस्पति का वायुमंडल" data-language-autonym="हिन्दी" data-language-local-name="Hindi" class="interlanguage-link-target">हिन्दी</a></li><li class="interlanguage-link interwiki-hr mw-list-item"><a href="https://hr.wikipedia.org/wiki/Jupiterova_atmosfera" title="Jupiterova atmosfera – Croatian" lang="hr" hreflang="hr" data-title="Jupiterova atmosfera" data-language-autonym="Hrvatski" data-language-local-name="Croatian" class="interlanguage-link-target">Hrvatski</a></li><li class="interlanguage-link interwiki-id mw-list-item"><a href="https://id.wikipedia.org/wiki/Atmosfer_Jupiter" title="Atmosfer Jupiter – Indonesian" lang="id" hreflang="id" data-title="Atmosfer Jupiter" data-language-autonym="Bahasa Indonesia" data-language-local-name="Indonesian" class="interlanguage-link-target">Bahasa Indonesia</a></li><li class="interlanguage-link interwiki-it badge-Q17437796 badge-featuredarticle mw-list-item" title="featured article badge"><a href="https://it.wikipedia.org/wiki/Atmosfera_di_Giove" title="Atmosfera di Giove – Italian" lang="it" hreflang="it" data-title="Atmosfera di Giove" data-language-autonym="Italiano" data-language-local-name="Italian" class="interlanguage-link-target">Italiano</a></li><li class="interlanguage-link interwiki-kn mw-list-item"><a href="https://kn.wikipedia.org/wiki/%E0%B2%97%E0%B3%81%E0%B2%B0%E0%B3%81_%E0%B2%97%E0%B3%8D%E0%B2%B0%E0%B2%B9%E0%B2%A6_%E0%B2%B5%E0%B2%BE%E0%B2%AF%E0%B3%81%E0%B2%AE%E0%B2%82%E0%B2%A1%E0%B2%B2" title="ಗುರು ಗ್ರಹದ ವಾಯುಮಂಡಲ – Kannada" lang="kn" hreflang="kn" data-title="ಗುರು ಗ್ರಹದ ವಾಯುಮಂಡಲ" data-language-autonym="ಕನ್ನಡ" data-language-local-name="Kannada" class="interlanguage-link-target">ಕನ್ನಡ</a></li><li class="interlanguage-link interwiki-mk mw-list-item"><a href="https://mk.wikipedia.org/wiki/%D0%90%D1%82%D0%BC%D0%BE%D1%81%D1%84%D0%B5%D1%80%D0%B0_%D0%BD%D0%B0_%D0%88%D1%83%D0%BF%D0%B8%D1%82%D0%B5%D1%80" title="Атмосфера на Јупитер – Macedonian" lang="mk" hreflang="mk" data-title="Атмосфера на Јупитер" data-language-autonym="Македонски" data-language-local-name="Macedonian" class="interlanguage-link-target">Македонски</a></li><li class="interlanguage-link interwiki-ja badge-Q17437798 badge-goodarticle mw-list-item" title="good article badge"><a href="https://ja.wikipedia.org/wiki/%E6%9C%A8%E6%98%9F%E3%81%AE%E5%A4%A7%E6%B0%97" title="木星の大気 – Japanese" lang="ja" hreflang="ja" data-title="木星の大気" data-language-autonym="日本語" data-language-local-name="Japanese" class="interlanguage-link-target">日本語</a></li><li class="interlanguage-link interwiki-no badge-Q17437796 badge-featuredarticle mw-list-item" title="featured article badge"><a href="https://no.wikipedia.org/wiki/Jupiters_atmosf%C3%A6re" title="Jupiters atmosfære – Norwegian Bokmål" lang="nb" hreflang="nb" data-title="Jupiters atmosfære" data-language-autonym="Norsk bokmål" data-language-local-name="Norwegian Bokmål" class="interlanguage-link-target">Norsk bokmål</a></li><li class="interlanguage-link interwiki-pt badge-Q17437796 badge-featuredarticle mw-list-item" title="featured article badge"><a href="https://pt.wikipedia.org/wiki/Atmosfera_de_J%C3%BApiter" title="Atmosfera de Júpiter – Portuguese" lang="pt" hreflang="pt" data-title="Atmosfera de Júpiter" data-language-autonym="Português" data-language-local-name="Portuguese" class="interlanguage-link-target">Português</a></li><li class="interlanguage-link interwiki-ro mw-list-item"><a href="https://ro.wikipedia.org/wiki/Atmosfera_lui_Jupiter" title="Atmosfera lui Jupiter – Romanian" lang="ro" hreflang="ro" data-title="Atmosfera lui Jupiter" data-language-autonym="Română" data-language-local-name="Romanian" class="interlanguage-link-target">Română</a></li><li class="interlanguage-link interwiki-ru badge-Q17437798 badge-goodarticle mw-list-item" title="good article badge"><a href="https://ru.wikipedia.org/wiki/%D0%90%D1%82%D0%BC%D0%BE%D1%81%D1%84%D0%B5%D1%80%D0%B0_%D0%AE%D0%BF%D0%B8%D1%82%D0%B5%D1%80%D0%B0" title="Атмосфера Юпитера – Russian" lang="ru" hreflang="ru" data-title="Атмосфера Юпитера" data-language-autonym="Русский" data-language-local-name="Russian" class="interlanguage-link-target">Русский</a></li><li class="interlanguage-link interwiki-simple mw-list-item"><a href="https://simple.wikipedia.org/wiki/Atmosphere_of_Jupiter" title="Atmosphere of Jupiter – Simple English" lang="en-simple" hreflang="en-simple" data-title="Atmosphere of Jupiter" data-language-autonym="Simple English" data-language-local-name="Simple English" class="interlanguage-link-target">Simple English</a></li><li class="interlanguage-link interwiki-sk mw-list-item"><a href="https://sk.wikipedia.org/wiki/Atmosf%C3%A9ra_Jupitera" title="Atmosféra Jupitera – Slovak" lang="sk" hreflang="sk" data-title="Atmosféra Jupitera" data-language-autonym="Slovenčina" data-language-local-name="Slovak" class="interlanguage-link-target">Slovenčina</a></li><li class="interlanguage-link interwiki-fi mw-list-item"><a href="https://fi.wikipedia.org/wiki/Jupiterin_pilvet" title="Jupiterin pilvet – Finnish" lang="fi" hreflang="fi" data-title="Jupiterin pilvet" data-language-autonym="Suomi" data-language-local-name="Finnish" class="interlanguage-link-target">Suomi</a></li><li class="interlanguage-link interwiki-tr mw-list-item"><a href="https://tr.wikipedia.org/wiki/J%C3%BCpiter%27in_atmosferi" title="Jüpiter'in atmosferi – Turkish" lang="tr" hreflang="tr" data-title="Jüpiter'in atmosferi" data-language-autonym="Türkçe" data-language-local-name="Turkish" class="interlanguage-link-target">Türkçe</a></li><li class="interlanguage-link interwiki-uk badge-Q17437796 badge-featuredarticle mw-list-item" title="featured article badge"><a href="https://uk.wikipedia.org/wiki/%D0%90%D1%82%D0%BC%D0%BE%D1%81%D1%84%D0%B5%D1%80%D0%B0_%D0%AE%D0%BF%D1%96%D1%82%D0%B5%D1%80%D0%B0" title="Атмосфера Юпітера – Ukrainian" lang="uk" hreflang="uk" data-title="Атмосфера Юпітера" data-language-autonym="Українська" data-language-local-name="Ukrainian" class="interlanguage-link-target">Українська</a></li><li class="interlanguage-link interwiki-vi badge-Q17437796 badge-featuredarticle mw-list-item" title="featured article badge"><a href="https://vi.wikipedia.org/wiki/Kh%C3%AD_quy%E1%BB%83n_Sao_M%E1%BB%99c" title="Khí quyển Sao Mộc – Vietnamese" lang="vi" hreflang="vi" data-title="Khí quyển Sao Mộc" data-language-autonym="Tiếng Việt" data-language-local-name="Vietnamese" class="interlanguage-link-target">Tiếng Việt</a></li><li class="interlanguage-link interwiki-zh mw-list-item"><a href="https://zh.wikipedia.org/wiki/%E6%9C%A8%E6%98%9F%E5%A4%A7%E6%B0%A3%E5%B1%A4" title="木星大氣層 – Chinese" lang="zh" hreflang="zh" data-title="木星大氣層" 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Click here for more information."><img alt="Featured article" src="//upload.wikimedia.org/wikipedia/en/thumb/e/e7/Cscr-featured.svg/20px-Cscr-featured.svg.png" decoding="async" width="20" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/en/thumb/e/e7/Cscr-featured.svg/30px-Cscr-featured.svg.png 1.5x, //upload.wikimedia.org/wikipedia/en/thumb/e/e7/Cscr-featured.svg/40px-Cscr-featured.svg.png 2x" data-file-width="466" data-file-height="443" /></a></div></div> </div> <div id="siteSub" class="noprint">From Wikipedia, the free encyclopedia</div> </div> <div id="contentSub"><div id="mw-content-subtitle"></div></div> <div id="mw-content-text" class="mw-body-content"><div class="mw-content-ltr mw-parser-output" lang="en" dir="ltr"><div class="shortdescription nomobile noexcerpt noprint searchaux" style="display:none">Layer of gases surrounding the planet Jupiter</div> <figure typeof="mw:File/Thumb"><a href="/wiki/File:Portrait_of_Jupiter_from_Cassini.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/300px-Portrait_of_Jupiter_from_Cassini.jpg" decoding="async" width="300" height="375" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/450px-Portrait_of_Jupiter_from_Cassini.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/600px-Portrait_of_Jupiter_from_Cassini.jpg 2x" data-file-width="1920" data-file-height="2400" /></a><figcaption>Jupiter's swirling clouds, in a <a href="/wiki/False_color#True_color" title="False color">true-color image</a> taken during fly-by of the <a href="/wiki/Cassini%E2%80%93Huygens" title="Cassini–Huygens">Cassini-Huygens probe</a> on 29th of December 29, 2000</figcaption></figure> The atmosphere of Jupiter is the largest <a href="/wiki/Planetary_atmosphere" class="mw-redirect" title="Planetary atmosphere">planetary atmosphere</a> in the <a href="/wiki/Solar_System" title="Solar System">Solar System</a>. It is mostly made of <a href="/wiki/Molecular_hydrogen" class="mw-redirect" title="Molecular hydrogen">molecular hydrogen</a> and <a href="/wiki/Helium" title="Helium">helium</a> in roughly <a href="/wiki/Sun#Composition" title="Sun">solar proportions</a>; other chemical compounds are present only in small amounts and include <a href="/wiki/Methane" title="Methane">methane</a>, <a href="/wiki/Ammonia" title="Ammonia">ammonia</a>, <a href="/wiki/Hydrogen_sulfide" title="Hydrogen sulfide">hydrogen sulfide</a>, and <a href="/wiki/Water" title="Water">water</a>. Although water is thought to reside deep in the atmosphere, its directly-measured concentration is very low. The <a href="/wiki/Nitrogen" title="Nitrogen">nitrogen</a>, <a href="/wiki/Sulfur" title="Sulfur">sulfur</a>, and <a href="/wiki/Noble_gas" title="Noble gas">noble gas</a> abundances in Jupiter's atmosphere exceed solar values by a factor of about three.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The atmosphere of <a href="/wiki/Jupiter" title="Jupiter">Jupiter</a> lacks a clear lower boundary and gradually transitions into the liquid interior of the planet.<a href="#cite_note-Guillot1999-2">[2]</a> From lowest to highest, the atmospheric layers are the <a href="/wiki/Troposphere" title="Troposphere">troposphere</a>, <a href="/wiki/Stratosphere" title="Stratosphere">stratosphere</a>, <a href="/wiki/Thermosphere" title="Thermosphere">thermosphere</a> and <a href="/wiki/Exosphere" title="Exosphere">exosphere</a>. Each layer has characteristic <a href="/wiki/Temperature_gradient" title="Temperature gradient">temperature gradients</a>.<a href="#cite_note-Sieff1998-3">[3]</a> The lowest layer, the troposphere, has a complicated system of clouds and hazes composed of layers of ammonia, <a href="/wiki/Ammonium_hydrosulfide" title="Ammonium hydrosulfide">ammonium hydrosulfide</a>, and water.<a href="#cite_note-FOOTNOTEAtreyaWong2005-4">[4]</a> The upper ammonia clouds visible at Jupiter's surface are organized in a dozen <a href="/wiki/Zonal_and_meridional" class="mw-redirect" title="Zonal and meridional">zonal</a> bands parallel to the <a href="/wiki/Equator" title="Equator">equator</a> and are bounded by powerful zonal atmospheric flows (winds) known as jets, exhibiting a phenomenon known as <a href="/wiki/Atmospheric_super-rotation" title="Atmospheric super-rotation">atmospheric super-rotation</a>. The bands alternate in color: the dark bands are called belts, while light ones are called zones. Zones, which are colder than belts, correspond to upwellings, while belts mark descending gas.<a href="#cite_note-Ingersoll1-5">[5]</a> The zones' lighter color is believed to result from ammonia ice; what gives the belts their darker colors is uncertain.<a href="#cite_note-Ingersoll1-5">[5]</a> The origins of the banded structure and jets are not well understood, though a "shallow model" and a "deep model" exist.<a href="#cite_note-1942Vasavada-6">[6]</a> <figure class="mw-default-size" typeof="mw:File/Thumb"><video id="mwe_player_0" poster="//upload.wikimedia.org/wikipedia/commons/thumb/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/220px--Jupiter_Cloud_Animation_from_Juno.webm.jpg" controls="" preload="none" data-mw-tmh="" class="mw-file-element" width="220" height="124" data-durationhint="9" data-mwtitle="Jupiter_Cloud_Animation_from_Juno.webm" data-mwprovider="wikimediacommons" resource="/wiki/File:Jupiter_Cloud_Animation_from_Juno.webm"><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.480p.vp9.webm" type="video/webm; codecs="vp9, opus"" data-transcodekey="480p.vp9.webm" data-width="854" data-height="480" /><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.720p.vp9.webm" type="video/webm; codecs="vp9, opus"" data-transcodekey="720p.vp9.webm" data-width="1280" data-height="720" /><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.1080p.vp9.webm" type="video/webm; codecs="vp9, opus"" data-transcodekey="1080p.vp9.webm" data-width="1920" data-height="1080" /><source src="//upload.wikimedia.org/wikipedia/commons/b/b7/Jupiter_Cloud_Animation_from_Juno.webm" type="video/webm; codecs="vp8, vorbis"" data-width="1920" data-height="1080" /><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.144p.mjpeg.mov" type="video/quicktime" data-transcodekey="144p.mjpeg.mov" data-width="256" data-height="144" /><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.240p.vp9.webm" type="video/webm; codecs="vp9, opus"" data-transcodekey="240p.vp9.webm" data-width="426" data-height="240" /><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.360p.webm" type="video/webm; codecs="vp8, vorbis"" data-transcodekey="360p.webm" data-width="640" data-height="360" /><source src="//upload.wikimedia.org/wikipedia/commons/transcoded/b/b7/Jupiter_Cloud_Animation_from_Juno.webm/Jupiter_Cloud_Animation_from_Juno.webm.360p.vp9.webm" type="video/webm; codecs="vp9, opus"" data-transcodekey="360p.vp9.webm" data-width="640" data-height="360" /></video><figcaption>False colored morphing animation of Jupiter's clouds in motion</figcaption></figure> The Jovian atmosphere shows a wide range of active phenomena, including band instabilities, vortices (<a href="/wiki/Cyclone" title="Cyclone">cyclones</a> and <a href="/wiki/Anticyclone" title="Anticyclone">anticyclones</a>), storms and lightning.<a href="#cite_note-1974Vasavada-7">[7]</a> The vortices reveal themselves as large red, white or brown spots (ovals). The largest two spots are the <a href="#Great_Red_Spot">Great Red Spot</a> (GRS)<a href="#cite_note-1978bVasavada-8">[8]</a> and <a href="#Oval_BA">Oval BA</a>,<a href="#cite_note-1980Vasavada-9">[9]</a> which is also red. These two and most of the other large spots are anticyclonic. Smaller <a href="/wiki/Anticyclone" title="Anticyclone">anticyclones</a> tend to be white. Vortices are thought to be relatively shallow structures with depths not exceeding several hundred kilometers. Located in the southern hemisphere, the GRS is the largest known vortex in the Solar System. It could engulf two or three Earths and has existed for at least three hundred years. Oval BA, south of GRS, is a red spot a third the size of GRS that formed in 2000 from the merging of three white ovals.<a href="#cite_note-1976Vasavada-10">[10]</a> Jupiter has powerful storms, often accompanied by lightning strikes. The storms are a result of moist convection in the atmosphere connected to the evaporation and condensation of water. They are sites of strong upward motion of the air, which leads to the formation of bright and dense clouds. The storms form mainly in belt regions. The lightning strikes on Jupiter are hundreds of times more powerful than those seen on Earth, and are assumed to be associated with the water clouds.<a href="#cite_note-11">[11]</a> Recent <a href="/wiki/Juno_(spacecraft)" title="Juno (spacecraft)">Juno</a> observations suggest Jovian lightning strikes occur above the altitude of water clouds (3-7 bars).<a href="#cite_note-:0-12">[12]</a> A charge separation between falling liquid ammonia-water droplets and water ice particles may generate higher-altitude lightning.<a href="#cite_note-:0-12">[12]</a> <a href="/wiki/Upper-atmospheric_lightning" title="Upper-atmospheric lightning">Upper-atmospheric lightning</a> has also been observed 260 km above the 1 bar level.<a href="#cite_note-13">[13]</a> <meta property="mw:PageProp/toc" /> <div class="mw-heading mw-heading2"><h2 id="Vertical_structure">Vertical structure</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=1" title="Edit section: Vertical structure">edit</a>]</div> <figure typeof="mw:File/Thumb"><a href="/wiki/File:Structure_of_Jovian_atmosphere.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f5/Structure_of_Jovian_atmosphere.png/400px-Structure_of_Jovian_atmosphere.png" decoding="async" width="400" height="258" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f5/Structure_of_Jovian_atmosphere.png/600px-Structure_of_Jovian_atmosphere.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f5/Structure_of_Jovian_atmosphere.png/800px-Structure_of_Jovian_atmosphere.png 2x" data-file-width="3000" data-file-height="1934" /></a><figcaption>Vertical structure of the atmosphere of Jupiter. Note that the temperature drops together with altitude above the tropopause. The <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo atmospheric probe</a> stopped transmitting at a depth of 132 km below the 1 bar "surface" of Jupiter.<a href="#cite_note-Sieff1998-3">[3]</a></figcaption></figure> The atmosphere of Jupiter is classified into four layers, by increasing altitude: the <a href="/wiki/Troposphere" title="Troposphere">troposphere</a>, <a href="/wiki/Stratosphere" title="Stratosphere">stratosphere</a>, <a href="/wiki/Thermosphere" title="Thermosphere">thermosphere</a> and <a href="/wiki/Exosphere" title="Exosphere">exosphere</a>. Unlike the <a href="/wiki/Earth%27s_atmosphere" class="mw-redirect" title="Earth's atmosphere">Earth's atmosphere</a>, Jupiter's lacks a <a href="/wiki/Mesosphere" title="Mesosphere">mesosphere</a>.<a href="#cite_note-Ingersoll7-14">[14]</a> Jupiter does not have a solid surface, and the lowest atmospheric layer, the troposphere, smoothly transitions into the planet's fluid interior.<a href="#cite_note-Guillot1999-2">[2]</a> This is a result of having temperatures and the pressures well above those of the <a href="/wiki/Critical_point_(thermodynamics)" title="Critical point (thermodynamics)">critical points</a> for hydrogen and helium, meaning that there is no sharp boundary between gas and liquid phases. Hydrogen is considered a <a href="/wiki/Supercritical_fluid" title="Supercritical fluid">supercritical fluid</a> when the temperature is above 33 K and the pressure is above 13 bar.<a href="#cite_note-Guillot1999-2">[2]</a> Since the lower boundary of the atmosphere is ill-defined, the pressure level of 10 <a href="/wiki/Bar_(unit)" title="Bar (unit)">bars</a>, at an altitude of about 90 km below 1 bar with a temperature of around 340 <a href="/wiki/Kelvin" title="Kelvin">K</a>, is commonly treated as the base of the troposphere.<a href="#cite_note-Sieff1998-3">[3]</a> In scientific literature, the 1 bar pressure level is usually chosen as a zero point for altitudes—a "surface" of Jupiter.<a href="#cite_note-Guillot1999-2">[2]</a> As is generally the case, the top atmospheric layer, the exosphere, does not have a specific upper boundary.<a href="#cite_note-Yelle1-15">[15]</a> The density gradually decreases until it smoothly transitions into the <a href="/wiki/Interplanetary_medium" title="Interplanetary medium">interplanetary medium</a> approximately 5,000 km above the "surface".<a href="#cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">[16]</a> The vertical temperature gradients in the Jovian atmosphere are similar to those of the <a href="/wiki/Atmosphere_of_Earth" title="Atmosphere of Earth">atmosphere of Earth</a>. The temperature of the troposphere decreases with height until it reaches a minimum at the <a href="/wiki/Tropopause" title="Tropopause">tropopause</a>,<a href="#cite_note-Ingersoll4-17">[17]</a> which is the boundary between the troposphere and stratosphere. On Jupiter, the tropopause is approximately 50 km above the visible clouds (or 1 bar level). The pressure and temperature at the tropopause are about 0.1 bar and 110 K.<a href="#cite_note-Sieff1998-3">[3]</a><a href="#cite_note-Ingersoll3-18">[18]</a> (This gives a drop of 340−110=230 °C over 90+50=140 km. The adiabatic <a href="/wiki/Lapse_rate" title="Lapse rate">lapse rate</a> on Earth is around 9.8 °C per km. The adiabatic lapse rate is proportional to the average molecular weight and the <a href="/wiki/Surface_gravity" title="Surface gravity">gravitational force</a>. The latter is about 2.5 times stronger than on Earth, but the average molecular weight is about 15 times less.) In the stratosphere, the temperatures rise to about 200 K at the transition into the thermosphere, at an altitude and pressure of around 320 km and 1 μbar.<a href="#cite_note-Sieff1998-3">[3]</a> In the thermosphere, temperatures continue to rise, eventually reaching 1000 K at about 1000 km, where pressure is about 1 nbar.<a href="#cite_note-Yelle3-19">[19]</a> Jupiter's troposphere contains a complicated cloud structure.<a href="#cite_note-FOOTNOTEAtreya_Wong_Baines_et_al.2005-20">[20]</a> The upper clouds, located in the pressure range 0.6–0.9 bar, are made of ammonia ice.<a href="#cite_note-FOOTNOTEAtreya_Wong_Owen_et_al.1999-21">[21]</a> Below these ammonia ice clouds, denser clouds made of <a href="/wiki/Ammonium_hydrosulfide" title="Ammonium hydrosulfide">ammonium hydrosulfide</a> ((NH4)SH) or <a href="/wiki/Ammonium_sulfide" class="mw-redirect" title="Ammonium sulfide">ammonium sulfide</a> ((NH4)2S, between 1–2 bar) and water (3–7 bar) are thought to exist.<a href="#cite_note-West20-22">[22]</a><a href="#cite_note-1937Vasavada-23">[23]</a> There are no methane clouds as the temperatures are too high for it to condense.<a href="#cite_note-FOOTNOTEAtreya_Wong_Baines_et_al.2005-20">[20]</a> The water clouds form the densest layer of clouds and have the strongest influence on the dynamics of the atmosphere. This is a result of the higher <a href="/wiki/Heat_of_vaporization" class="mw-redirect" title="Heat of vaporization">condensation heat</a> of water and higher water abundance as compared to the ammonia and hydrogen sulfide (oxygen is a more <a href="/wiki/Abundance_of_the_chemical_elements" title="Abundance of the chemical elements">abundant</a> chemical element than either nitrogen or sulfur).<a href="#cite_note-Ingersoll7-14">[14]</a> Various tropospheric (at 200–500 mbar) and stratospheric (at 10–100 mbar) haze layers reside above the main cloud layers.<a href="#cite_note-West20-22">[22]</a><a href="#cite_note-Ingersoll8-24">[24]</a> The stratospheric haze layers are made from condensed heavy <a href="/wiki/Polycyclic_aromatic_hydrocarbon" title="Polycyclic aromatic hydrocarbon">polycyclic aromatic hydrocarbons</a> or <a href="/wiki/Hydrazine" title="Hydrazine">hydrazine</a>, which are generated in the upper stratosphere (1–100 μbar) from methane under the influence of the solar ultraviolet radiation (UV).<a href="#cite_note-FOOTNOTEAtreya_Wong_Baines_et_al.2005-20">[20]</a> The methane abundance relative to molecular hydrogen in the stratosphere is about 10−4,<a href="#cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">[16]</a> while the abundance ratio of other light hydrocarbons, like ethane and acetylene, to molecular hydrogen is about 10−6.<a href="#cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">[16]</a> Jupiter's thermosphere is located at pressures lower than 1 μbar and demonstrates such phenomena as <a href="/wiki/Airglow" title="Airglow">airglow</a>, polar <a href="/wiki/Aurora_(astronomy)" class="mw-redirect" title="Aurora (astronomy)">aurorae</a> and <a href="/wiki/X-ray" title="X-ray">X-ray</a> emissions.<a href="#cite_note-Yelle2-25">[25]</a> Within it lie layers of increased electron and ion density that form the <a href="/wiki/Ionosphere" title="Ionosphere">ionosphere</a>.<a href="#cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">[16]</a> The high temperatures prevalent in the thermosphere (800–1000 K) have not been explained yet;<a href="#cite_note-Yelle3-19">[19]</a> existing models predict a temperature no higher than about 400 K.<a href="#cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">[16]</a> They may be caused by absorption of high-energy solar radiation (UV or X-ray), by heating from the charged particles precipitating from the Jovian magnetosphere, or by dissipation of upward-propagating <a href="/wiki/Gravity_wave" title="Gravity wave">gravity waves</a>.<a href="#cite_note-Yelle4-26">[26]</a> The thermosphere and exosphere at the poles and at low latitudes emit X-rays, which were first observed by the <a href="/wiki/Einstein_Observatory" title="Einstein Observatory">Einstein Observatory</a> in 1983.<a href="#cite_note-FOOTNOTEBhardwajGladstone2000299–302-27">[27]</a> The energetic particles coming from Jupiter's magnetosphere create bright auroral ovals, which encircle the poles. Unlike their terrestrial analogs, which appear only during <a href="/wiki/Magnetic_storm" class="mw-redirect" title="Magnetic storm">magnetic storms</a>, aurorae are permanent features of Jupiter's atmosphere.<a href="#cite_note-FOOTNOTEBhardwajGladstone2000299–302-27">[27]</a> The thermosphere was the first place outside the Earth where the <a href="/wiki/Trihydrogen_cation" title="Trihydrogen cation">trihydrogen cation</a> (H+ 3) was discovered.<a href="#cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">[16]</a> This ion emits strongly in the mid-infrared part of the spectrum, at wavelengths between 3 and 5 μm; this is the main cooling mechanism of the thermosphere.<a href="#cite_note-Yelle2-25">[25]</a> <div class="mw-heading mw-heading2"><h2 id="Chemical_composition">Chemical composition</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=2" title="Edit section: Chemical composition">edit</a>]</div> <div style="float: right; margin-left: 1em; width: 25em;"> <table class="wikitable" style="text-align: center; margin-right: 0; width: 100%;"> <caption>Elemental abundances relative to hydrogen in Jupiter and Sun<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> </caption> <tbody><tr> <th>Element</th> <th>Sun</th> <th>Jupiter/Sun </th></tr> <tr> <td><a href="/wiki/Helium" title="Helium">He</a>/<a href="/wiki/Hydrogen" title="Hydrogen">H</a></td> <td>0.0975</td> <td>0.807 ± 0.02 </td></tr> <tr> <td><a href="/wiki/Neon" title="Neon">Ne</a>/H</td> <td>1.23 × 10−4</td> <td>0.10 ± 0.01 </td></tr> <tr> <td><a href="/wiki/Argon" title="Argon">Ar</a>/H</td> <td>3.62 × 10−6</td> <td>2.5 ± 0.5 </td></tr> <tr> <td><a href="/wiki/Krypton" title="Krypton">Kr</a>/H</td> <td>1.61 × 10−9</td> <td>2.7 ± 0.5 </td></tr> <tr> <td><a href="/wiki/Xenon" title="Xenon">Xe</a>/H</td> <td>1.68 × 10−10</td> <td>2.6 ± 0.5 </td></tr> <tr> <td><a href="/wiki/Carbon" title="Carbon">C</a>/H</td> <td>3.62 × 10−4</td> <td>2.9 ± 0.5 </td></tr> <tr> <td><a href="/wiki/Nitrogen" title="Nitrogen">N</a>/H</td> <td>1.12 × 10−4 </td> <td>3.6 ± 0.5 (8 bar) 3.2 ± 1.4 (9–12 bar) </td></tr> <tr> <td><a href="/wiki/Oxygen" title="Oxygen">O</a>/H</td> <td>8.51 × 10−4 </td> <td>0.033 ± 0.015 (12 bar) 0.19–0.58 (19 bar) </td></tr> <tr> <td><a href="/wiki/Phosphorus" title="Phosphorus">P</a>/H</td> <td>3.73 × 10−7</td> <td>0.82 </td></tr> <tr> <td><a href="/wiki/Sulfur" title="Sulfur">S</a>/H</td> <td>1.62 × 10−5</td> <td>2.5 ± 0.15 </td></tr></tbody></table> <table class="wikitable" style="text-align: center; margin-right: 0; width: 100%;"> <caption>Isotopic ratios in Jupiter and Sun<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> </caption> <tbody><tr> <th>Ratio</th> <th>Sun</th> <th>Jupiter </th></tr> <tr> <td><a href="/wiki/Carbon-13" title="Carbon-13">13C</a>/<a href="/wiki/Carbon-12" title="Carbon-12">12C</a></td> <td>0.011</td> <td>0.0108 ± 0.0005 </td></tr> <tr> <td><a href="/wiki/Nitrogen-15" class="mw-redirect" title="Nitrogen-15">15N</a>/<a href="/wiki/Nitrogen-14" class="mw-redirect" title="Nitrogen-14">14N</a></td> <td><2.8 × 10−3</td> <td>2.3 ± 0.3 × 10−3 (0.08–2.8 bar) </td></tr> <tr> <td><a href="/wiki/Argon-36" class="mw-redirect" title="Argon-36">36Ar</a>/<a href="/wiki/Argon-38" class="mw-redirect" title="Argon-38">38Ar</a></td> <td>5.77 ± 0.08</td> <td>5.6 ± 0.25 </td></tr> <tr> <td><a href="/wiki/Neon-20" class="mw-redirect" title="Neon-20">20Ne</a>/<a href="/wiki/Neon-22" class="mw-redirect" title="Neon-22">22Ne</a></td> <td>13.81 ± 0.08</td> <td>13 ± 2 </td></tr> <tr> <td><a href="/wiki/Helium-3" title="Helium-3">3He</a>/<a href="/wiki/Helium-4" title="Helium-4">4He</a></td> <td>1.5 ± 0.3 × 10−4</td> <td>1.66 ± 0.05 × 10−4 </td></tr> <tr> <td><a href="/wiki/Deuterium" title="Deuterium">D</a>/<a href="/wiki/Hydrogen-1" class="mw-redirect" title="Hydrogen-1">H</a></td> <td>3.0 ± 0.17 × 10−5</td> <td>2.25 ± 0.35 × 10−5 </td></tr></tbody></table> </div> The composition of Jupiter's atmosphere is similar to that of the planet as a whole.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> Jupiter's atmosphere is the most comprehensively understood of those of all the <a href="/wiki/Giant_planet" title="Giant planet">giant planets</a> because it was observed directly by the <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo atmospheric probe</a> when it entered the Jovian atmosphere on December 7, 1995.<a href="#cite_note-28">[28]</a> Other sources of information about Jupiter's atmospheric composition include the <a href="/wiki/Infrared_Space_Observatory" title="Infrared Space Observatory">Infrared Space Observatory</a> (ISO),<a href="#cite_note-FOOTNOTEEncrenaz2003-29">[29]</a> the <a href="/wiki/Galileo_(spacecraft)" title="Galileo (spacecraft)">Galileo</a> and <a href="/wiki/Cassini_(spacecraft)" class="mw-redirect" title="Cassini (spacecraft)">Cassini</a> orbiters,<a href="#cite_note-Kunde2004-30">[30]</a> and Earth-based observations.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The two main constituents of the Jovian atmosphere are <a href="/wiki/Molecular_hydrogen" class="mw-redirect" title="Molecular hydrogen">molecular hydrogen</a> (H 2) and <a href="/wiki/Helium" title="Helium">helium</a>.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The helium abundance is 0.157 ± 0.004 relative to molecular hydrogen by number of molecules, and its mass fraction is 0.234 ± 0.005, which is slightly lower than the Solar System's <a href="/wiki/Primordial_element" class="mw-redirect" title="Primordial element">primordial</a> value.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The reason for this low abundance is not entirely understood, but some of the helium may have condensed into the core of Jupiter.<a href="#cite_note-FOOTNOTEAtreya_Wong_Owen_et_al.1999-21">[21]</a> This condensation is likely to be in the form of helium rain: as hydrogen turns into the <a href="/wiki/Metallic_hydrogen" title="Metallic hydrogen">metallic state</a> at depths of more than 10,000 km, helium separates from it forming droplets which, being denser than the metallic hydrogen, descend towards the core. This can also explain the severe depletion of neon (see Table), an element that easily dissolves in helium droplets and would be transported in them towards the core as well.<a href="#cite_note-Sanders2010-31">[31]</a> The atmosphere contains various simple compounds such as <a href="/wiki/Water" title="Water">water</a>, <a href="/wiki/Methane" title="Methane">methane</a> (CH4), <a href="/wiki/Hydrogen_sulfide" title="Hydrogen sulfide">hydrogen sulfide</a> (H2S), <a href="/wiki/Ammonia" title="Ammonia">ammonia</a> (NH3) and <a href="/wiki/Phosphine" title="Phosphine">phosphine</a> (PH3).<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> Their abundances in the deep (below 10 bar) troposphere imply that the atmosphere of Jupiter is enriched in the elements <a href="/wiki/Carbon" title="Carbon">carbon</a>, <a href="/wiki/Nitrogen" title="Nitrogen">nitrogen</a>, <a href="/wiki/Sulfur" title="Sulfur">sulfur</a> and possibly <a href="/wiki/Oxygen" title="Oxygen">oxygen</a><style data-mw-deduplicate="TemplateStyles:r1041539562">.mw-parser-output .citation{word-wrap:break-word}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}</style><a href="#endnote_Bnone">[b]</a> by a factor of 2–4 relative to the Sun.<link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#endnote_Cnone">[c]</a><a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The noble gases <a href="/wiki/Argon" title="Argon">argon</a>, <a href="/wiki/Krypton" title="Krypton">krypton</a> and <a href="/wiki/Xenon" title="Xenon">xenon</a> also appear in abundance relative to solar levels (see table), while <a href="/wiki/Neon" title="Neon">neon</a> is scarcer.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> Other chemical compounds such as <a href="/wiki/Arsine" title="Arsine">arsine</a> (AsH3) and <a href="/wiki/Germane" title="Germane">germane</a> (GeH4) are present only in trace amounts.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The upper atmosphere of Jupiter contains small amounts of simple <a href="/wiki/Hydrocarbon" title="Hydrocarbon">hydrocarbons</a> such as <a href="/wiki/Ethane" title="Ethane">ethane</a>, <a href="/wiki/Acetylene" title="Acetylene">acetylene</a>, and <a href="/wiki/Diacetylene" title="Diacetylene">diacetylene</a>, which form from methane under the influence of the solar <a href="/wiki/Ultraviolet_radiation" class="mw-redirect" title="Ultraviolet radiation">ultraviolet radiation</a> and charged particles coming from <a href="/wiki/Jupiter#Magnetosphere" title="Jupiter">Jupiter's magnetosphere</a>.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The <a href="/wiki/Carbon_dioxide" title="Carbon dioxide">carbon dioxide</a>, <a href="/wiki/Carbon_monoxide" title="Carbon monoxide">carbon monoxide</a> and water present in the upper atmosphere are thought to originate from impacting <a href="/wiki/Comet" title="Comet">comets</a>, such as <a href="/wiki/Comet_Shoemaker-Levy_9" class="mw-redirect" title="Comet Shoemaker-Levy 9">Shoemaker-Levy 9</a>. The water cannot come from the troposphere because the cold <a href="/wiki/Tropopause" title="Tropopause">tropopause</a> acts like a cold trap, effectively preventing water from rising to the <a href="/wiki/Stratosphere" title="Stratosphere">stratosphere</a> (see Vertical structure above).<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> Earth- and spacecraft-based measurements have led to improved knowledge of the <a href="/wiki/Isotope_geochemistry" title="Isotope geochemistry">isotopic ratios</a> in Jupiter's atmosphere. As of July 2003, the accepted value for the <a href="/wiki/Deuterium" title="Deuterium">deuterium</a> abundance is (2.25 ± 0.35) × 10−5,<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> which probably represents the primordial value in the <a href="/wiki/Nebular_hypothesis" title="Nebular hypothesis">protosolar nebula</a> that gave birth to the Solar System.<a href="#cite_note-FOOTNOTEEncrenaz2003-29">[29]</a> The ratio of nitrogen isotopes in the Jovian atmosphere, <a href="/wiki/Nitrogen-15" class="mw-redirect" title="Nitrogen-15">15N</a> to <a href="/wiki/Nitrogen-14" class="mw-redirect" title="Nitrogen-14">14N</a>, is 2.3 × 10−3, a third lower than that in the <a href="/wiki/Earth%27s_atmosphere" class="mw-redirect" title="Earth's atmosphere">Earth's atmosphere</a> (3.5 × 10−3).<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> The latter discovery is especially significant since the previous theories of <a href="/wiki/Formation_and_evolution_of_the_Solar_System" title="Formation and evolution of the Solar System">Solar System formation</a> considered the terrestrial value for the ratio of nitrogen isotopes to be primordial.<a href="#cite_note-FOOTNOTEEncrenaz2003-29">[29]</a> <div class="mw-heading mw-heading2"><h2 id="Zones,_belts_and_jets">Zones, belts and jets</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=3" title="Edit section: Zones, belts and jets">edit</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Map_of_Jupiter.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/d/d3/Map_of_Jupiter.jpg/220px-Map_of_Jupiter.jpg" decoding="async" width="220" height="223" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d3/Map_of_Jupiter.jpg/330px-Map_of_Jupiter.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d3/Map_of_Jupiter.jpg/440px-Map_of_Jupiter.jpg 2x" data-file-width="2231" data-file-height="2266" /></a><figcaption>A polar <a href="/wiki/Stereographic_projection" title="Stereographic projection">stereographic projection</a> of Jupiter's atmosphere centered about Jupiter's south pole</figcaption></figure> The visible surface of Jupiter is divided into several bands parallel to the equator. There are two types of bands: lightly colored zones and relatively dark belts.<a href="#cite_note-Ingersoll1-5">[5]</a> The wider <a href="/wiki/Equator" title="Equator">Equatorial Zone</a> (EZ) extends between <a href="/wiki/Latitude" title="Latitude">latitudes</a> of approximately 7°S to 7°N. Above and below the EZ, the North and South Equatorial belts (NEB and SEB) extend to 18°N and 18°S, respectively. Farther from the equator lie the North and South Tropical zones (NtrZ and STrZ).<a href="#cite_note-Ingersoll1-5">[5]</a> The alternating pattern of belts and zones continues until the polar regions at approximately 50 degrees latitude, where their visible appearance becomes somewhat muted.<a href="#cite_note-Rogers1-32">[32]</a> The difference in the appearance between zones and belts is caused by differences in the opacity of the clouds. Ammonia concentration is higher in zones, which leads to the appearance of denser clouds of ammonia ice at higher altitudes, which in turn leads to their lighter color.<a href="#cite_note-Ingersoll4-17">[17]</a> On the other hand, in belts clouds are thinner and are located at lower altitudes.<a href="#cite_note-Ingersoll4-17">[17]</a> The upper troposphere is colder in zones and warmer in belts.<a href="#cite_note-Ingersoll1-5">[5]</a> The exact nature of chemicals that make Jovian zones and bands so colorful is not known, but they may include complicated compounds of <a href="/wiki/Sulfur" title="Sulfur">sulfur</a>, <a href="/wiki/Phosphorus" title="Phosphorus">phosphorus</a> and <a href="/wiki/Carbon" title="Carbon">carbon</a>.<a href="#cite_note-Ingersoll1-5">[5]</a> The Jovian bands are bounded by zonal atmospheric flows (winds), called <a href="/wiki/Jet_stream" title="Jet stream">jets</a>. The eastward (<a href="/wiki/Direct_motion" class="mw-redirect" title="Direct motion">prograde</a>) jets are found at the transition from zones to belts (going away from the equator), whereas westward (<a href="/wiki/Retrograde_and_direct_motion" class="mw-redirect" title="Retrograde and direct motion">retrograde</a>) jets mark the transition from belts to zones.<a href="#cite_note-Ingersoll1-5">[5]</a> Such flow velocity patterns mean that the jets' eastward momentum decreases in belts and increases in zones from the equator to the pole. Therefore, <a href="/wiki/Wind_shear" title="Wind shear">wind shear</a> in belts is <a href="/wiki/Cyclone" title="Cyclone">cyclonic</a>, while in zones it is <a href="/wiki/Anticyclone" title="Anticyclone">anticyclonic</a>.<a href="#cite_note-1937Vasavada-23">[23]</a> The EZ is an exception to this rule, showing a strong eastward (prograde) jet and has a local minimum of the wind speed exactly at the equator. The jet speeds are high on Jupiter, reaching more than 100 m/s.<a href="#cite_note-Ingersoll1-5">[5]</a> These speeds correspond to ammonia clouds located in the pressure range 0.7–1 bar. The prograde jets are generally more powerful than the retrograde jets.<a href="#cite_note-Ingersoll1-5">[5]</a> The jets extend thousands of kilometers into the interior, as measured by the gravitometer instrument onboard of the <a href="/wiki/Juno_(spacecraft)" title="Juno (spacecraft)">Juno spacecraft</a>.<a href="#cite_note-33">[33]</a> The direction at which the jets extend into the planet is parallel to Jupiter's <a href="/wiki/Rotation_around_a_fixed_axis" title="Rotation around a fixed axis">axis of rotation</a><a href="#cite_note-34">[34]</a> rather than in a radial direction (toward the center of the planet), consistent with the <a href="/wiki/Taylor-Proudman_theorem" class="mw-redirect" title="Taylor-Proudman theorem">Taylor-Proudman theorem</a>.<a href="#cite_note-35">[35]</a> The <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo Probe</a> measured the vertical profile of a jet along its descent trajectory into Jupiter's atmosphere, finding the winds to decay over two to three <a href="/wiki/Scale_height" title="Scale height">scale heights</a><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#endnote_Anone">[a]</a> above the clouds, while below the cloud level, winds increase slightly and then remain constant down to at least 22 bar—the maximum operational depth reached by the probe.<a href="#cite_note-Ingersoll3-18">[18]</a> <figure class="mw-default-size mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:Wind_speeds_on_Jupiter.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Wind_speeds_on_Jupiter.png/220px-Wind_speeds_on_Jupiter.png" decoding="async" width="220" height="154" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Wind_speeds_on_Jupiter.png/330px-Wind_speeds_on_Jupiter.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Wind_speeds_on_Jupiter.png/440px-Wind_speeds_on_Jupiter.png 2x" data-file-width="3000" data-file-height="2105" /></a><figcaption>Zonal wind speeds in the atmosphere of Jupiter</figcaption></figure> The origin of Jupiter's colored banded structure is not completely clear, though it may resemble the cloud structure of Earth's <a href="/wiki/Hadley_cell" title="Hadley cell">Hadley cells</a>. The simplest interpretation is that zones are sites of atmospheric <a href="/wiki/Upwelling" title="Upwelling">upwelling</a>, whereas belts are manifestations of <a href="/wiki/Downwelling" title="Downwelling">downwelling</a>.<a href="#cite_note-Ingersoll2-36">[36]</a> When air enriched in ammonia rises in zones, it expands and cools, forming high and dense white clouds. In belts, however, the air descends, warming <a href="/wiki/Adiabatic_process" title="Adiabatic process">adiabatically</a> as in a <a href="/wiki/Convergence_zone" title="Convergence zone">convergence zone</a> on Earth, and white ammonia clouds evaporate, revealing lower, darker clouds. The location and width of bands, speed and location of jets on Jupiter are remarkably stable, having changed only slightly between 1980 and 2000. One example of change is a decrease of the speed of the strongest eastward jet located at the boundary between the North Tropical zone and North Temperate belts at 23°N.<a href="#cite_note-1942Vasavada-6">[6]</a><a href="#cite_note-Ingersoll2-36">[36]</a> However bands vary in coloration and intensity over time (see "specific band"). These variations were first observed in the early seventeenth century.<a href="#cite_note-37">[37]</a> <div class="mw-heading mw-heading3"><h3 id="Meridional_circulation_cells">Meridional circulation cells</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=4" title="Edit section: Meridional circulation cells">edit</a>]</div> <a href="/wiki/Atmospheric_circulation" title="Atmospheric circulation">Meridional circulation cells</a> are a large-scale atmospheric motion where gas rises at a certain latitude, travel in the north-south (meridional) direction, descends, and get back to the origin in a closed cell circulation.<a href="#cite_note-38">[38]</a> On Earth, the meridional circulation is composed of 3 cells in each hemisphere: <a href="/wiki/Hadley_cell" title="Hadley cell">Hadley</a>, <a href="/wiki/Ferrel_cell" class="mw-redirect" title="Ferrel cell">Ferrel</a> and <a href="/wiki/Polar_cells" class="mw-redirect" title="Polar cells">Polar</a> cells. On Jupiter, the visible cloud bands gave indication for upward motion in the zones and downward motion in the belts, indicative only for the upper few bars.<a href="#cite_note-39">[39]</a> However, higher frequency of lightning flashes in the belts, indicative of upward atmospheric motion, gave indication for a reversed motion in the deeper atmosphere.<a href="#cite_note-40">[40]</a><a href="#cite_note-41">[41]</a> Juno's microwave measurements probe the atmosphere down to ~240 bar.<a href="#cite_note-42">[42]</a> These measurements confirmed the existence of these motions as a part of mid-latitudes large circulation cells with upward motion in the belts and downward motions in the zones, extending from ~1 bar down to at least ~240 bar.<a href="#cite_note-:2-43">[43]</a> So far, 8 cells have been identified at each of Jupiter's hemispheres along latitudes 20°-60° N\S.<a href="#cite_note-:2-43">[43]</a> The mid-latitude cells are driven by breaking of <a href="/wiki/Rossby_wave" title="Rossby wave">atmospheric waves</a>, similar to the Ferrel cells on Earth.<a href="#cite_note-:2-43">[43]</a> While on Earth, the return flow in the cells' lower branch is balanced by friction in the <a href="/wiki/Ekman_layer" title="Ekman layer">Ekman layer</a>, the balance in Jupiter in yet unknown, but one possibility is that the friction is maintained by magnetic drag.<a href="#cite_note-44">[44]</a> <div class="mw-heading mw-heading3"><h3 id="Specific_bands">Specific bands</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=5" title="Edit section: Specific bands">edit</a>]</div> <figure typeof="mw:File/Thumb"><a href="/wiki/File:Jupiter_cloud_bands.svg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/23/Jupiter_cloud_bands.svg/300px-Jupiter_cloud_bands.svg.png" decoding="async" width="300" height="220" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/23/Jupiter_cloud_bands.svg/450px-Jupiter_cloud_bands.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/23/Jupiter_cloud_bands.svg/600px-Jupiter_cloud_bands.svg.png 2x" data-file-width="522" data-file-height="382" /></a><figcaption>Idealized illustration of Jupiter's cloud bands, labeled with their official abbreviations. Lighter zones are indicated to the right, darker belts to the left. The Great Red Spot and Oval BA are shown in the South Tropical Zone and South Temperate Belt, respectively.</figcaption></figure> The belts and zones that divide Jupiter's atmosphere each have their own names and unique characteristics. They begin below the North and South Polar Regions, which extend from the poles to roughly 40–48° N/S. These bluish-gray regions are usually featureless.<a href="#cite_note-Rogers1-32">[32]</a> The North North Temperate Region rarely shows more detail than the polar regions, due to <a href="/wiki/Limb_darkening" title="Limb darkening">limb darkening</a>, <a href="/wiki/Foreshortening" class="mw-redirect" title="Foreshortening">foreshortening</a>, and the general diffuseness of features. However, the North-North Temperate Belt (NNTB) is the northernmost distinct belt, though it occasionally disappears. Disturbances tend to be minor and short-lived. The North-North Temperate Zone (NNTZ) is perhaps more prominent, but also generally quiet. Other minor belts and zones in the region are occasionally observed.<a href="#cite_note-45">[45]</a> The North Temperate Region is part of a latitudinal region easily observable from Earth, and thus has a superb record of observation.<a href="#cite_note-Rogers2-46">[46]</a> It also features the strongest <a href="/wiki/Direct_motion" class="mw-redirect" title="Direct motion">prograde</a> <a href="/wiki/Jet_stream" title="Jet stream">jet stream</a> on the planet—a westerly current that forms the southern boundary of the North Temperate Belt (NTB).<a href="#cite_note-Rogers2-46">[46]</a> The NTB fades roughly once a decade (this was the case during the Voyager encounters), making the North Temperate Zone (NTZ) apparently merge into the North Tropical Zone (NTropZ).<a href="#cite_note-Rogers2-46">[46]</a> Other times, the NTZ is divided by a narrow belt into northern and southern components.<a href="#cite_note-Rogers2-46">[46]</a> The North Tropical Region is composed of the NTropZ and the North Equatorial Belt (NEB). The NTropZ is generally stable in coloration, changing in tint only in tandem with activity on the NTB's southern jet stream. Like the NTZ, it too is sometimes divided by a narrow band, the NTropB. On rare occasions, the southern NTropZ plays host to "Little Red Spots". As the name suggests, these are northern equivalents of the Great Red Spot. Unlike the GRS, they tend to occur in pairs and are always short-lived, lasting a year on average; one was present during the <a href="/wiki/Pioneer_10" title="Pioneer 10">Pioneer 10</a> encounter.<a href="#cite_note-47">[47]</a> The NEB is one of the most active belts on the planet. It is characterized by anticyclonic white ovals and cyclonic "barges" (also known as "brown ovals"), with the former usually forming farther north than the latter; as in the NTropZ, most of these features are relatively short-lived. Like the South Equatorial Belt (SEB), the NEB has sometimes dramatically faded and "revived". The timescale of these changes is about 25 years.<a href="#cite_note-48">[48]</a> <figure typeof="mw:File/Thumb"><a href="/wiki/File:PIA02863_-_Jupiter_surface_motion_animation.gif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/76/PIA02863_-_Jupiter_surface_motion_animation.gif/500px-PIA02863_-_Jupiter_surface_motion_animation.gif" decoding="async" width="500" height="167" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/76/PIA02863_-_Jupiter_surface_motion_animation.gif/750px-PIA02863_-_Jupiter_surface_motion_animation.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/76/PIA02863_-_Jupiter_surface_motion_animation.gif/1000px-PIA02863_-_Jupiter_surface_motion_animation.gif 2x" data-file-width="1799" data-file-height="600" /></a><figcaption>Zones, belts and vortices on Jupiter. The wide equatorial zone is visible in the center surrounded by two dark equatorial belts (SEB and NEB). The large grayish-blue irregular "hot spots" at the northern edge of the white Equatorial Zone change over the course of time as they march eastward across the planet. The Great Red Spot is at the southern margin of the SEB. Strings of small storms rotate around northern-hemisphere ovals. Small, very bright features, possible lightning storms, appear quickly and randomly in turbulent regions. The smallest features visible at the equator are about 600 kilometers across. This 14-frame animation spans 24 Jovian days, or about 10 Earth days. The passage of time is accelerated by a factor of 600,000. The occasional black spots in the image are <a href="/wiki/Moons_of_Jupiter" title="Moons of Jupiter">moons of Jupiter</a> getting into the field of view.</figcaption></figure> The Equatorial Region (EZ) is one of the most stable regions of the planet, in latitude and in activity. The northern edge of the EZ hosts spectacular plumes that trail southwest from the NEB, which are bounded by dark, warm (in <a href="/wiki/Infrared" title="Infrared">infrared</a>) features known as festoons (hot spots).<a href="#cite_note-1987Vasavada-49">[49]</a> Though the southern boundary of the EZ is usually quiescent, observations from the late 19th into the early 20th century show that this pattern was then reversed relative to today. The EZ varies considerably in coloration, from pale to an <a href="/wiki/Ochre" title="Ochre">ochre</a>, or even coppery hue; it is occasionally divided by an Equatorial Band (EB).<a href="#cite_note-50">[50]</a> Features in the EZ move roughly 390 km/h relative to the other latitudes.<a href="#cite_note-51">[51]</a><a href="#cite_note-52">[52]</a> The South Tropical Region includes the South Equatorial Belt (SEB) and the South Tropical Zone. It is by far the most active region on the planet, as it is home to its strongest <a href="/wiki/Retrograde_and_direct_motion" class="mw-redirect" title="Retrograde and direct motion">retrograde</a> jet stream. The SEB is usually the broadest, darkest belt on Jupiter; it is sometimes split by a zone (the SEBZ), and can fade entirely every 3 to 15 years before reappearing in what is known as an SEB Revival cycle. A period of weeks or months following the belt's disappearance, a white spot forms and erupts dark brownish material which is stretched into a new belt by Jupiter's winds. The belt most recently disappeared in May 2010.<a href="#cite_note-53">[53]</a> Another characteristic of the SEB is a long train of cyclonic disturbances following the Great Red Spot. Like the NTropZ, the STropZ is one of the most prominent zones on the planet; not only does it contain the GRS, but it is occasionally rent by a South Tropical Disturbance (STropD), a division of the zone that can be very long-lived; the most famous one lasted from 1901 to 1939.<a href="#cite_note-54">[54]</a> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Jupiter_at_a_glance.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/0/0b/Jupiter_at_a_glance.jpg/220px-Jupiter_at_a_glance.jpg" decoding="async" width="220" height="98" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0b/Jupiter_at_a_glance.jpg/330px-Jupiter_at_a_glance.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0b/Jupiter_at_a_glance.jpg/440px-Jupiter_at_a_glance.jpg 2x" data-file-width="3600" data-file-height="1598" /></a><figcaption>This false color image from the HST reveals a rare wave structure just north of the planet's equator.<a href="#cite_note-55">[55]</a></figcaption></figure> The South Temperate Region, or South Temperate Belt (STB), is yet another dark, prominent belt, more so than the NTB; until March 2000, its most famous features were the long-lived white ovals BC, DE, and FA, which have since merged to form Oval BA ("Red Jr."). The ovals were part of South Temperate Zone, but they extended into STB partially blocking it.<a href="#cite_note-Ingersoll1-5">[5]</a> The STB has occasionally faded, apparently due to complex interactions between the white ovals and the GRS. The appearance of the South Temperate Zone (STZ)—the zone in which the white ovals originated—is highly variable.<a href="#cite_note-56">[56]</a> There are other features on Jupiter that are either temporary or difficult to observe from Earth. The South South Temperate Region is harder to discern even than the NNTR; its detail is subtle and can only be studied well by large telescopes or spacecraft.<a href="#cite_note-57">[57]</a> Many zones and belts are more transient in nature and are not always visible. These include the Equatorial band (EB),<a href="#cite_note-Rogers2003-58">[58]</a> North Equatorial belt zone (NEBZ, a white zone within the belt) and South Equatorial belt zone (SEBZ).<a href="#cite_note-Rogers2001-59">[59]</a> Belts are also occasionally split by a sudden disturbance. When a disturbance divides a normally singular belt or zone, an N or an S is added to indicate whether the component is the northern or southern one; e.g., NEB(N) and NEB(S).<a href="#cite_note-60">[60]</a> <div class="mw-heading mw-heading2"><h2 id="Dynamics">Dynamics</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=6" title="Edit section: Dynamics">edit</a>]</div> <style data-mw-deduplicate="TemplateStyles:r1237032888/mw-parser-output/.tmulti">.mw-parser-output .tmulti .multiimageinner{display:flex;flex-direction:column}.mw-parser-output .tmulti .trow{display:flex;flex-direction:row;clear:left;flex-wrap:wrap;width:100%;box-sizing:border-box}.mw-parser-output .tmulti .tsingle{margin:1px;float:left}.mw-parser-output .tmulti .theader{clear:both;font-weight:bold;text-align:center;align-self:center;background-color:transparent;width:100%}.mw-parser-output .tmulti .thumbcaption{background-color:transparent}.mw-parser-output .tmulti .text-align-left{text-align:left}.mw-parser-output .tmulti .text-align-right{text-align:right}.mw-parser-output .tmulti .text-align-center{text-align:center}@media all and (max-width:720px){.mw-parser-output .tmulti .thumbinner{width:100%!important;box-sizing:border-box;max-width:none!important;align-items:center}.mw-parser-output .tmulti .trow{justify-content:center}.mw-parser-output .tmulti .tsingle{float:none!important;max-width:100%!important;box-sizing:border-box;text-align:center}.mw-parser-output .tmulti .tsingle .thumbcaption{text-align:left}.mw-parser-output .tmulti .trow>.thumbcaption{text-align:center}}@media screen{html.skin-theme-clientpref-night .mw-parser-output .tmulti .multiimageinner img{background-color:white}}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .tmulti .multiimageinner img{background-color:white}}</style><div class="thumb tmulti tright"><div class="thumbinner multiimageinner" style="width:408px;max-width:408px"><div class="trow"><div class="tsingle" style="width:202px;max-width:202px"><div class="thumbimage"><a href="/wiki/File:Jupiter_on_2009-07-23_(captured_by_the_Hubble_Space_Telescope).jpg" class="mw-file-description"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/4/43/Jupiter_on_2009-07-23_%28captured_by_the_Hubble_Space_Telescope%29.jpg/200px-Jupiter_on_2009-07-23_%28captured_by_the_Hubble_Space_Telescope%29.jpg" decoding="async" width="200" height="207" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/43/Jupiter_on_2009-07-23_%28captured_by_the_Hubble_Space_Telescope%29.jpg/300px-Jupiter_on_2009-07-23_%28captured_by_the_Hubble_Space_Telescope%29.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/43/Jupiter_on_2009-07-23_%28captured_by_the_Hubble_Space_Telescope%29.jpg/400px-Jupiter_on_2009-07-23_%28captured_by_the_Hubble_Space_Telescope%29.jpg 2x" data-file-width="1368" data-file-height="1416" /></a></div><div class="thumbcaption text-align-center">2009</div></div><div class="tsingle" style="width:202px;max-width:202px"><div class="thumbimage"><a href="/wiki/File:Jupiter_on_2010-06-07_(captured_by_the_Hubble_Space_Telescope).jpg" class="mw-file-description"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1a/Jupiter_on_2010-06-07_%28captured_by_the_Hubble_Space_Telescope%29.jpg/200px-Jupiter_on_2010-06-07_%28captured_by_the_Hubble_Space_Telescope%29.jpg" decoding="async" width="200" height="207" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1a/Jupiter_on_2010-06-07_%28captured_by_the_Hubble_Space_Telescope%29.jpg/300px-Jupiter_on_2010-06-07_%28captured_by_the_Hubble_Space_Telescope%29.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1a/Jupiter_on_2010-06-07_%28captured_by_the_Hubble_Space_Telescope%29.jpg/400px-Jupiter_on_2010-06-07_%28captured_by_the_Hubble_Space_Telescope%29.jpg 2x" data-file-width="1368" data-file-height="1416" /></a></div><div class="thumbcaption text-align-center">2010</div></div></div></div></div> Circulation in Jupiter's atmosphere is markedly different from that <a href="/wiki/Atmospheric_circulation" title="Atmospheric circulation">in the atmosphere of Earth</a>. The interior of Jupiter is fluid and lacks any solid surface. Therefore, <a href="/wiki/Convection" title="Convection">convection</a> may occur throughout the planet's outer molecular envelope. As of 2008, a comprehensive theory of the dynamics of the Jovian atmosphere has not been developed. Any such theory needs to explain the following facts: the existence of narrow stable bands and jets that are symmetric relative to Jupiter's equator, the strong prograde jet observed at the equator, the difference between zones and belts, and the origin and persistence of large vortices such as the Great Red Spot.<a href="#cite_note-1942Vasavada-6">[6]</a> The theories regarding the dynamics of the Jovian atmosphere can be broadly divided into two classes: shallow and deep. The former hold that the observed circulation is largely confined to a thin outer (weather) layer of the planet, which overlays the stable interior. The latter hypothesis postulates that the observed atmospheric flows are only a surface manifestation of deeply rooted circulation in the outer molecular envelope of Jupiter.<a href="#cite_note-1943Vasavada-61">[61]</a> As both theories have their own successes and failures, many planetary scientists think that the true theory will include elements of both models.<a href="#cite_note-Heimpel2005-62">[62]</a> <div class="mw-heading mw-heading3"><h3 id="Shallow_models">Shallow models</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=7" title="Edit section: Shallow models">edit</a>]</div> The first attempts to explain Jovian atmospheric dynamics date back to the 1960s.<a href="#cite_note-1943Vasavada-61">[61]</a><a href="#cite_note-Ingersoll1969-63">[63]</a> They were partly based on terrestrial <a href="/wiki/Meteorology" title="Meteorology">meteorology</a>, which had become well developed by that time. Those shallow models assumed that the jets on Jupiter are driven by small scale <a href="/wiki/Turbulence" title="Turbulence">turbulence</a>, which is in turn maintained by moist convection in the outer layer of the atmosphere (above the water clouds).<a href="#cite_note-1947Vasavada-64">[64]</a><a href="#cite_note-Ingersoll5-65">[65]</a> The moist convection is a phenomenon related to the condensation and evaporation of water and is one of the major drivers of terrestrial weather.<a href="#cite_note-Ingersoll6-66">[66]</a> The production of the jets in this model is related to a well-known property of two dimensional turbulence—the so-called inverse cascade, in which small turbulent structures (vortices) merge to form larger ones.<a href="#cite_note-1947Vasavada-64">[64]</a> The finite size of the planet means that the cascade can not produce structures larger than some characteristic scale, which for Jupiter is called the Rhines scale. Its existence is connected to production of <a href="/wiki/Rossby_wave" title="Rossby wave">Rossby waves</a>. This process works as follows: when the largest turbulent structures reach a certain size, the energy begins to flow into Rossby waves instead of larger structures, and the inverse cascade stops.<a href="#cite_note-1949Vasavada-67">[67]</a> Since on the spherical rapidly rotating planet the <a href="/wiki/Dispersion_relation" title="Dispersion relation">dispersion relation</a> of the Rossby waves is <a href="/wiki/Anisotropic" class="mw-redirect" title="Anisotropic">anisotropic</a>, the Rhines scale in the direction parallel to the equator is larger than in the direction orthogonal to it.<a href="#cite_note-1949Vasavada-67">[67]</a> The ultimate result of the process described above is production of large scale elongated structures, which are parallel to the equator. The meridional extent of them appears to match the actual width of jets.<a href="#cite_note-1947Vasavada-64">[64]</a> Therefore, in shallow models vortices actually feed the jets and should disappear by merging into them. While these weather–layer models can successfully explain the existence of a dozen narrow jets, they have serious problems.<a href="#cite_note-1947Vasavada-64">[64]</a> A glaring failure of the model is the prograde (super-rotating) equatorial jet: with some rare exceptions shallow models produce a strong retrograde (subrotating) jet, contrary to observations. In addition, the jets tend to be unstable and can disappear over time.<a href="#cite_note-1947Vasavada-64">[64]</a> Shallow models cannot explain how the observed atmospheric flows on Jupiter violate stability criteria.<a href="#cite_note-1945Vasavada-68">[68]</a> More elaborated multilayer versions of weather–layer models produce more stable circulation, but many problems persist.<a href="#cite_note-1962Vasavada-69">[69]</a> Meanwhile, the <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo Probe</a> found that the winds on Jupiter extend well below the water clouds at 5–7 bar and do not show any evidence of decay down to 22 bar pressure level, which implies that circulation in the Jovian atmosphere may in fact be deep.<a href="#cite_note-Ingersoll3-18">[18]</a> <div class="mw-heading mw-heading3"><h3 id="Deep_models">Deep models</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=8" title="Edit section: Deep models">edit</a>]</div> The deep model was first proposed by Busse in 1976.<a href="#cite_note-1966Vasavada-70">[70]</a><a href="#cite_note-Busse1976-71">[71]</a> His model was based on another well-known feature of fluid mechanics, the <a href="/wiki/Taylor%E2%80%93Proudman_theorem" title="Taylor–Proudman theorem">Taylor–Proudman theorem</a>. It holds that in any fast-rotating <a href="/wiki/Barotropic" class="mw-redirect" title="Barotropic">barotropic</a> ideal liquid, the flows are organized in a series of cylinders parallel to the rotational axis. The conditions of the theorem are probably met in the fluid Jovian interior. Therefore, the planet's molecular hydrogen mantle may be divided into cylinders, each cylinder having a circulation independent of the others.<a href="#cite_note-1966-1Vasavada-72">[72]</a> Those latitudes where the cylinders' outer and inner boundaries intersect with the visible surface of the planet correspond to the jets; the cylinders themselves are observed as zones and belts. <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Thermal_emission_of_Jupiter.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2c/Thermal_emission_of_Jupiter.jpg/220px-Thermal_emission_of_Jupiter.jpg" decoding="async" width="220" height="240" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2c/Thermal_emission_of_Jupiter.jpg/330px-Thermal_emission_of_Jupiter.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2c/Thermal_emission_of_Jupiter.jpg/440px-Thermal_emission_of_Jupiter.jpg 2x" data-file-width="1100" data-file-height="1200" /></a><figcaption>False color thermal image of Jupiter obtained by <a href="/wiki/NASA_Infrared_Telescope_Facility" title="NASA Infrared Telescope Facility">NASA Infrared Telescope Facility</a></figcaption></figure> The deep model easily explains the strong prograde jet observed at the equator of Jupiter; the jets it produces are stable and do not obey the 2D stability criterion.<a href="#cite_note-1966-1Vasavada-72">[72]</a> However it has major difficulties; it produces a very small number of broad jets, and realistic simulations of 3D flows are not possible as of 2008, meaning that the simplified models used to justify deep circulation may fail to catch important aspects of the <a href="/wiki/Fluid_mechanics" title="Fluid mechanics">fluid dynamics</a> within Jupiter.<a href="#cite_note-1966-1Vasavada-72">[72]</a> One model published in 2004 successfully reproduced the Jovian band-jet structure.<a href="#cite_note-Heimpel2005-62">[62]</a> It assumed that the molecular hydrogen mantle is thinner than in all other models; occupying only the outer 10% of Jupiter's radius. In standard models of the Jovian interior, the mantle comprises the outer 20–30%.<a href="#cite_note-1970Vasavada-73">[73]</a> The driving of deep circulation is another problem. The deep flows can be caused both by shallow forces (moist convection, for instance) or by deep planet-wide convection that transports heat out of the Jovian interior.<a href="#cite_note-1947Vasavada-64">[64]</a> Which of these mechanisms is more important is not clear yet. <div class="mw-heading mw-heading3"><h3 id="Internal_heat">Internal heat</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=9" title="Edit section: Internal heat">edit</a>]</div> As has been known since 1966,<a href="#cite_note-Low-74">[74]</a> Jupiter radiates much more heat than it receives from the Sun. It is estimated that the ratio of the thermal power emitted by the planet to the thermal power absorbed from the Sun is 1.67 ± 0.09. The internal <a href="/wiki/Heat_flux" title="Heat flux">heat flux</a> from Jupiter is 5.44 ± 0.43 W/m2, whereas the total emitted power is 335 ± 26 <a href="/wiki/Petawatt" class="mw-redirect" title="Petawatt">petawatts</a>. The latter value is approximately equal to one billionth of the total power radiated by the Sun. This excess heat is mainly the primordial heat from the early phases of Jupiter's formation, but may result in part from the precipitation of helium into the core.<a href="#cite_note-FOOTNOTEPearl_Conrath_et_al.199012,_26-75">[75]</a> The <a href="/wiki/Internal_heat" class="mw-redirect" title="Internal heat">internal heat</a> may be important for the dynamics of the Jovian atmosphere. While Jupiter has a small obliquity of about 3°, and its poles receive much less solar radiation than its equator, the tropospheric temperatures do not change appreciably from the equator to poles. One explanation is that Jupiter's convective interior acts like a thermostat, releasing more heat near the poles than in the equatorial region. This leads to a uniform temperature in the troposphere. While heat is transported from the equator to the poles mainly <a href="/wiki/Atmospheric_circulation" title="Atmospheric circulation">via the atmosphere</a> on Earth, on Jupiter deep convection <a href="/wiki/Thermodynamic_equilibrium#Thermal_equilibrium" title="Thermodynamic equilibrium">equilibrates</a> heat. The convection in the Jovian interior is thought to be driven mainly by the internal heat.<a href="#cite_note-Ingersoll9-76">[76]</a> <div class="mw-heading mw-heading2"><h2 id="Discrete_features">Discrete features</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=10" title="Edit section: Discrete features">edit</a>]</div> <div class="mw-heading mw-heading3"><h3 id="Vortices">Vortices</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=11" title="Edit section: Vortices">edit</a>]</div> <figure class="mw-default-size mw-halign-right" typeof="mw:File/Thumb"><a href="/wiki/File:NH_Jupiter_IR_(contrast_enhanced).jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/d/db/NH_Jupiter_IR_%28contrast_enhanced%29.jpg/220px-NH_Jupiter_IR_%28contrast_enhanced%29.jpg" decoding="async" width="220" height="418" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/d/db/NH_Jupiter_IR_%28contrast_enhanced%29.jpg 1.5x" data-file-width="253" data-file-height="481" /></a><figcaption><a href="/wiki/New_Horizons" title="New Horizons">New Horizons</a> IR view of Jupiter's atmosphere, <a href="/wiki/False_color" title="False color">false color</a></figcaption></figure> The atmosphere of Jupiter is home to hundreds of <a href="/wiki/Vortex" title="Vortex">vortices</a>—circular rotating structures that, as in the Earth's atmosphere, can be divided into two classes: <a href="/wiki/Cyclone" title="Cyclone">cyclones</a> and <a href="/wiki/Anticyclone" title="Anticyclone">anticyclones</a>.<a href="#cite_note-1974Vasavada-7">[7]</a> Cyclones rotate in the direction similar to the rotation of the planet (<a href="/wiki/Counterclockwise" class="mw-redirect" title="Counterclockwise">counterclockwise</a> in the northern hemisphere and <a href="/wiki/Clockwise" title="Clockwise">clockwise</a> in the southern); anticyclones rotate in the reverse direction. However, unlike in the <a href="/wiki/Earth%27s_atmosphere" class="mw-redirect" title="Earth's atmosphere">terrestrial atmosphere</a>, anticyclones predominate over cyclones on Jupiter—more than 90% of vortices larger than 2000 km in diameter are anticyclones.<a href="#cite_note-1978Vasavada-77">[77]</a> The lifetime of Jovian vortices varies from several days to hundreds of years, depending on their size. For instance, the average lifetime of an anticyclone between 1000 and 6000 km in diameter is 1–3 years.<a href="#cite_note-1977Vasavada-78">[78]</a> Vortices have never been observed in the equatorial region of Jupiter (within 10° of latitude), where they are unstable.<a href="#cite_note-1976Vasavada-10">[10]</a> As on any rapidly rotating planet, Jupiter's anticyclones are high <a href="/wiki/Pressure" title="Pressure">pressure</a> centers, while cyclones are low pressure.<a href="#cite_note-1987Vasavada-49">[49]</a> <figure class="mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:Great_Cold_Spot_discovered_on_Jupiter.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f8/Great_Cold_Spot_discovered_on_Jupiter.jpg/150px-Great_Cold_Spot_discovered_on_Jupiter.jpg" decoding="async" width="150" height="127" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f8/Great_Cold_Spot_discovered_on_Jupiter.jpg/225px-Great_Cold_Spot_discovered_on_Jupiter.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f8/Great_Cold_Spot_discovered_on_Jupiter.jpg/300px-Great_Cold_Spot_discovered_on_Jupiter.jpg 2x" data-file-width="2388" data-file-height="2023" /></a><figcaption>Great Cold Spot on Jupiter, false color<a href="#cite_note-79">[79]</a></figcaption></figure> <figure class="mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:PIA21972_Jupiter_Blues.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/5c/PIA21972_Jupiter_Blues.jpg/150px-PIA21972_Jupiter_Blues.jpg" decoding="async" width="150" height="127" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5c/PIA21972_Jupiter_Blues.jpg/225px-PIA21972_Jupiter_Blues.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5c/PIA21972_Jupiter_Blues.jpg/300px-PIA21972_Jupiter_Blues.jpg 2x" data-file-width="1920" data-file-height="1630" /></a><figcaption>Jupiter clouds in false color (<a href="/wiki/Juno_(spacecraft)" title="Juno (spacecraft)">Juno</a>; October 2017)</figcaption></figure> The anticyclones in Jupiter's atmosphere are always confined within zones, where the wind speed increases in direction from the <a href="/wiki/Equator" title="Equator">equator</a> to the poles.<a href="#cite_note-1977Vasavada-78">[78]</a> They are usually bright and appear as white ovals.<a href="#cite_note-1974Vasavada-7">[7]</a> They can move in <a href="/wiki/Longitude" title="Longitude">longitude</a>, but stay at approximately the same latitude as they are unable to escape from the confining zone.<a href="#cite_note-1976Vasavada-10">[10]</a> The wind speeds at their periphery are about 100 m/s.<a href="#cite_note-1980Vasavada-9">[9]</a> Different anticyclones located in one zone tend to merge when they approach each other.<a href="#cite_note-80">[80]</a> However Jupiter has two anticyclones that are somewhat different from all others. They are the Great Red Spot (GRS)<a href="#cite_note-1978bVasavada-8">[8]</a> and the Oval BA;<a href="#cite_note-1980Vasavada-9">[9]</a> the latter formed only in 2000. In contrast to white ovals, these structures are red, arguably due to dredging up of red material from the planet's depths.<a href="#cite_note-1978bVasavada-8">[8]</a> On Jupiter the anticyclones usually form through merges of smaller structures including convective storms (see below),<a href="#cite_note-1977Vasavada-78">[78]</a> although large ovals can result from the instability of jets. The latter was observed in 1938–1940, when a few white ovals appeared as a result of instability of the southern temperate zone; they later merged to form Oval BA.<a href="#cite_note-1980Vasavada-9">[9]</a><a href="#cite_note-1977Vasavada-78">[78]</a> In contrast to anticyclones, the Jovian cyclones tend to be small, dark and irregular structures. Some of the darker and more regular features are known as brown ovals (or badges).<a href="#cite_note-1978Vasavada-77">[77]</a> However the existence of a few long–lived large cyclones has been suggested. In addition to compact cyclones, Jupiter has several large irregular filamentary patches, which demonstrate <a href="/wiki/Cyclonic_rotation" title="Cyclonic rotation">cyclonic rotation</a>.<a href="#cite_note-1974Vasavada-7">[7]</a> One of them is located to the west of the GRS (in its <a href="/wiki/Wake_(physics)" title="Wake (physics)">wake</a> region) in the southern equatorial belt.<a href="#cite_note-1979Vasavada-81">[81]</a> These patches are called cyclonic regions (CR). The cyclones are always located in the belts and tend to merge when they encounter each other, much like anticyclones.<a href="#cite_note-1977Vasavada-78">[78]</a> The deep structure of vortices is not completely clear. They are thought to be relatively thin, as any thickness greater than about 500 km will lead to instability. The large anticyclones are known to extend only a few tens of kilometers above the visible clouds. As of 2008, the early hypothesis that the vortices are deep <a href="/wiki/Convection" title="Convection">convective plumes</a> (or convective columns) is not shared by the majority of <a href="/wiki/Planetary_science" title="Planetary science">planetary scientists</a>.<a href="#cite_note-1976Vasavada-10">[10]</a> <div class="mw-heading mw-heading4"><h4 id="Great_Red_Spot">Great Red Spot</h4>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=12" title="Edit section: Great Red Spot">edit</a>]</div> <style data-mw-deduplicate="TemplateStyles:r1236090951">.mw-parser-output .hatnote{font-style:italic}.mw-parser-output div.hatnote{padding-left:1.6em;margin-bottom:0.5em}.mw-parser-output .hatnote i{font-style:normal}.mw-parser-output .hatnote+link+.hatnote{margin-top:-0.5em}@media print{body.ns-0 .mw-parser-output .hatnote{display:none!important}}</style><div role="note" class="hatnote navigation-not-searchable">Main article: <a href="/wiki/Great_Red_Spot" title="Great Red Spot">Great Red Spot</a></div> <figure class="mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/3/30/NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg/400px-NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg" decoding="async" width="400" height="250" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/30/NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg/600px-NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/30/NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg/800px-NASA14135-Jupiter-GreatRedSpot-Shrinks-20140515.jpg 2x" data-file-width="1200" data-file-height="750" /></a><figcaption>The Great Red Spot is decreasing in size (May 15, 2014).<a href="#cite_note-NASA-20140515-82">[82]</a></figcaption></figure> The Great Red Spot (GRS) is a persistent <a href="/wiki/Anticyclonic_storm" title="Anticyclonic storm">anticyclonic storm</a>, 22° south of Jupiter's equator; observations from Earth establish a minimum storm lifetime of 350 years.<a href="#cite_note-83">[83]</a><a href="#cite_note-84">[84]</a> A storm was described as a "permanent spot" by <a href="/wiki/Gian_Domenico_Cassini" class="mw-redirect" title="Gian Domenico Cassini">Gian Domenico Cassini</a> after observing the feature in July 1665 with his instrument-maker <a href="/wiki/Eustachio_Divini" title="Eustachio Divini">Eustachio Divini</a>.<a href="#cite_note-85">[85]</a> According to a report by <a href="/wiki/Giovanni_Battista_Riccioli" title="Giovanni Battista Riccioli">Giovanni Battista Riccioli</a> in 1635, Leander Bandtius, whom Riccioli identified as the Abbot of Dunisburgh who possessed an "extraordinary telescope", observed a large spot that he described as "oval, equaling one seventh of Jupiter's diameter at its longest." According to Riccioli, "these features are seldom able to be seen, and then only by a telescope of exceptional quality and magnification".<a href="#cite_note-86">[86]</a> The Great Spot has been continually observed since the 1870s, however. The GRS rotates counter-clockwise, with a period of about six Earth days<a href="#cite_note-87">[87]</a> or 14 <a href="/wiki/Jupiter" title="Jupiter">Jovian</a> days. Its dimensions are 24,000–40,000 km east-to-west and 12,000–14,000 km north-to-south. The spot is large enough to contain two or three planets the size of Earth. At the start of 2004, the Great Red Spot had approximately half the longitudinal extent it had a century ago, when it was 40,000 km in diameter. At the present rate of reduction, it could potentially become circular by 2040, although this is unlikely because of the distortion effect of the neighboring jet streams.<a href="#cite_note-Irwin171-88">[88]</a> It is not known how long the spot will last, or whether the change is a result of normal fluctuations.<a href="#cite_note-89">[89]</a> <figure class="mw-halign-right" typeof="mw:File/Thumb"><a href="/wiki/File:GRS_in_far_infrared.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f9/GRS_in_far_infrared.jpg/200px-GRS_in_far_infrared.jpg" decoding="async" width="200" height="241" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f9/GRS_in_far_infrared.jpg/300px-GRS_in_far_infrared.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f9/GRS_in_far_infrared.jpg/400px-GRS_in_far_infrared.jpg 2x" data-file-width="469" data-file-height="566" /></a><figcaption>An infrared image of GRS (top) and Oval BA (lower left) showing its cool center, taken by the ground based Very Large Telescope. An image made by the Hubble Space Telescope (bottom) is shown for comparison.</figcaption></figure> According to a study by scientists at the <a href="/wiki/University_of_California,_Berkeley" title="University of California, Berkeley">University of California, Berkeley</a>, between 1996 and 2006 the spot lost 15 percent of its diameter along its major axis. Xylar Asay-Davis, who was on the team that conducted the study, noted that the spot is not disappearing because "velocity is a more robust measurement because the clouds associated with the Red Spot are also strongly influenced by numerous other phenomena in the surrounding atmosphere."<a href="#cite_note-90">[90]</a> <a href="/wiki/Infrared" title="Infrared">Infrared</a> data have long indicated that the Great Red Spot is colder (and thus, higher in altitude) than most of the other clouds on the planet;<a href="#cite_note-91">[91]</a> the <a href="/wiki/Cloud" title="Cloud">cloudtops</a> of the GRS are about 8 km above the surrounding clouds. Furthermore, careful tracking of atmospheric features revealed the spot's counterclockwise circulation as far back as 1966 – observations dramatically confirmed by the first time-lapse movies from the Voyager flybys.<a href="#cite_note-92">[92]</a> The spot is spatially confined by a modest eastward <a href="/wiki/Jet_stream" title="Jet stream">jet stream</a> (prograde) to its south and a very strong westward (retrograde) one to its north.<a href="#cite_note-93">[93]</a> Though winds around the edge of the spot peak at about 120 m/s (432 km/h), currents inside it seem stagnant, with little inflow or outflow.<a href="#cite_note-94">[94]</a> The rotation period of the spot has decreased with time, perhaps as a direct result of its steady reduction in size.<a href="#cite_note-95">[95]</a> In 2010, astronomers imaged the GRS in the far infrared (from 8.5 to 24 μm) with a spatial resolution higher than ever before and found that its central, reddest region is warmer than its surroundings by between 3–4 <a href="/wiki/Kelvin_(unit)" class="mw-redirect" title="Kelvin (unit)">K</a>. The warm airmass is located in the upper troposphere in the pressure range of 200–500 mbar. This warm central spot slowly counter-rotates and may be caused by a weak subsidence of air in the center of GRS.<a href="#cite_note-Fletcher2010-96">[96]</a> The Great Red Spot's latitude has been stable for the duration of good observational records, typically varying by about a degree. Its <a href="/wiki/Longitude" title="Longitude">longitude</a>, however, is subject to constant variation.<a href="#cite_note-97">[97]</a><a href="#cite_note-98">[98]</a> Because Jupiter's visible features do not rotate uniformly at all latitudes, astronomers have defined three different systems for defining the longitude. System II is used for latitudes of more than 10°, and was originally based on the average rotation rate of the Great Red Spot of 9h 55m 42s.<a href="#cite_note-99">[99]</a><a href="#cite_note-100">[100]</a> Despite this, the spot has "lapped" the planet in System II at least 10 times since the early 19th century. Its drift rate has changed dramatically over the years and has been linked to the brightness of the South Equatorial Belt, and the presence or absence of a South Tropical Disturbance.<a href="#cite_note-101">[101]</a> <figure class="mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:Jupiter,_Earth_size_comparison.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/c/c2/Jupiter%2C_Earth_size_comparison.jpg/250px-Jupiter%2C_Earth_size_comparison.jpg" decoding="async" width="250" height="214" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/c2/Jupiter%2C_Earth_size_comparison.jpg/375px-Jupiter%2C_Earth_size_comparison.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/c2/Jupiter%2C_Earth_size_comparison.jpg/500px-Jupiter%2C_Earth_size_comparison.jpg 2x" data-file-width="3000" data-file-height="2571" /></a><figcaption>Approximate size comparison of Earth superimposed on this Dec 29, 2000 image showing the Great Red Spot</figcaption></figure> It is not known exactly what causes the Great Red Spot's reddish color. Theories supported by laboratory experiments suppose that the color may be caused by complex organic molecules, red phosphorus, or yet another sulfur compound. The GRS varies greatly in hue, from almost brick-red to pale salmon, or even white. The higher temperature of the reddest central region is the first evidence that the Spot's color is affected by environmental factors.<a href="#cite_note-Fletcher2010-96">[96]</a> The spot occasionally disappears from the visible spectrum, becoming evident only through the Red Spot Hollow, which is its niche in the South Equatorial Belt (SEB). The visibility of GRS is apparently coupled to the appearance of the SEB; when the belt is bright white, the spot tends to be dark, and when it is dark, the spot is usually light. The periods when the spot is dark or light occur at irregular intervals; in the 50 years from 1947 to 1997, the spot was darkest in the periods 1961–1966, 1968–1975, 1989–1990, and 1992–1993.<a href="#cite_note-Beebe1-102">[102]</a> In November 2014, an analysis of data from NASA's Cassini mission revealed that the red color is likely a product of simple chemicals being broken apart by solar ultraviolet irradiation in the planet's upper atmosphere.<a href="#cite_note-103">[103]</a><a href="#cite_note-104">[104]</a><a href="#cite_note-Hudson2018-105">[105]</a> The Great Red Spot should not be confused with the Great Dark Spot, a feature observed near Jupiter's north pole (bottom) in 2000 by the <a href="/wiki/Cassini%E2%80%93Huygens" title="Cassini–Huygens">Cassini–Huygens</a> spacecraft.<a href="#cite_note-106">[106]</a> A feature in the atmosphere of <a href="/wiki/Neptune" title="Neptune">Neptune</a> was also called the <a href="/wiki/Great_Dark_Spot" title="Great Dark Spot">Great Dark Spot</a>. The latter feature, imaged by <a href="/wiki/Voyager_2" title="Voyager 2">Voyager 2</a> in 1989, may have been an atmospheric hole rather than a storm. It was no longer present in 1994, although a similar spot had appeared farther to the north.<a href="#cite_note-107">[107]</a> <div class="mw-heading mw-heading4"><h4 id="Oval_BA">Oval BA</h4>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=13" title="Edit section: Oval BA">edit</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Redjunior.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/6a/Redjunior.jpg/220px-Redjunior.jpg" decoding="async" width="220" height="119" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/6a/Redjunior.jpg/330px-Redjunior.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/6a/Redjunior.jpg/440px-Redjunior.jpg 2x" data-file-width="1500" data-file-height="808" /></a><figcaption>Oval BA (left)</figcaption></figure> Oval BA is a red storm in Jupiter's southern hemisphere similar in form to, though smaller than, the Great Red Spot (it is often affectionately referred to as "Red Spot Jr.", "Red Jr." or "The Little Red Spot"). A feature in the South Temperate Belt, Oval BA was first seen in 2000 after the collision of three small white storms, and has intensified since then.<a href="#cite_note-Sanchez-Lavega_2001-108">[108]</a> The formation of the three white oval storms that later merged into Oval BA can be traced to 1939, when the South Temperate Zone was torn by dark features that effectively split the zone into three long sections. Jovian observer Elmer J. Reese labeled the dark sections AB, CD, and EF. The rifts expanded, shrinking the remaining segments of the STZ into the white ovals FA, BC, and DE.<a href="#cite_note-109">[109]</a> Ovals BC and DE merged in 1998, forming Oval BE. Then, in March 2000, BE and FA joined, forming Oval BA.<a href="#cite_note-Sanchez-Lavega_2001-108">[108]</a> (see <a href="#White_ovals">White ovals</a>, below) <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Oval_BA_(Hubble).jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2d/Oval_BA_%28Hubble%29.jpg/220px-Oval_BA_%28Hubble%29.jpg" decoding="async" width="220" height="154" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2d/Oval_BA_%28Hubble%29.jpg/330px-Oval_BA_%28Hubble%29.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2d/Oval_BA_%28Hubble%29.jpg/440px-Oval_BA_%28Hubble%29.jpg 2x" data-file-width="693" data-file-height="485" /></a><figcaption>Formation of Oval BA from three white ovals</figcaption></figure> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/3/3d/Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg/220px-Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg" decoding="async" width="220" height="103" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/3d/Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg/330px-Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/3d/Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg/440px-Three_Red_Spots_Mix_it_Up_on_Jupiter.jpg 2x" data-file-width="1000" data-file-height="467" /></a><figcaption>Oval BA (bottom), Great Red Spot (top) and "Baby Red Spot" (middle) during a brief encounter in June, 2008</figcaption></figure> Oval BA slowly began to turn red in August 2005.<a href="#cite_note-go-110">[110]</a> On February 24, 2006, <a href="/wiki/Filipino_people" class="mw-redirect" title="Filipino people">Filipino</a> amateur astronomer Christopher Go discovered the color change, noting that it had reached the same shade as the GRS.<a href="#cite_note-go-110">[110]</a> As a result, NASA writer Dr. Tony Phillips suggested it be called "Red Spot Jr." or "Red Jr."<a href="#cite_note-111">[111]</a> In April 2006, a team of astronomers, believing that Oval BA might converge with the GRS that year, observed the storms through the <a href="/wiki/Hubble_Space_Telescope" title="Hubble Space Telescope">Hubble Space Telescope</a>.<a href="#cite_note-Tony-112">[112]</a> The storms pass each other about every two years, but the passings of 2002 and 2004 did not produce anything exciting. Dr. <a href="/wiki/Amy_Simon" title="Amy Simon">Amy Simon</a>-Miller, of the <a href="/wiki/Goddard_Space_Flight_Center" title="Goddard Space Flight Center">Goddard Space Flight Center</a>, predicted the storms would have their closest passing on July 4, 2006.<a href="#cite_note-Tony-112">[112]</a> On July 20, the two storms were photographed passing each other by the <a href="/wiki/Gemini_Observatory" title="Gemini Observatory">Gemini Observatory</a> without converging.<a href="#cite_note-113">[113]</a> Why Oval BA turned red is not well understood. According to a 2008 study by Dr. Santiago Pérez-Hoyos of the University of the Basque Country, the most likely mechanism is "an upward and inward diffusion of either a colored compound or a coating vapor that may interact later with high energy solar photons at the upper levels of Oval BA."<a href="#cite_note-basque-114">[114]</a> Some believe that small storms (and their corresponding white spots) on Jupiter turn red when the winds become powerful enough to draw certain gases from deeper within the atmosphere which change color when those gases are exposed to sunlight.<a href="#cite_note-NYTimes-115">[115]</a> Oval BA is getting stronger according to observations made with the Hubble Space Telescope in 2007. The wind speeds have reached 618 km/h; about the same as in the Great Red Spot and far stronger than any of the progenitor storms.<a href="#cite_note-116">[116]</a><a href="#cite_note-117">[117]</a> As of July 2008, its size is about the diameter of <a href="/wiki/Earth" title="Earth">Earth</a>—approximately half the size of the Great Red Spot.<a href="#cite_note-basque-114">[114]</a> Oval BA should not be confused with another major storm on Jupiter, the South Tropical Little Red Spot (LRS) (nicknamed "the Baby Red Spot" by NASA<a href="#cite_note-Rogers2008-118">[118]</a>), which was destroyed by the GRS.<a href="#cite_note-NYTimes-115">[115]</a> The new storm, previously a white spot in Hubble images, turned red in May 2008. The observations were led by Imke de Pater of the <a href="/wiki/University_of_California,_Berkeley" title="University of California, Berkeley">University of California, at Berkeley, US</a>.<a href="#cite_note-119">[119]</a> The Baby Red Spot encountered the GRS in late June to early July 2008, and in the course of a collision, the smaller red spot was shredded into pieces. The remnants of the Baby Red Spot first orbited, then were later consumed by the GRS. The last of the remnants with a reddish color to have been identified by astronomers had disappeared by mid-July, and the remaining pieces again collided with the GRS, then finally merged with the bigger storm. The remaining pieces of the Baby Red Spot had completely disappeared by August 2008.<a href="#cite_note-Rogers2008-118">[118]</a> During this encounter Oval BA was present nearby, but played no apparent role in the destruction of the Baby Red Spot.<a href="#cite_note-Rogers2008-118">[118]</a> <div class="mw-heading mw-heading3"><h3 id="Storms_and_lightning">Storms and lightning</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=14" title="Edit section: Storms and lightning">edit</a>]</div> <figure class="mw-default-size mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:Jupiter_lightnings.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/10/Jupiter_lightnings.jpg/220px-Jupiter_lightnings.jpg" decoding="async" width="220" height="116" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/10/Jupiter_lightnings.jpg/330px-Jupiter_lightnings.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/10/Jupiter_lightnings.jpg/440px-Jupiter_lightnings.jpg 2x" data-file-width="1700" data-file-height="900" /></a><figcaption>Lightning on Jupiter's night side, imaged by the Galileo orbiter in 1997</figcaption></figure> <figure class="mw-default-size mw-halign-right" typeof="mw:File/Thumb"><a href="/wiki/File:PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/b/b0/PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg/220px-PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg" decoding="async" width="220" height="242" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/b0/PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg/330px-PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/b0/PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg/440px-PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg 2x" data-file-width="2646" data-file-height="2915" /></a><figcaption>Jupiter – southern storms – <a href="/wiki/JunoCam" title="JunoCam">JunoCam</a>. False color image.<a href="#cite_note-NYT-20170525-120">[120]</a></figcaption></figure> The storms on Jupiter are similar to <a href="/wiki/Thunderstorm" title="Thunderstorm">thunderstorms</a> on Earth. They reveal themselves via bright clumpy clouds about 1000 km in size, which appear from time to time in the belts' cyclonic regions, especially within the strong westward (retrograde) jets.<a href="#cite_note-1982Vasavada-121">[121]</a> In contrast to vortices, storms are short-lived phenomena; the strongest of them may exist for several months, while the average lifetime is only 3–4 days.<a href="#cite_note-1982Vasavada-121">[121]</a> They are believed to be due mainly to moist convection within Jupiter's troposphere. Storms are actually tall convective columns (<a href="/wiki/Plume_(hydrodynamics)" class="mw-redirect" title="Plume (hydrodynamics)">plumes</a>), which bring the wet air from the depths to the upper part of the troposphere, where it condenses in clouds. A typical vertical extent of Jovian storms is about 100 km; as they extend from a pressure level of about 5–7 bar, where the base of a hypothetical water cloud layer is located, to as high as 0.2–0.5 bar.<a href="#cite_note-Sanchez-Lavega2008-437-122">[122]</a> Storms on Jupiter are always associated with <a href="/wiki/Lightning" title="Lightning">lightning</a>. The imaging of the night–side hemisphere of Jupiter by <a href="/wiki/Galileo_(spacecraft)" title="Galileo (spacecraft)">Galileo</a> and <a href="/wiki/Cassini_(spacecraft)" class="mw-redirect" title="Cassini (spacecraft)">Cassini</a> spacecraft revealed regular light flashes in Jovian belts and near the locations of the westward jets, particularly at 51°N, 56°S and 14°S latitudes.<a href="#cite_note-1983Vasavada-123">[123]</a> On Jupiter lightning strikes are on average a few times more powerful than those on Earth. However, they are less frequent; the light <a href="/wiki/Power_(physics)" title="Power (physics)">power</a> emitted from a given area is similar to that on Earth.<a href="#cite_note-1983Vasavada-123">[123]</a> A few flashes have been detected in polar regions, making Jupiter the second known planet after Earth to exhibit polar lightning.<a href="#cite_note-FOOTNOTEBaines_Simon-Miller_et_al.2007226-124">[124]</a> A <a href="/wiki/Microwave_Radiometer_(Juno)" title="Microwave Radiometer (Juno)">Microwave Radiometer (Juno)</a> detected many more in 2018. Every 15–17 years Jupiter is marked by especially powerful storms. They appear at 23°N latitude, where the strongest eastward jet, that can reach 150 m/s, is located. The last time such an event was observed was in March–June 2007.<a href="#cite_note-Sanchez-Lavega2008-437-122">[122]</a> Two storms appeared in the northern temperate belt 55° apart in longitude. They significantly disturbed the belt. The dark material that was shed by the storms mixed with clouds and changed the belt's color. The storms moved with a speed as high as 170 m/s, slightly faster than the jet itself, hinting at the existence of strong winds deep in the atmosphere.<a href="#cite_note-Sanchez-Lavega2008-437-122">[122]</a><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#endnote_Dnone">[d]</a> <div class="mw-heading mw-heading3"><h3 id="Circumpolar_cyclones">Circumpolar cyclones</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=15" title="Edit section: Circumpolar cyclones">edit</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:JIRAM_Image_Southern_CPCs.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/71/JIRAM_Image_Southern_CPCs.jpg/220px-JIRAM_Image_Southern_CPCs.jpg" decoding="async" width="220" height="187" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/71/JIRAM_Image_Southern_CPCs.jpg/330px-JIRAM_Image_Southern_CPCs.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/71/JIRAM_Image_Southern_CPCs.jpg/440px-JIRAM_Image_Southern_CPCs.jpg 2x" data-file-width="1600" data-file-height="1360" /></a><figcaption><a href="/w/index.php?title=False_Color&action=edit&redlink=1" class="new" title="False Color (page does not exist)">False colored</a> JIRAM image of southern CPCs</figcaption></figure> Other notable features of Jupiter are its cyclones near the northern and southern poles of the planet. These are called circumpolar cyclones (CPCs) and they have been observed by the Juno Spacecraft using JunoCam and JIRAM. The cyclones have now been observed for about 5 years, as Juno completed 39 orbits around Jupiter.<a href="#cite_note-125">[125]</a> The northern pole has eight cyclones moving around a central cyclone (NPC) while the southern pole only has five cyclones around a central cyclone (SPC), with a gap between the first and second cyclones.<a href="#cite_note-126">[126]</a> The cyclones look like the hurricanes on Earth with trailing spiral arms and a denser center, although there are differences between the centers depending on the individual cyclone. Northern CPCs generally maintain their shape and position compared to the southern CPCs and this could be due to the faster wind speeds that are experienced in the south, where the maximum wind velocities are around 80 m/s to 90 m/s.<a href="#cite_note-127">[127]</a> Although there is more movement among the southern CPCs they tend to retain the pentagonal structure relative to the pole. It has also been observed that the angular wind velocity increases as the center is approached and radius becomes smaller, except for one cyclone in the north, which may have rotation in the opposite direction. The difference in the number of cyclones in the north compared to the south is probably due to the size of the cyclones.<a href="#cite_note-128">[128]</a> The southern CPCs tend to be bigger with radii ranging from 5,600 km to 7,000 km while northern CPCs range from 4,000 km to 4,600 km.<a href="#cite_note-129">[129]</a> The mechanism for the stability of these two symmetric structures of cyclones is an outcome of <a href="/wiki/Tropical_cyclone#Beta_drift" title="Tropical cyclone">Beta-drift</a>, a known effect causing cyclones to move poleward and anti-cyclones to move equatorward due to the conservation of momentum along <a href="/wiki/Streamlines,_streaklines,_and_pathlines" title="Streamlines, streaklines, and pathlines">streamlines</a> in a vortex, under the change of the <a href="/wiki/Coriolis_frequency" title="Coriolis frequency">Coriolis parameter</a>.<a href="#cite_note-130">[130]</a> Thus, cyclones forming in the polar regions may congregate at the pole and form a polar cyclone such as those observed on <a href="/wiki/Saturn%27s_hexagon" title="Saturn's hexagon">Saturn's poles</a>.<a href="#cite_note-131">[131]</a><a href="#cite_note-132">[132]</a> The polar cyclone (the central cyclone in the polygons) also emit a <a href="/wiki/Vorticity" title="Vorticity">vorticity</a> field which can repel other cyclones (see <a href="/wiki/Fujiwhara_effect" title="Fujiwhara effect">Fujiwhara effect</a>) similar to the beta-effect. The <a href="/wiki/Latitude" title="Latitude">latitude</a> where the circumpolar cyclones are positioned (~84°) fits, in calculations, the hypothesis that the poleward beta-drift force balances the equatorward rejection of the polar cyclone on the circumpolar cyclones,<a href="#cite_note-:1-133">[133]</a> assuming they have an anticyclonic ring around them, consistent with model simulations<a href="#cite_note-134">[134]</a> and observations.<a href="#cite_note-:1-133">[133]</a> The northern cyclones tend to maintain an octagonal structure with the NPC as a center point. Northern cyclones have less data than southern cyclones because of limited illumination in the north-polar winter, making it difficult for JunoCam to obtain accurate measurements of northern CPC positions at each perijove (53 days), but JIRAM is able to collect enough data to understand the northern CPCs. The limited illumination makes it difficult to see the northern central cyclone, but by making four orbits, the NPC can be partially seen and the octagonal structure of the cyclones can be identified. Limited illumination also makes it difficult to view the motion of the cyclones, but early observations show that the NPC is offset from the pole by about 0.5˚ and the CPCs generally maintained their position around the center. Despite data being harder to obtain, it has been observed that the northern CPCs have a drift rate of about 1˚ to 2.5˚ per perijove to the west. The seventh cyclone in the north (n7) drifts a little more than the others and this is due to an anticyclonic white oval (AWO) that pulls it farther from the NPC, which causes the octagonal shape to be slightly distorted. The instantaneous locations of the south polar cyclones have been tracked for 5 years by the <a href="/wiki/JIRAM" class="mw-redirect" title="JIRAM">JIRAM</a> instrument and by <a href="/wiki/JunoCam" title="JunoCam">JunoCam</a>.<a href="#cite_note-135">[135]</a><a href="#cite_note-136">[136]</a> The locations over time were revealed to form an oscillatory motion of each of the 6 cyclones, with periods of approximately one (Earth) year and radii of about 400 km.<a href="#cite_note-137">[137]</a> These oscillations around the CPCs' mean positions were explained to be a result of imbalances between the beta-drift, pulling the CPCs toward the pole and the rejection forces that develop due to the interactions between the cyclones, similar to a 6-body spring system.<a href="#cite_note-138">[138]</a> In addition to this periodic motion, the south polar cyclones were observed to drift westward by 7.5±0.7˚ per year.<a href="#cite_note-139">[139]</a> The reason for this drift is still unknown. The circumpolar cyclones have different morphologies, especially in the north, where cyclones have a "filled" or "chaotic" structure. The inner part of the "chaotic" cyclones have small-scale cloud streaks and flecks. The "filled" cyclones have a sharply-bound, lobate area that is bright white near the edge with a dark inner portion. There are four "filled" cyclones and four "chaotic" cyclones in the north. The southern cyclones all have an extensive fine-scale spiral structure on their outside but they all differ in size and shape. There is very little observation of the cyclones due to low sun angles and a haze that is typically over the atmosphere but what little has been observed shows the cyclones to be a reddish color. <figure class="mw-default-size mw-halign-right" typeof="mw:File/Thumb"><a href="/wiki/File:Jupiter_equatorial_hot_spot.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Jupiter_equatorial_hot_spot.jpg/220px-Jupiter_equatorial_hot_spot.jpg" decoding="async" width="220" height="248" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Jupiter_equatorial_hot_spot.jpg/330px-Jupiter_equatorial_hot_spot.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Jupiter_equatorial_hot_spot.jpg/440px-Jupiter_equatorial_hot_spot.jpg 2x" data-file-width="800" data-file-height="900" /></a><figcaption>True color (top) and false color image (bottom) of an equatorial hot spot on Jupiter</figcaption></figure> <div class="mw-heading mw-heading3"><h3 id="Disturbances">Disturbances</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=16" title="Edit section: Disturbances">edit</a>]</div> The normal pattern of bands and zones is sometimes disrupted for periods of time. One particular class of disruption are long-lived darkenings of the South Tropical Zone, normally referred to as "South Tropical Disturbances" (STD). The longest lived STD in recorded history was followed from 1901 until 1939, having been first seen by <a href="/wiki/Percy_B._Molesworth" title="Percy B. Molesworth">Percy B. Molesworth</a> on February 28, 1901. It took the form of darkening over part of the normally bright South Tropical zone. Several similar disturbances in the South Tropical Zone have been recorded since then.<a href="#cite_note-140">[140]</a> <div class="mw-heading mw-heading3"><h3 id="Hot_spots">Hot spots</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=17" title="Edit section: Hot spots">edit</a>]</div> Some of the most mysterious features in the atmosphere of Jupiter are hot spots. In them, the air is relatively free of clouds and heat can escape from the depths without much absorption. The spots look like bright spots in the infrared images obtained at the wavelength of about 5 μm.<a href="#cite_note-1987Vasavada-49">[49]</a> They are preferentially located in the belts, although there is a train of prominent hot spots at the northern edge of the Equatorial Zone. The <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo Probe</a> descended into one of those equatorial spots. Each equatorial spot is associated with a bright cloudy <a href="/wiki/Plume_(hydrodynamics)" class="mw-redirect" title="Plume (hydrodynamics)">plume</a> located to the west of it and reaching up to 10,000 km in size.<a href="#cite_note-Ingersoll1-5">[5]</a> Hot spots generally have round shapes, although they do not resemble vortices.<a href="#cite_note-1987Vasavada-49">[49]</a> The origin of hot spots is not clear. They can be either <a href="/wiki/Downdraft" class="mw-redirect" title="Downdraft">downdrafts</a>, where the descending air is <a href="/wiki/Adiabatic" class="mw-redirect" title="Adiabatic">adiabatically</a> heated and dried or, alternatively, they can be a manifestation of planetary scale waves. The latter hypotheses explains the periodical pattern of the equatorial spots.<a href="#cite_note-Ingersoll1-5">[5]</a><a href="#cite_note-1987Vasavada-49">[49]</a> <div class="mw-heading mw-heading3"><h3 id="The_possibility_of_life">The possibility of life</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=18" title="Edit section: The possibility of life">edit</a>]</div> In 1953, the <a href="/wiki/Miller%E2%80%93Urey_experiment" title="Miller–Urey experiment">Miller–Urey experiment</a> proved that the combination of lightning and compounds existing in the primitive Earth's atmosphere can form organic matter (including amino acids), which can be used as the cornerstone of life. The simulated atmosphere consists of water, methane, ammonia and hydrogen molecules; all of these substances are found in today's Jupiter atmosphere. Jupiter's atmosphere has a strong vertical air flow that carries these compounds into lower regions. But there are higher temperatures inside Jupiter, which will decompose these chemicals and hinder the formation of life similar to Earth.<a href="#cite_note-141">[141]</a> This was speculated by <a href="/wiki/Carl_Sagan" title="Carl Sagan">Carl Sagan</a> and <a href="/wiki/Edwin_E._Salpeter" title="Edwin E. Salpeter">Edwin E. Salpeter</a>. <div class="mw-heading mw-heading2"><h2 id="Observational_history">Observational history</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=19" title="Edit section: Observational history">edit</a>]</div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1236090951"><div role="note" class="hatnote navigation-not-searchable">Main article: <a href="/wiki/Exploration_of_Jupiter" title="Exploration of Jupiter">Exploration of Jupiter</a></div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:790106-0203_Voyager_58M_to_31M_reduced.gif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif/220px-790106-0203_Voyager_58M_to_31M_reduced.gif" decoding="async" width="220" height="226" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif/330px-790106-0203_Voyager_58M_to_31M_reduced.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif 2x" data-file-width="390" data-file-height="400" /></a><figcaption>Time-lapse sequence from the approach of <a href="/wiki/Voyager_1" title="Voyager 1">Voyager 1</a> to Jupiter</figcaption></figure> Early modern astronomers, using small telescopes, recorded the changing appearance of Jupiter's atmosphere.<a href="#cite_note-Ingersoll8-24">[24]</a> Their descriptive terms—belts and zones, brown spots and red spots, plumes, barges, festoons, and streamers—are still used.<a href="#cite_note-Ingersoll10-142">[142]</a> Other terms such as vorticity, vertical motion, cloud heights have entered in use later, in the 20th century.<a href="#cite_note-Ingersoll8-24">[24]</a> The first observations of the Jovian atmosphere at higher resolution than possible with Earth-based telescopes were taken by the <a href="/wiki/Pioneer_program" title="Pioneer program">Pioneer</a> <a href="/wiki/Pioneer_10" title="Pioneer 10">10</a> and <a href="/wiki/Pioneer_11" title="Pioneer 11">11</a> spacecraft. The first truly detailed images of Jupiter's atmosphere were provided by the <a href="/wiki/Voyager_program" title="Voyager program">Voyagers</a>.<a href="#cite_note-Ingersoll8-24">[24]</a> The two spacecraft were able to image details at a resolution as low as 5 km in size in various spectra, and also able to create "approach movies" of the atmosphere in motion.<a href="#cite_note-Ingersoll8-24">[24]</a> The <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo Probe</a>, which suffered an antenna problem, saw less of Jupiter's atmosphere but at a better average resolution and a wider spectral bandwidth.<a href="#cite_note-Ingersoll8-24">[24]</a> Today, astronomers have access to a continuous record of Jupiter's atmospheric activity thanks to telescopes such as Hubble Space Telescope. These show that the atmosphere is occasionally wracked by massive disturbances, but that, overall, it is remarkably stable.<a href="#cite_note-Ingersoll8-24">[24]</a> The vertical motion of Jupiter's atmosphere was largely determined by the identification of trace gases by ground-based telescopes.<a href="#cite_note-Ingersoll8-24">[24]</a> <a href="/wiki/Astronomical_spectroscopy" title="Astronomical spectroscopy">Spectroscopic</a> studies after the collision of <a href="/wiki/Comet_Shoemaker%E2%80%93Levy_9" title="Comet Shoemaker–Levy 9">Comet Shoemaker–Levy 9</a> gave a glimpse of the Jupiter's composition beneath the cloud tops. The presence of <a href="/wiki/Diatomic_sulfur" class="mw-redirect" title="Diatomic sulfur">diatomic sulfur</a> (S2) and <a href="/wiki/Carbon_disulfide" title="Carbon disulfide">carbon disulfide</a> (CS2) was recorded—the first detection of either in Jupiter, and only the second detection of S2 in any <a href="/wiki/Astronomical_object" title="Astronomical object">astronomical object</a>— together with other molecules such as <a href="/wiki/Ammonia" title="Ammonia">ammonia</a> (NH3) and <a href="/wiki/Hydrogen_sulfide" title="Hydrogen sulfide">hydrogen sulfide</a> (H2S), while <a href="/wiki/Oxygen" title="Oxygen">oxygen</a>-bearing molecules such as <a href="/wiki/Sulfur_dioxide" title="Sulfur dioxide">sulfur dioxide</a> were not detected, to the surprise of astronomers.<a href="#cite_note-Noll1995-143">[143]</a> The <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">Galileo atmospheric probe</a>, as it plunged into Jupiter, measured the wind, temperature, composition, clouds, and radiation levels down to 22 bar. However, below 1 bar elsewhere on Jupiter there is uncertainty in the quantities.<a href="#cite_note-Ingersoll8-24">[24]</a> <div class="mw-heading mw-heading3"><h3 id="Great_Red_Spot_studies">Great Red Spot studies</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=20" title="Edit section: Great Red Spot studies">edit</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Great_Red_Spot_From_Voyager_1.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/e/ec/Great_Red_Spot_From_Voyager_1.jpg/220px-Great_Red_Spot_From_Voyager_1.jpg" decoding="async" width="220" height="208" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/ec/Great_Red_Spot_From_Voyager_1.jpg/330px-Great_Red_Spot_From_Voyager_1.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/ec/Great_Red_Spot_From_Voyager_1.jpg/440px-Great_Red_Spot_From_Voyager_1.jpg 2x" data-file-width="895" data-file-height="848" /></a><figcaption>A narrower view of Jupiter and the Great Red Spot as seen from <a href="/wiki/Voyager_1" title="Voyager 1">Voyager 1</a> in 1979</figcaption></figure> The first sighting of the <a href="#Great_Red_Spot">GRS</a> is often credited to <a href="/wiki/Robert_Hooke" title="Robert Hooke">Robert Hooke</a>, who described a spot on the planet in May 1664; however, it is likely that Hooke's spot was in the wrong belt altogether (the North Equatorial Belt, versus the current location in the South Equatorial Belt). Much more convincing is <a href="/wiki/Giovanni_Cassini" class="mw-redirect" title="Giovanni Cassini">Giovanni Cassini</a>'s description of a "permanent spot" in the following year.<a href="#cite_note-144">[144]</a> With fluctuations in visibility, Cassini's spot was observed from 1665 to 1713.<a href="#cite_note-Rogers2008b-145">[145]</a> A minor mystery concerns a Jovian spot depicted around 1700 on a canvas by <a href="/wiki/Donato_Creti" title="Donato Creti">Donato Creti</a>, which is exhibited in the <a href="/wiki/Vatican_City" title="Vatican City">Vatican</a>.<a href="#cite_note-Rogers188-146">[146]</a><a href="#cite_note-Hockey1-147">[147]</a> It is a part of a series of panels in which different (magnified) heavenly bodies serve as backdrops for various Italian scenes, the creation of all of them overseen by the astronomer <a href="/wiki/Eustachio_Manfredi" title="Eustachio Manfredi">Eustachio Manfredi</a> for accuracy. Creti's painting is the first known to depict the GRS as red. No Jovian feature was officially described as red before the late 19th century.<a href="#cite_note-Hockey1-147">[147]</a> The present GRS was first seen only after 1830 and well-studied only after a prominent apparition in 1879. A 118-year gap separates the observations made after 1830 from its 17th-century discovery; whether the original spot dissipated and re-formed, whether it faded, or even if the observational record was simply poor are unknown.<a href="#cite_note-Beebe1-102">[102]</a> The older spots had a short observational history and slower motion than that of the modern spot, which make their identity unlikely.<a href="#cite_note-Rogers188-146">[146]</a> <figure class="mw-default-size mw-halign-left" typeof="mw:File/Thumb"><a href="/wiki/File:Jupiter_and_its_shrunken_Great_Red_Spot.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2b/Jupiter_and_its_shrunken_Great_Red_Spot.jpg/220px-Jupiter_and_its_shrunken_Great_Red_Spot.jpg" decoding="async" width="220" height="220" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2b/Jupiter_and_its_shrunken_Great_Red_Spot.jpg/330px-Jupiter_and_its_shrunken_Great_Red_Spot.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2b/Jupiter_and_its_shrunken_Great_Red_Spot.jpg/440px-Jupiter_and_its_shrunken_Great_Red_Spot.jpg 2x" data-file-width="940" data-file-height="940" /></a><figcaption>Hubble's <a href="/wiki/Wide_Field_Camera_3" title="Wide Field Camera 3">Wide Field Camera 3</a> took the GRS region at its smallest size ever. Color and contrast are highly exaggerated.</figcaption></figure> On February 25, 1979, when the <a href="/wiki/Voyager_1" title="Voyager 1">Voyager 1</a> spacecraft was 9.2 million kilometers from Jupiter it transmitted the first detailed image of the Great Red Spot back to Earth. Cloud details as small as 160 km across were visible. The colorful, wavy cloud pattern seen to the west (left) of the GRS is the spot's wake region, where extraordinarily complex and variable cloud motions are observed.<a href="#cite_note-148">[148]</a> <div class="mw-heading mw-heading3"><h3 id="White_ovals">White ovals</h3>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=21" title="Edit section: White ovals">edit</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Whiteovals.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/64/Whiteovals.jpg/220px-Whiteovals.jpg" decoding="async" width="220" height="156" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/64/Whiteovals.jpg/330px-Whiteovals.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/64/Whiteovals.jpg/440px-Whiteovals.jpg 2x" data-file-width="492" data-file-height="349" /></a><figcaption>The white ovals that later formed Oval BA, imaged by the <a href="/wiki/Galileo_orbiter" class="mw-redirect" title="Galileo orbiter">Galileo orbiter</a> in 1997</figcaption></figure> The white ovals that were to become Oval BA formed in 1939. They covered almost 90 <a href="/wiki/Degree_(angle)" title="Degree (angle)">degrees</a> of <a href="/wiki/Longitude" title="Longitude">longitude</a> shortly after their formation, but contracted rapidly during their first decade; their length stabilized at 10 degrees or less after 1965.<a href="#cite_note-Rogers3-149">[149]</a> Although they originated as segments of the STZ, they evolved to become completely embedded in the South Temperate Belt, suggesting that they moved north, "digging" a niche into the STB.<a href="#cite_note-150">[150]</a> Indeed, much like the GRS, their circulations were confined by two opposing <a href="/wiki/Jet_stream" title="Jet stream">jet streams</a> on their northern and southern boundaries, with an eastward jet to their north and a retrograde westward one to the south.<a href="#cite_note-Rogers3-149">[149]</a> The longitudinal movement of the ovals seemed to be influenced by two factors: Jupiter's position in its <a href="/wiki/Orbit" title="Orbit">orbit</a> (they became faster at <a href="/wiki/Aphelion" class="mw-redirect" title="Aphelion">aphelion</a>), and their proximity to the GRS (they accelerated when within 50 degrees of the Spot).<a href="#cite_note-151">[151]</a> The overall trend of the white oval drift rate was deceleration, with a decrease by half between 1940 and 1990.<a href="#cite_note-152">[152]</a> During the Voyager fly-bys, the ovals extended roughly 9000 km from east to west, 5000 km from north to south, and rotated every five days (compared to six for the GRS at the time).<a href="#cite_note-153">[153]</a> <div class="mw-heading mw-heading2"><h2 id="See_also">See also</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=22" title="Edit section: See also">edit</a>]</div> <style data-mw-deduplicate="TemplateStyles:r1239009302">.mw-parser-output .portalbox{padding:0;margin:0.5em 0;display:table;box-sizing:border-box;max-width:175px;list-style:none}.mw-parser-output .portalborder{border:1px solid var(--border-color-base,#a2a9b1);padding:0.1em;background:var(--background-color-neutral-subtle,#f8f9fa)}.mw-parser-output .portalbox-entry{display:table-row;font-size:85%;line-height:110%;height:1.9em;font-style:italic;font-weight:bold}.mw-parser-output .portalbox-image{display:table-cell;padding:0.2em;vertical-align:middle;text-align:center}.mw-parser-output .portalbox-link{display:table-cell;padding:0.2em 0.2em 0.2em 0.3em;vertical-align:middle}@media(min-width:720px){.mw-parser-output .portalleft{clear:left;float:left;margin:0.5em 1em 0.5em 0}.mw-parser-output .portalright{clear:right;float:right;margin:0.5em 0 0.5em 1em}}</style><ul role="navigation" aria-label="Portals" class="noprint portalbox portalborder portalright"> <li class="portalbox-entry"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/22px-Solar_system.jpg" decoding="async" width="22" height="28" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/34px-Solar_system.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/45px-Solar_system.jpg 2x" data-file-width="4500" data-file-height="5600" /><a href="/wiki/Portal:Solar_System" title="Portal:Solar System">Solar System portal</a></li></ul> <ul><li><a href="/wiki/Comet_Shoemaker%E2%80%93Levy_9" title="Comet Shoemaker–Levy 9">Comet Shoemaker–Levy 9</a></li> <li><a href="/wiki/Extrasolar_planet" class="mw-redirect" title="Extrasolar planet">Extrasolar planet</a> (many <a href="/wiki/List_of_extrasolar_planets#Planet_data_table" class="mw-redirect" title="List of extrasolar planets">larger than Jupiter</a>)</li> <li><a href="/wiki/Galileo_Spacecraft" class="mw-redirect" title="Galileo Spacecraft">Galileo Spacecraft</a> (a mission that included both an orbiter and an <a href="/wiki/Galileo_Probe" class="mw-redirect" title="Galileo Probe">atmospheric-entry probe</a>)</li> <li><a href="/wiki/Juno_(spacecraft)" title="Juno (spacecraft)">Juno</a> probe</li> <li><a href="/wiki/2009_Jupiter_impact_event" title="2009 Jupiter impact event">2009 Jupiter impact event</a></li> <li><a href="/wiki/2010_Jupiter_impact_event" title="2010 Jupiter impact event">2010 Jupiter impact event</a></li> <li><a href="/wiki/Ulysses_(spacecraft)" title="Ulysses (spacecraft)">Ulysses (spacecraft)</a></li> <li><a href="/wiki/Voyager_1" title="Voyager 1">Voyager 1</a>, <a href="/wiki/Voyager_2" title="Voyager 2">Voyager 2</a></li></ul> <div style="clear:both;" class=""></div> <div class="mw-heading mw-heading2"><h2 id="Notes">Notes</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=23" title="Edit section: Notes">edit</a>]</div> <style data-mw-deduplicate="TemplateStyles:r1239549316">.mw-parser-output .refbegin{margin-bottom:0.5em}.mw-parser-output .refbegin-hanging-indents>ul{margin-left:0}.mw-parser-output .refbegin-hanging-indents>ul>li{margin-left:0;padding-left:3.2em;text-indent:-3.2em}.mw-parser-output .refbegin-hanging-indents ul,.mw-parser-output .refbegin-hanging-indents ul li{list-style:none}@media(max-width:720px){.mw-parser-output .refbegin-hanging-indents>ul>li{padding-left:1.6em;text-indent:-1.6em}}.mw-parser-output .refbegin-columns{margin-top:0.3em}.mw-parser-output .refbegin-columns ul{margin-top:0}.mw-parser-output .refbegin-columns li{page-break-inside:avoid;break-inside:avoid-column}@media screen{.mw-parser-output .refbegin{font-size:90%}}</style><div class="refbegin" style=""> <ol type="a"> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#ref_Anone">^</a> The scale height sh is defined as sh = RT/(Mgj), where R = 8.31 J/mol/K is the <a href="/wiki/Gas_constant" title="Gas constant">gas constant</a>, M ≈ 0.0023 kg/mol is the average molar mass in the Jovian atmosphere,<a href="#cite_note-Sieff1998-3">[3]</a> T is temperature and gj ≈ 25 m/s2 is the gravitational acceleration at the surface of Jupiter. As the temperature varies from 110 K in the tropopause up to 1000 K in the thermosphere,<a href="#cite_note-Sieff1998-3">[3]</a> the scale height can assume values from 15 to 150 km. </li><li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#ref_Bnone">^</a> The Galileo atmospheric probe failed to measure the deep abundance of oxygen, because the water concentration continued to increase down to the pressure level of 22 bar, when it ceased operating. While the actually measured oxygen abundances are much lower than the solar value, the observed rapid increase of water content of the atmosphere with depth makes it highly likely that the deep abundance of oxygen indeed exceeds the solar value by a factor of about 3—much like other elements.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> </li><li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#ref_Cnone">^</a> Various explanations of the overabundance of carbon, oxygen, nitrogen and other elements have been proposed. The leading one is that Jupiter captured a large number of icy <a href="/wiki/Planetesimal" title="Planetesimal">planetesimals</a> during the later stages of its accretion. The volatiles like noble gases are thought to have been trapped as <a href="/wiki/Clathrate_hydrates" class="mw-redirect" title="Clathrate hydrates">clathrate hydrates</a> in water ice.<a href="#cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">[1]</a> </li><li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1041539562"><a href="#ref_Dnone">^</a> NASA's <a href="/wiki/Hubble_Space_Telescope" title="Hubble Space Telescope">Hubble Space Telescope</a> recorded on 25 August 2020, a storm traveling around the planet at 350 miles per hour (560 km/h).<a href="#cite_note-154">[154]</a> In addition, researches from the <a href="/wiki/California_Institute_of_Technology" title="California Institute of Technology">California Institute of Technology</a> reported that storms on Jupiter are similar to those on Earth, which form close to the equator, then move towards the poles. However, Jupiter's storms do not experience any friction from the land or oceans; hence, they drift until they reach the poles, which generate the so-called <a href="/wiki/Polygon" title="Polygon">polygon</a> storms.<a href="#cite_note-155">[155]</a> </li> </ol> </div> <div class="mw-heading mw-heading2"><h2 id="References">References</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=24" title="Edit section: References">edit</a>]</div> <style data-mw-deduplicate="TemplateStyles:r1239543626">.mw-parser-output .reflist{margin-bottom:0.5em;list-style-type:decimal}@media screen{.mw-parser-output .reflist{font-size:90%}}.mw-parser-output .reflist .references{font-size:100%;margin-bottom:0;list-style-type:inherit}.mw-parser-output .reflist-columns-2{column-width:30em}.mw-parser-output .reflist-columns-3{column-width:25em}.mw-parser-output .reflist-columns{margin-top:0.3em}.mw-parser-output .reflist-columns ol{margin-top:0}.mw-parser-output .reflist-columns li{page-break-inside:avoid;break-inside:avoid-column}.mw-parser-output .reflist-upper-alpha{list-style-type:upper-alpha}.mw-parser-output .reflist-upper-roman{list-style-type:upper-roman}.mw-parser-output .reflist-lower-alpha{list-style-type:lower-alpha}.mw-parser-output .reflist-lower-greek{list-style-type:lower-greek}.mw-parser-output .reflist-lower-roman{list-style-type:lower-roman}</style><div class="reflist reflist-columns references-column-width" style="column-width: 25em;"> <ol class="references"> <li id="cite_note-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1">^ <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-0">a</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-1">b</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-2">c</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-3">d</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-4">e</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-5">f</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-6">g</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-7">h</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-8">i</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-9">j</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-10">k</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-11">l</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-12">m</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-13">n</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-14">o</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-15">p</a> <a href="#cite_ref-FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003_1-16">q</a> <a href="#CITEREFAtreya_Mahaffy_Niemann_et_al.2003">Atreya Mahaffy Niemann et al. 2003</a>. </li> <li id="cite_note-Guillot1999-2">^ <a href="#cite_ref-Guillot1999_2-0">a</a> <a href="#cite_ref-Guillot1999_2-1">b</a> <a href="#cite_ref-Guillot1999_2-2">c</a> <a href="#cite_ref-Guillot1999_2-3">d</a> <a href="#Guillot">Guillot (1999)</a> </li> <li id="cite_note-Sieff1998-3">^ <a href="#cite_ref-Sieff1998_3-0">a</a> <a href="#cite_ref-Sieff1998_3-1">b</a> <a href="#cite_ref-Sieff1998_3-2">c</a> <a href="#cite_ref-Sieff1998_3-3">d</a> <a href="#cite_ref-Sieff1998_3-4">e</a> <a href="#cite_ref-Sieff1998_3-5">f</a> <a href="#cite_ref-Sieff1998_3-6">g</a> <a href="#Sieff">Sieff et al. (1998)</a> </li> <li id="cite_note-FOOTNOTEAtreyaWong2005-4"><a href="#cite_ref-FOOTNOTEAtreyaWong2005_4-0">^</a> <a href="#CITEREFAtreyaWong2005">Atreya & Wong 2005</a>. </li> <li id="cite_note-Ingersoll1-5">^ <a href="#cite_ref-Ingersoll1_5-0">a</a> <a href="#cite_ref-Ingersoll1_5-1">b</a> <a href="#cite_ref-Ingersoll1_5-2">c</a> <a href="#cite_ref-Ingersoll1_5-3">d</a> <a href="#cite_ref-Ingersoll1_5-4">e</a> <a href="#cite_ref-Ingersoll1_5-5">f</a> <a href="#cite_ref-Ingersoll1_5-6">g</a> <a href="#cite_ref-Ingersoll1_5-7">h</a> <a href="#cite_ref-Ingersoll1_5-8">i</a> <a href="#cite_ref-Ingersoll1_5-9">j</a> <a href="#cite_ref-Ingersoll1_5-10">k</a> <a href="#cite_ref-Ingersoll1_5-11">l</a> <a href="#Ingersoll">Ingersoll (2004)</a>, pp. 2–5 </li> <li id="cite_note-1942Vasavada-6">^ <a href="#cite_ref-1942Vasavada_6-0">a</a> <a href="#cite_ref-1942Vasavada_6-1">b</a> <a href="#cite_ref-1942Vasavada_6-2">c</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1942–1974 </li> <li id="cite_note-1974Vasavada-7">^ <a href="#cite_ref-1974Vasavada_7-0">a</a> <a href="#cite_ref-1974Vasavada_7-1">b</a> <a href="#cite_ref-1974Vasavada_7-2">c</a> <a href="#cite_ref-1974Vasavada_7-3">d</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1974 </li> <li id="cite_note-1978bVasavada-8">^ <a href="#cite_ref-1978bVasavada_8-0">a</a> <a href="#cite_ref-1978bVasavada_8-1">b</a> <a href="#cite_ref-1978bVasavada_8-2">c</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1978–1980 </li> <li id="cite_note-1980Vasavada-9">^ <a href="#cite_ref-1980Vasavada_9-0">a</a> <a href="#cite_ref-1980Vasavada_9-1">b</a> <a href="#cite_ref-1980Vasavada_9-2">c</a> <a href="#cite_ref-1980Vasavada_9-3">d</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1980–1982 </li> <li id="cite_note-1976Vasavada-10">^ <a href="#cite_ref-1976Vasavada_10-0">a</a> <a href="#cite_ref-1976Vasavada_10-1">b</a> <a href="#cite_ref-1976Vasavada_10-2">c</a> <a href="#cite_ref-1976Vasavada_10-3">d</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1976 </li> <li id="cite_note-11"><a href="#cite_ref-11">^</a> <style data-mw-deduplicate="TemplateStyles:r1238218222">.mw-parser-output cite.citation{font-style:inherit;word-wrap:break-word}.mw-parser-output .citation q{quotes:"\"""\"""'""'"}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}.mw-parser-output .id-lock-free.id-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/6/65/Lock-green.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-limited.id-lock-limited a,.mw-parser-output .id-lock-registration.id-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/d/d6/Lock-gray-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-subscription.id-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/a/aa/Lock-red-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .cs1-ws-icon a{background:url("//upload.wikimedia.org/wikipedia/commons/4/4c/Wikisource-logo.svg")right 0.1em center/12px no-repeat}body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-free a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-limited a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-registration a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-subscription a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .cs1-ws-icon a{background-size:contain;padding:0 1em 0 0}.mw-parser-output .cs1-code{color:inherit;background:inherit;border:none;padding:inherit}.mw-parser-output .cs1-hidden-error{display:none;color:var(--color-error,#d33)}.mw-parser-output .cs1-visible-error{color:var(--color-error,#d33)}.mw-parser-output .cs1-maint{display:none;color:#085;margin-left:0.3em}.mw-parser-output .cs1-kern-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right{padding-right:0.2em}.mw-parser-output .citation .mw-selflink{font-weight:inherit}@media screen{.mw-parser-output .cs1-format{font-size:95%}html.skin-theme-clientpref-night .mw-parser-output .cs1-maint{color:#18911f}}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .cs1-maint{color:#18911f}}</style><cite id="CITEREFSmithSoderblomJohnsonIngersoll1979" class="citation journal cs1">Smith, Bradford A.; Soderblom, Laurence A.; Johnson, Torrence V.; Ingersoll, Andrew P.; Collins, Stewart A.; Shoemaker, Eugene M.; Hunt, G. E.; Masursky, Harold; Carr, Michael H. (1979-06-01). "The Jupiter System Through the Eyes of Voyager 1". Science. 204 (4396): 951–972. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1979Sci...204..951S">1979Sci...204..951S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.204.4396.951">10.1126/science.204.4396.951</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0036-8075">0036-8075</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/17800430">17800430</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:33147728">33147728</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=The+Jupiter+System+Through+the+Eyes+of+Voyager+1&rft.volume=204&rft.issue=4396&rft.pages=951-972&rft.date=1979-06-01&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A33147728%23id-name%3DS2CID&rft_id=info%3Abibcode%2F1979Sci...204..951S&rft.issn=0036-8075&rft_id=info%3Adoi%2F10.1126%2Fscience.204.4396.951&rft_id=info%3Apmid%2F17800430&rft.aulast=Smith&rft.aufirst=Bradford+A.&rft.au=Soderblom%2C+Laurence+A.&rft.au=Johnson%2C+Torrence+V.&rft.au=Ingersoll%2C+Andrew+P.&rft.au=Collins%2C+Stewart+A.&rft.au=Shoemaker%2C+Eugene+M.&rft.au=Hunt%2C+G.+E.&rft.au=Masursky%2C+Harold&rft.au=Carr%2C+Michael+H.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-:0-12">^ <a href="#cite_ref-:0_12-0">a</a> <a href="#cite_ref-:0_12-1">b</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFBeckerAlexanderAtreyaBolton2020" class="citation journal cs1"><a href="/wiki/Heidi_N._Becker" title="Heidi N. Becker">Becker, Heidi N.</a>; Alexander, James W.; Atreya, Sushil K.; Bolton, Scott J.; Brennan, Martin J.; Brown, Shannon T.; Guillaume, Alexandre; Guillot, Tristan; Ingersoll, Andrew P.; Levin, Steven M.; Lunine, Jonathan I. (5 August 2020). <a rel="nofollow" class="external text" href="https://www.nature.com/articles/s41586-020-2532-1">"Small lightning flashes from shallow electrical storms on Jupiter"</a>. Nature. 584 (7819): 55–58. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2020Natur.584...55B">2020Natur.584...55B</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fs41586-020-2532-1">10.1038/s41586-020-2532-1</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1476-4687">1476-4687</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/32760043">32760043</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:220980694">220980694</a>. Retrieved 17 January 2021.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Small+lightning+flashes+from+shallow+electrical+storms+on+Jupiter&rft.volume=584&rft.issue=7819&rft.pages=55-58&rft.date=2020-08-05&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A220980694%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2020Natur.584...55B&rft.issn=1476-4687&rft_id=info%3Adoi%2F10.1038%2Fs41586-020-2532-1&rft_id=info%3Apmid%2F32760043&rft.aulast=Becker&rft.aufirst=Heidi+N.&rft.au=Alexander%2C+James+W.&rft.au=Atreya%2C+Sushil+K.&rft.au=Bolton%2C+Scott+J.&rft.au=Brennan%2C+Martin+J.&rft.au=Brown%2C+Shannon+T.&rft.au=Guillaume%2C+Alexandre&rft.au=Guillot%2C+Tristan&rft.au=Ingersoll%2C+Andrew+P.&rft.au=Levin%2C+Steven+M.&rft.au=Lunine%2C+Jonathan+I.&rft_id=https%3A%2F%2Fwww.nature.com%2Farticles%2Fs41586-020-2532-1&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-13"><a href="#cite_ref-13">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGilesGreathouseBonfondGladstone2020" class="citation journal cs1">Giles, Rohini S.; Greathouse, Thomas K.; Bonfond, Bertrand; Gladstone, G. Randall; Kammer, Joshua A.; Hue, Vincent; Grodent, Denis C.; Gérard, Jean-Claude; Versteeg, Maarten H.; Wong, Michael H.; Bolton, Scott J. (2020). <a rel="nofollow" class="external text" href="https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2020JE006659">"Possible Transient Luminous Events Observed in Jupiter's Upper Atmosphere"</a>. Journal of Geophysical Research: Planets. 125 (11): e2020JE006659. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2010.13740">2010.13740</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2020JGRE..12506659G">2020JGRE..12506659G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2020JE006659">10.1029/2020JE006659</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/2268%2F252816">2268/252816</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/2169-9100">2169-9100</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:225075904">225075904</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+Geophysical+Research%3A+Planets&rft.atitle=Possible+Transient+Luminous+Events+Observed+in+Jupiter%27s+Upper+Atmosphere&rft.volume=125&rft.issue=11&rft.pages=e2020JE006659&rft.date=2020&rft_id=info%3Ahdl%2F2268%2F252816&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A225075904%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2020JGRE..12506659G&rft_id=info%3Aarxiv%2F2010.13740&rft.issn=2169-9100&rft_id=info%3Adoi%2F10.1029%2F2020JE006659&rft.aulast=Giles&rft.aufirst=Rohini+S.&rft.au=Greathouse%2C+Thomas+K.&rft.au=Bonfond%2C+Bertrand&rft.au=Gladstone%2C+G.+Randall&rft.au=Kammer%2C+Joshua+A.&rft.au=Hue%2C+Vincent&rft.au=Grodent%2C+Denis+C.&rft.au=G%C3%A9rard%2C+Jean-Claude&rft.au=Versteeg%2C+Maarten+H.&rft.au=Wong%2C+Michael+H.&rft.au=Bolton%2C+Scott+J.&rft_id=https%3A%2F%2Fagupubs.onlinelibrary.wiley.com%2Fdoi%2Fabs%2F10.1029%2F2020JE006659&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Ingersoll7-14">^ <a href="#cite_ref-Ingersoll7_14-0">a</a> <a href="#cite_ref-Ingersoll7_14-1">b</a> <a href="#Ingersoll">Ingersoll (2004)</a>, pp. 13–14 </li> <li id="cite_note-Yelle1-15"><a href="#cite_ref-Yelle1_15-0">^</a> <a href="#Yelle">Yelle (2004)</a>, p. 1 </li> <li id="cite_note-FOOTNOTEMiller_Aylward_et_al.2005-16">^ <a href="#cite_ref-FOOTNOTEMiller_Aylward_et_al.2005_16-0">a</a> <a href="#cite_ref-FOOTNOTEMiller_Aylward_et_al.2005_16-1">b</a> <a href="#cite_ref-FOOTNOTEMiller_Aylward_et_al.2005_16-2">c</a> <a href="#cite_ref-FOOTNOTEMiller_Aylward_et_al.2005_16-3">d</a> <a href="#cite_ref-FOOTNOTEMiller_Aylward_et_al.2005_16-4">e</a> <a href="#cite_ref-FOOTNOTEMiller_Aylward_et_al.2005_16-5">f</a> <a href="#CITEREFMiller_Aylward_et_al.2005">Miller Aylward et al. 2005</a>. </li> <li id="cite_note-Ingersoll4-17">^ <a href="#cite_ref-Ingersoll4_17-0">a</a> <a href="#cite_ref-Ingersoll4_17-1">b</a> <a href="#cite_ref-Ingersoll4_17-2">c</a> <a href="#Ingersoll">Ingersoll (2004)</a>, pp. 5–7 </li> <li id="cite_note-Ingersoll3-18">^ <a href="#cite_ref-Ingersoll3_18-0">a</a> <a href="#cite_ref-Ingersoll3_18-1">b</a> <a href="#cite_ref-Ingersoll3_18-2">c</a> <a href="#Ingersoll">Ingersoll (2004)</a>, p. 12 </li> <li id="cite_note-Yelle3-19">^ <a href="#cite_ref-Yelle3_19-0">a</a> <a href="#cite_ref-Yelle3_19-1">b</a> <a href="#Yelle">Yelle (2004)</a>, pp. 15–16 </li> <li id="cite_note-FOOTNOTEAtreya_Wong_Baines_et_al.2005-20">^ <a href="#cite_ref-FOOTNOTEAtreya_Wong_Baines_et_al.2005_20-0">a</a> <a href="#cite_ref-FOOTNOTEAtreya_Wong_Baines_et_al.2005_20-1">b</a> <a href="#cite_ref-FOOTNOTEAtreya_Wong_Baines_et_al.2005_20-2">c</a> <a href="#CITEREFAtreya_Wong_Baines_et_al.2005">Atreya Wong Baines et al. 2005</a>. </li> <li id="cite_note-FOOTNOTEAtreya_Wong_Owen_et_al.1999-21">^ <a href="#cite_ref-FOOTNOTEAtreya_Wong_Owen_et_al.1999_21-0">a</a> <a href="#cite_ref-FOOTNOTEAtreya_Wong_Owen_et_al.1999_21-1">b</a> <a href="#CITEREFAtreya_Wong_Owen_et_al.1999">Atreya Wong Owen et al. 1999</a>. </li> <li id="cite_note-West20-22">^ <a href="#cite_ref-West20_22-0">a</a> <a href="#cite_ref-West20_22-1">b</a> <a href="#West">West et al. (2004)</a>, pp. 9–10, 20–23 </li> <li id="cite_note-1937Vasavada-23">^ <a href="#cite_ref-1937Vasavada_23-0">a</a> <a href="#cite_ref-1937Vasavada_23-1">b</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1937 </li> <li id="cite_note-Ingersoll8-24">^ <a href="#cite_ref-Ingersoll8_24-0">a</a> <a href="#cite_ref-Ingersoll8_24-1">b</a> <a href="#cite_ref-Ingersoll8_24-2">c</a> <a href="#cite_ref-Ingersoll8_24-3">d</a> <a href="#cite_ref-Ingersoll8_24-4">e</a> <a href="#cite_ref-Ingersoll8_24-5">f</a> <a href="#cite_ref-Ingersoll8_24-6">g</a> <a href="#cite_ref-Ingersoll8_24-7">h</a> <a href="#cite_ref-Ingersoll8_24-8">i</a> <a href="#Ingersoll">Ingersoll (2004)</a>, p. 8 </li> <li id="cite_note-Yelle2-25">^ <a href="#cite_ref-Yelle2_25-0">a</a> <a href="#cite_ref-Yelle2_25-1">b</a> <a href="#Yelle">Yelle (2004)</a>, pp. 1–12 </li> <li id="cite_note-Yelle4-26"><a href="#cite_ref-Yelle4_26-0">^</a> <a href="#Yelle">Yelle (2004)</a>, pp. 22–27 </li> <li id="cite_note-FOOTNOTEBhardwajGladstone2000299–302-27">^ <a href="#cite_ref-FOOTNOTEBhardwajGladstone2000299–302_27-0">a</a> <a href="#cite_ref-FOOTNOTEBhardwajGladstone2000299–302_27-1">b</a> <a href="#CITEREFBhardwajGladstone2000">Bhardwaj & Gladstone 2000</a>, pp. 299–302. </li> <li id="cite_note-28"><a href="#cite_ref-28">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMcDowell1995" class="citation web cs1">McDowell, Jonathan (1995-12-08). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20110810051445/http://www.planet4589.org/space/jsr/back/news.267">"Jonathan's Space Report, No. 267"</a>. <a href="/wiki/Harvard-Smithsonian_Center_for_Astrophysics" class="mw-redirect" title="Harvard-Smithsonian Center for Astrophysics">Harvard-Smithsonian Center for Astrophysics</a>. Archived from <a rel="nofollow" class="external text" href="http://www.planet4589.org/space/jsr/back/news.267">the original</a> on 2011-08-10. Retrieved 2007-05-06.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Jonathan%27s+Space+Report%2C+No.+267&rft.pub=Harvard-Smithsonian+Center+for+Astrophysics&rft.date=1995-12-08&rft.aulast=McDowell&rft.aufirst=Jonathan&rft_id=http%3A%2F%2Fwww.planet4589.org%2Fspace%2Fjsr%2Fback%2Fnews.267&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-FOOTNOTEEncrenaz2003-29">^ <a href="#cite_ref-FOOTNOTEEncrenaz2003_29-0">a</a> <a href="#cite_ref-FOOTNOTEEncrenaz2003_29-1">b</a> <a href="#cite_ref-FOOTNOTEEncrenaz2003_29-2">c</a> <a href="#CITEREFEncrenaz2003">Encrenaz 2003</a>. </li> <li id="cite_note-Kunde2004-30"><a href="#cite_ref-Kunde2004_30-0">^</a> <a href="#Kunde">Kunde et al. (2004)</a> </li> <li id="cite_note-Sanders2010-31"><a href="#cite_ref-Sanders2010_31-0">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFSanders2010" class="citation web cs1">Sanders, Robert (22 March 2010). <a rel="nofollow" class="external text" href="http://newscenter.berkeley.edu/2010/03/22/helium_rain/">"Helium rain on Jupiter explains lack of neon in atmosphere"</a>. University of Berkeley. Retrieved 24 July 2012.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Helium+rain+on+Jupiter+explains+lack+of+neon+in+atmosphere&rft.pub=University+of+Berkeley&rft.date=2010-03-22&rft.aulast=Sanders&rft.aufirst=Robert&rft_id=http%3A%2F%2Fnewscenter.berkeley.edu%2F2010%2F03%2F22%2Fhelium_rain%2F&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Rogers1-32">^ <a href="#cite_ref-Rogers1_32-0">a</a> <a href="#cite_ref-Rogers1_32-1">b</a> <a href="#Rogers">Rogers (1995)</a>, p. 81. </li> <li id="cite_note-33"><a href="#cite_ref-33">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFKaspiGalantiHubbardStevenson2018" class="citation journal cs1">Kaspi, Y.; Galanti, E.; Hubbard, W. B.; Stevenson, D. J.; Bolton, S. J.; Iess, L.; Guillot, T.; Bloxham, J.; Connerney, J. E. P.; Cao, H.; Durante, D. (2018-03-08). <a rel="nofollow" class="external text" href="http://www.nature.com/articles/nature25793">"Jupiter's atmospheric jet streams extend thousands of kilometres deep"</a>. Nature. 555 (7695): 223–226. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2018Natur.555..223K">2018Natur.555..223K</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fnature25793">10.1038/nature25793</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/11573%2F1091959">11573/1091959</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0028-0836">0028-0836</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/29516995">29516995</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:4120368">4120368</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Jupiter%27s+atmospheric+jet+streams+extend+thousands+of+kilometres+deep&rft.volume=555&rft.issue=7695&rft.pages=223-226&rft.date=2018-03-08&rft_id=info%3Ahdl%2F11573%2F1091959&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A4120368%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2018Natur.555..223K&rft.issn=0028-0836&rft_id=info%3Adoi%2F10.1038%2Fnature25793&rft_id=info%3Apmid%2F29516995&rft.aulast=Kaspi&rft.aufirst=Y.&rft.au=Galanti%2C+E.&rft.au=Hubbard%2C+W.+B.&rft.au=Stevenson%2C+D.+J.&rft.au=Bolton%2C+S.+J.&rft.au=Iess%2C+L.&rft.au=Guillot%2C+T.&rft.au=Bloxham%2C+J.&rft.au=Connerney%2C+J.+E.+P.&rft.au=Cao%2C+H.&rft.au=Durante%2C+D.&rft_id=http%3A%2F%2Fwww.nature.com%2Farticles%2Fnature25793&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-34"><a href="#cite_ref-34">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGalantiKaspiDuerFletcher2021" class="citation journal cs1">Galanti, Eli; Kaspi, Yohai; Duer, Keren; Fletcher, Leigh; Ingersoll, Andrew P.; Li, Cheng; Orton, Glenn S.; Guillot, Tristan; Levin, Steven M.; Bolton, Scott J. (2021). <a rel="nofollow" class="external text" href="https://onlinelibrary.wiley.com/doi/10.1029/2021GL092912">"Constraints on the Latitudinal Profile of Jupiter's Deep Jets"</a>. Geophysical Research Letters. 48 (9). <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2102.10595">2102.10595</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021GeoRL..4892912G">2021GeoRL..4892912G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2021GL092912">10.1029/2021GL092912</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/2027.42%2F167748">2027.42/167748</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0094-8276">0094-8276</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:231985747">231985747</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Geophysical+Research+Letters&rft.atitle=Constraints+on+the+Latitudinal+Profile+of+Jupiter%27s+Deep+Jets&rft.volume=48&rft.issue=9&rft.date=2021&rft_id=info%3Ahdl%2F2027.42%2F167748&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A231985747%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2021GeoRL..4892912G&rft_id=info%3Aarxiv%2F2102.10595&rft.issn=0094-8276&rft_id=info%3Adoi%2F10.1029%2F2021GL092912&rft.aulast=Galanti&rft.aufirst=Eli&rft.au=Kaspi%2C+Yohai&rft.au=Duer%2C+Keren&rft.au=Fletcher%2C+Leigh&rft.au=Ingersoll%2C+Andrew+P.&rft.au=Li%2C+Cheng&rft.au=Orton%2C+Glenn+S.&rft.au=Guillot%2C+Tristan&rft.au=Levin%2C+Steven+M.&rft.au=Bolton%2C+Scott+J.&rft_id=https%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1029%2F2021GL092912&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-35"><a href="#cite_ref-35">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFBusse1976" class="citation journal cs1">Busse, F.H. (1976). <a rel="nofollow" class="external text" href="https://linkinghub.elsevier.com/retrieve/pii/0019103576900531">"A simple model of convection in the Jovian atmosphere"</a>. Icarus. 29 (2): 255–260. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1976Icar...29..255B">1976Icar...29..255B</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2F0019-1035%2876%2990053-1">10.1016/0019-1035(76)90053-1</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=A+simple+model+of+convection+in+the+Jovian+atmosphere&rft.volume=29&rft.issue=2&rft.pages=255-260&rft.date=1976&rft_id=info%3Adoi%2F10.1016%2F0019-1035%2876%2990053-1&rft_id=info%3Abibcode%2F1976Icar...29..255B&rft.aulast=Busse&rft.aufirst=F.H.&rft_id=https%3A%2F%2Flinkinghub.elsevier.com%2Fretrieve%2Fpii%2F0019103576900531&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Ingersoll2-36">^ <a href="#cite_ref-Ingersoll2_36-0">a</a> <a href="#cite_ref-Ingersoll2_36-1">b</a> <a href="#Ingersoll">Ingersoll (2004)</a>, p. 5 </li> <li id="cite_note-37"><a href="#cite_ref-37">^</a> <a href="#Graney">Graney</a> (2010) </li> <li id="cite_note-38"><a href="#cite_ref-38">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFJames_R._Holton2004" class="citation book cs1">James R. Holton, ed. (2004). An introduction to dynamic meteorology (4th ed.). Burlington, MA: Elsevier Academic Press. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-08-047021-4" title="Special:BookSources/978-0-08-047021-4"><bdi>978-0-08-047021-4</bdi></a>. <a href="/wiki/OCLC_(identifier)" class="mw-redirect" title="OCLC (identifier)">OCLC</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/oclc/162572802">162572802</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=An+introduction+to+dynamic+meteorology&rft.place=Burlington%2C+MA&rft.edition=4th&rft.pub=Elsevier+Academic+Press&rft.date=2004&rft_id=info%3Aoclcnum%2F162572802&rft.isbn=978-0-08-047021-4&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-39"><a href="#cite_ref-39">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFFletcherKaspiGuillotShowman2020" class="citation journal cs1">Fletcher, Leigh N.; Kaspi, Yohai; Guillot, Tristan; Showman, Adam P. (2020-03-12). <a rel="nofollow" class="external text" href="https://doi.org/10.1007/s11214-019-0631-9">"How Well Do We Understand the Belt/Zone Circulation of Giant Planet Atmospheres?"</a>. Space Science Reviews. 216 (2): 30. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/1907.01822">1907.01822</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2020SSRv..216...30F">2020SSRv..216...30F</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1007%2Fs11214-019-0631-9">10.1007/s11214-019-0631-9</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1572-9672">1572-9672</a>. <a href="/wiki/PMC_(identifier)" class="mw-redirect" title="PMC (identifier)">PMC</a> <a rel="nofollow" class="external text" href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7067733">7067733</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/32214508">32214508</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Space+Science+Reviews&rft.atitle=How+Well+Do+We+Understand+the+Belt%2FZone+Circulation+of+Giant+Planet+Atmospheres%3F&rft.volume=216&rft.issue=2&rft.pages=30&rft.date=2020-03-12&rft_id=https%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpmc%2Farticles%2FPMC7067733%23id-name%3DPMC&rft_id=info%3Abibcode%2F2020SSRv..216...30F&rft_id=info%3Aarxiv%2F1907.01822&rft.issn=1572-9672&rft_id=info%3Adoi%2F10.1007%2Fs11214-019-0631-9&rft_id=info%3Apmid%2F32214508&rft.aulast=Fletcher&rft.aufirst=Leigh+N.&rft.au=Kaspi%2C+Yohai&rft.au=Guillot%2C+Tristan&rft.au=Showman%2C+Adam+P.&rft_id=https%3A%2F%2Fdoi.org%2F10.1007%2Fs11214-019-0631-9&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-40"><a href="#cite_ref-40">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFShowmande_Pater2005" class="citation journal cs1">Showman, Adam P.; de Pater, Imke (2005). <a rel="nofollow" class="external text" href="https://linkinghub.elsevier.com/retrieve/pii/S0019103504003562">"Dynamical implications of Jupiter's tropospheric ammonia abundance"</a>. Icarus. 174 (1): 192–204. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005Icar..174..192S">2005Icar..174..192S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.icarus.2004.10.004">10.1016/j.icarus.2004.10.004</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=Dynamical+implications+of+Jupiter%27s+tropospheric+ammonia+abundance&rft.volume=174&rft.issue=1&rft.pages=192-204&rft.date=2005&rft_id=info%3Adoi%2F10.1016%2Fj.icarus.2004.10.004&rft_id=info%3Abibcode%2F2005Icar..174..192S&rft.aulast=Showman&rft.aufirst=Adam+P.&rft.au=de+Pater%2C+Imke&rft_id=https%3A%2F%2Flinkinghub.elsevier.com%2Fretrieve%2Fpii%2FS0019103504003562&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-41"><a href="#cite_ref-41">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFIngersollGieraschBanfieldVasavada2000" class="citation journal cs1">Ingersoll, A. P.; Gierasch, P. J.; Banfield, D.; Vasavada, A. R.; Galileo Imaging Team (2000). <a rel="nofollow" class="external text" href="http://www.nature.com/articles/35001021">"Moist convection as an energy source for the large-scale motions in Jupiter's atmosphere"</a>. Nature. 403 (6770): 630–632. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2000Natur.403..630I">2000Natur.403..630I</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2F35001021">10.1038/35001021</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0028-0836">0028-0836</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/10688192">10688192</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:4381087">4381087</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Moist+convection+as+an+energy+source+for+the+large-scale+motions+in+Jupiter%27s+atmosphere&rft.volume=403&rft.issue=6770&rft.pages=630-632&rft.date=2000&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A4381087%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2000Natur.403..630I&rft.issn=0028-0836&rft_id=info%3Adoi%2F10.1038%2F35001021&rft_id=info%3Apmid%2F10688192&rft.aulast=Ingersoll&rft.aufirst=A.+P.&rft.au=Gierasch%2C+P.+J.&rft.au=Banfield%2C+D.&rft.au=Vasavada%2C+A.+R.&rft.au=Galileo+Imaging+Team&rft_id=http%3A%2F%2Fwww.nature.com%2Farticles%2F35001021&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-42"><a href="#cite_ref-42">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFJanssenOswaldBrownGulkis2017" class="citation journal cs1">Janssen, M. A.; Oswald, J. E.; Brown, S. T.; Gulkis, S.; Levin, S. M.; Bolton, S. J.; Allison, M. D.; Atreya, S. K.; Gautier, D.; Ingersoll, A. P.; Lunine, J. I. (2017). <a rel="nofollow" class="external text" href="http://link.springer.com/10.1007/s11214-017-0349-5">"MWR: Microwave Radiometer for the Juno Mission to Jupiter"</a>. Space Science Reviews. 213 (1–4): 139–185. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2017SSRv..213..139J">2017SSRv..213..139J</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1007%2Fs11214-017-0349-5">10.1007/s11214-017-0349-5</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0038-6308">0038-6308</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:125905820">125905820</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Space+Science+Reviews&rft.atitle=MWR%3A+Microwave+Radiometer+for+the+Juno+Mission+to+Jupiter&rft.volume=213&rft.issue=1%E2%80%934&rft.pages=139-185&rft.date=2017&rft_id=info%3Adoi%2F10.1007%2Fs11214-017-0349-5&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A125905820%23id-name%3DS2CID&rft.issn=0038-6308&rft_id=info%3Abibcode%2F2017SSRv..213..139J&rft.aulast=Janssen&rft.aufirst=M.+A.&rft.au=Oswald%2C+J.+E.&rft.au=Brown%2C+S.+T.&rft.au=Gulkis%2C+S.&rft.au=Levin%2C+S.+M.&rft.au=Bolton%2C+S.+J.&rft.au=Allison%2C+M.+D.&rft.au=Atreya%2C+S.+K.&rft.au=Gautier%2C+D.&rft.au=Ingersoll%2C+A.+P.&rft.au=Lunine%2C+J.+I.&rft_id=http%3A%2F%2Flink.springer.com%2F10.1007%2Fs11214-017-0349-5&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-:2-43">^ <a href="#cite_ref-:2_43-0">a</a> <a href="#cite_ref-:2_43-1">b</a> <a href="#cite_ref-:2_43-2">c</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFDuerGavrielGalantiKaspi2021" class="citation journal cs1">Duer, Keren; Gavriel, Nimrod; Galanti, Eli; Kaspi, Yohai; Fletcher, Leigh N.; Guillot, Tristan; Bolton, Scott J.; Levin, Steven M.; Atreya, Sushil K.; Grassi, Davide; Ingersoll, Andrew P. (2021-12-16). <a rel="nofollow" class="external text" href="https://onlinelibrary.wiley.com/doi/10.1029/2021GL095651">"Evidence for Multiple Ferrel-Like Cells on Jupiter"</a>. Geophysical Research Letters. 48 (23). <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2110.07255">2110.07255</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021GeoRL..4895651D">2021GeoRL..4895651D</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2021GL095651">10.1029/2021GL095651</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/2027.42%2F170953">2027.42/170953</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0094-8276">0094-8276</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:238856819">238856819</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Geophysical+Research+Letters&rft.atitle=Evidence+for+Multiple+Ferrel-Like+Cells+on+Jupiter&rft.volume=48&rft.issue=23&rft.date=2021-12-16&rft_id=info%3Ahdl%2F2027.42%2F170953&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A238856819%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2021GeoRL..4895651D&rft_id=info%3Aarxiv%2F2110.07255&rft.issn=0094-8276&rft_id=info%3Adoi%2F10.1029%2F2021GL095651&rft.aulast=Duer&rft.aufirst=Keren&rft.au=Gavriel%2C+Nimrod&rft.au=Galanti%2C+Eli&rft.au=Kaspi%2C+Yohai&rft.au=Fletcher%2C+Leigh+N.&rft.au=Guillot%2C+Tristan&rft.au=Bolton%2C+Scott+J.&rft.au=Levin%2C+Steven+M.&rft.au=Atreya%2C+Sushil+K.&rft.au=Grassi%2C+Davide&rft.au=Ingersoll%2C+Andrew+P.&rft_id=https%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1029%2F2021GL095651&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-44"><a href="#cite_ref-44">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFLiuSchneider2010" class="citation journal cs1">Liu, Junjun; Schneider, Tapio (2010-11-01). <a rel="nofollow" class="external text" href="https://journals.ametsoc.org/doi/10.1175/2010JAS3492.1">"Mechanisms of Jet Formation on the Giant Planets"</a>. Journal of the Atmospheric Sciences. 67 (11): 3652–3672. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/0910.3682">0910.3682</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2010JAtS...67.3652L">2010JAtS...67.3652L</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F2010JAS3492.1">10.1175/2010JAS3492.1</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1520-0469">1520-0469</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:9416783">9416783</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Mechanisms+of+Jet+Formation+on+the+Giant+Planets&rft.volume=67&rft.issue=11&rft.pages=3652-3672&rft.date=2010-11-01&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A9416783%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2010JAtS...67.3652L&rft_id=info%3Aarxiv%2F0910.3682&rft.issn=1520-0469&rft_id=info%3Adoi%2F10.1175%2F2010JAS3492.1&rft.aulast=Liu&rft.aufirst=Junjun&rft.au=Schneider%2C+Tapio&rft_id=https%3A%2F%2Fjournals.ametsoc.org%2Fdoi%2F10.1175%2F2010JAS3492.1&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-45"><a href="#cite_ref-45">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 85, 91–4. </li> <li id="cite_note-Rogers2-46">^ <a href="#cite_ref-Rogers2_46-0">a</a> <a href="#cite_ref-Rogers2_46-1">b</a> <a href="#cite_ref-Rogers2_46-2">c</a> <a href="#cite_ref-Rogers2_46-3">d</a> <a href="#Rogers">Rogers (1995)</a>, pp. 101–105. </li> <li id="cite_note-47"><a href="#cite_ref-47">^</a> <a href="#Rogers">Rogers (1995)</a>, pp.113–117. </li> <li id="cite_note-48"><a href="#cite_ref-48">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 125–130. </li> <li id="cite_note-1987Vasavada-49">^ <a href="#cite_ref-1987Vasavada_49-0">a</a> <a href="#cite_ref-1987Vasavada_49-1">b</a> <a href="#cite_ref-1987Vasavada_49-2">c</a> <a href="#cite_ref-1987Vasavada_49-3">d</a> <a href="#cite_ref-1987Vasavada_49-4">e</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1987–1989 </li> <li id="cite_note-50"><a href="#cite_ref-50">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 133, 145–147. </li> <li id="cite_note-51"><a href="#cite_ref-51">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 133. </li> <li id="cite_note-52"><a href="#cite_ref-52">^</a> <a href="#Beebe">Beebe (1997)</a>, p. 24. </li> <li id="cite_note-53"><a href="#cite_ref-53">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFNancy_Atkinson2010" class="citation web cs1">Nancy Atkinson (2010). <a rel="nofollow" class="external text" href="http://www.universetoday.com/2010/05/13/jupiter-it-is-a-changing/">"Jupiter, It Is A-Changing"</a>. Universe Today. Retrieved 2010-12-24.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Jupiter%2C+It+Is+A-Changing&rft.pub=Universe+Today&rft.date=2010&rft.au=Nancy+Atkinson&rft_id=http%3A%2F%2Fwww.universetoday.com%2F2010%2F05%2F13%2Fjupiter-it-is-a-changing%2F&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-54"><a href="#cite_ref-54">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 159–160 </li> <li id="cite_note-55"><a href="#cite_ref-55">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite class="citation web cs1"><a rel="nofollow" class="external text" href="http://www.spacetelescope.org/news/heic1522/">"Hubble's planetary portrait captures changes in Jupiter's Great Red Spot"</a>. Retrieved 15 October 2015.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Hubble%27s+planetary+portrait+captures+changes+in+Jupiter%27s+Great+Red+Spot&rft_id=http%3A%2F%2Fwww.spacetelescope.org%2Fnews%2Fheic1522%2F&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-56"><a href="#cite_ref-56">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 219–221, 223, 228–229. </li> <li id="cite_note-57"><a href="#cite_ref-57">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 235. </li> <li id="cite_note-Rogers2003-58"><a href="#cite_ref-Rogers2003_58-0">^</a> <a href="#Rogers2003">Rogers et al. (2003)</a> </li> <li id="cite_note-Rogers2001-59"><a href="#cite_ref-Rogers2001_59-0">^</a> <a href="#Rogers2001">Rogers and Metig (2001)</a> </li> <li id="cite_note-60"><a href="#cite_ref-60">^</a> <a href="#Ridpath">Ridpath (1998)</a> </li> <li id="cite_note-1943Vasavada-61">^ <a href="#cite_ref-1943Vasavada_61-0">a</a> <a href="#cite_ref-1943Vasavada_61-1">b</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1943–1945 </li> <li id="cite_note-Heimpel2005-62">^ <a href="#cite_ref-Heimpel2005_62-0">a</a> <a href="#cite_ref-Heimpel2005_62-1">b</a> <a href="#Heimpel2005">Heimpel et al. (2005)</a> </li> <li id="cite_note-Ingersoll1969-63"><a href="#cite_ref-Ingersoll1969_63-0">^</a> See, e. g., <a href="#Ingersoll1969">Ingersoll et al. (1969)</a> </li> <li id="cite_note-1947Vasavada-64">^ <a href="#cite_ref-1947Vasavada_64-0">a</a> <a href="#cite_ref-1947Vasavada_64-1">b</a> <a href="#cite_ref-1947Vasavada_64-2">c</a> <a href="#cite_ref-1947Vasavada_64-3">d</a> <a href="#cite_ref-1947Vasavada_64-4">e</a> <a href="#cite_ref-1947Vasavada_64-5">f</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1947–1958 </li> <li id="cite_note-Ingersoll5-65"><a href="#cite_ref-Ingersoll5_65-0">^</a> <a href="#Ingersoll">Ingersoll (2004)</a>, pp. 16–17 </li> <li id="cite_note-Ingersoll6-66"><a href="#cite_ref-Ingersoll6_66-0">^</a> <a href="#Ingersoll">Ingersoll (2004)</a>, pp. 14–15 </li> <li id="cite_note-1949Vasavada-67">^ <a href="#cite_ref-1949Vasavada_67-0">a</a> <a href="#cite_ref-1949Vasavada_67-1">b</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1949 </li> <li id="cite_note-1945Vasavada-68"><a href="#cite_ref-1945Vasavada_68-0">^</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1945–1947 </li> <li id="cite_note-1962Vasavada-69"><a href="#cite_ref-1962Vasavada_69-0">^</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1962–1966 </li> <li id="cite_note-1966Vasavada-70"><a href="#cite_ref-1966Vasavada_70-0">^</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1966 </li> <li id="cite_note-Busse1976-71"><a href="#cite_ref-Busse1976_71-0">^</a> <a href="#Busse">Busse (1976)</a> </li> <li id="cite_note-1966-1Vasavada-72">^ <a href="#cite_ref-1966-1Vasavada_72-0">a</a> <a href="#cite_ref-1966-1Vasavada_72-1">b</a> <a href="#cite_ref-1966-1Vasavada_72-2">c</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1966–1972 </li> <li id="cite_note-1970Vasavada-73"><a href="#cite_ref-1970Vasavada_73-0">^</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1970 </li> <li id="cite_note-Low-74"><a href="#cite_ref-Low_74-0">^</a> <a href="#Low">Low (1966)</a> </li> <li id="cite_note-FOOTNOTEPearl_Conrath_et_al.199012,_26-75"><a href="#cite_ref-FOOTNOTEPearl_Conrath_et_al.199012,_26_75-0">^</a> <a href="#CITEREFPearl_Conrath_et_al.1990">Pearl Conrath et al. 1990</a>, pp. 12, 26. </li> <li id="cite_note-Ingersoll9-76"><a href="#cite_ref-Ingersoll9_76-0">^</a> <a href="#Ingersoll">Ingersoll (2004)</a>, pp. 11, 17–18 </li> <li id="cite_note-1978Vasavada-77">^ <a href="#cite_ref-1978Vasavada_77-0">a</a> <a href="#cite_ref-1978Vasavada_77-1">b</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1978 </li> <li id="cite_note-1977Vasavada-78">^ <a href="#cite_ref-1977Vasavada_78-0">a</a> <a href="#cite_ref-1977Vasavada_78-1">b</a> <a href="#cite_ref-1977Vasavada_78-2">c</a> <a href="#cite_ref-1977Vasavada_78-3">d</a> <a href="#cite_ref-1977Vasavada_78-4">e</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1977 </li> <li id="cite_note-79"><a href="#cite_ref-79">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite class="citation web cs1"><a rel="nofollow" class="external text" href="https://www.eso.org/public/images/potw1716a/">"Great Cold Spot discovered on Jupiter"</a>. www.eso.org. Retrieved 17 April 2017.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=www.eso.org&rft.atitle=Great+Cold+Spot+discovered+on+Jupiter&rft_id=https%3A%2F%2Fwww.eso.org%2Fpublic%2Fimages%2Fpotw1716a%2F&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-80"><a href="#cite_ref-80">^</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1975 </li> <li id="cite_note-1979Vasavada-81"><a href="#cite_ref-1979Vasavada_81-0">^</a> <a href="#Vasavada">Vasavada (2005)</a>, p. 1979 </li> <li id="cite_note-NASA-20140515-82"><a href="#cite_ref-NASA-20140515_82-0">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFHarringtonWeaverVillard2014" class="citation web cs1">Harrington, J.D.; Weaver, Donna; Villard, Ray (May 15, 2014). <a rel="nofollow" class="external text" href="https://www.nasa.gov/press/2014/may/nasas-hubble-shows-jupiters-great-red-spot-is-smaller-than-ever-measured">"Release 14-135 - NASA's Hubble Shows Jupiter's Great Red Spot is Smaller than Ever Measured"</a>. <a href="/wiki/NASA" title="NASA">NASA</a>. Retrieved May 16, 2014.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=NASA&rft.atitle=Release+14-135+-+NASA%27s+Hubble+Shows+Jupiter%27s+Great+Red+Spot+is+Smaller+than+Ever+Measured&rft.date=2014-05-15&rft.aulast=Harrington&rft.aufirst=J.D.&rft.au=Weaver%2C+Donna&rft.au=Villard%2C+Ray&rft_id=http%3A%2F%2Fwww.nasa.gov%2Fpress%2F2014%2Fmay%2Fnasas-hubble-shows-jupiters-great-red-spot-is-smaller-than-ever-measured&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-83"><a href="#cite_ref-83">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFStaff2007" class="citation web cs1">Staff (2007). <a rel="nofollow" class="external text" href="http://www.space.com/scienceastronomy/solarsystem/jupiter-ez.html">"Jupiter Data Sheet – SPACE.com"</a>. Imaginova. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20080511205433/http://www.space.com/scienceastronomy/solarsystem/jupiter-ez.html">Archived</a> from the original on 11 May 2008. Retrieved 2008-06-03.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Jupiter+Data+Sheet+%E2%80%93+SPACE.com&rft.pub=Imaginova&rft.date=2007&rft.au=Staff&rft_id=http%3A%2F%2Fwww.space.com%2Fscienceastronomy%2Fsolarsystem%2Fjupiter-ez.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-84"><a href="#cite_ref-84">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFAnonymous2000" class="citation web cs1">Anonymous (August 10, 2000). <a rel="nofollow" class="external text" href="http://csep10.phys.utk.edu/astr161/lect/jupiter/redspot.html">"The Solar System – The Planet Jupiter – The Great Red Spot"</a>. Dept. Physics & Astronomy – <a href="/wiki/University_of_Tennessee" title="University of Tennessee">University of Tennessee</a>. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20080607102754/http://csep10.phys.utk.edu/astr161/lect/jupiter/redspot.html">Archived</a> from the original on 7 June 2008. Retrieved 2008-06-03.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=The+Solar+System+%E2%80%93+The+Planet+Jupiter+%E2%80%93+The+Great+Red+Spot&rft.pub=Dept.+Physics+%26+Astronomy+%E2%80%93+University+of+Tennessee&rft.date=2000-08-10&rft.au=Anonymous&rft_id=http%3A%2F%2Fcsep10.phys.utk.edu%2Fastr161%2Flect%2Fjupiter%2Fredspot.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-85"><a href="#cite_ref-85">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFRogers1995" class="citation book cs1">Rogers, John Hubert (1995). <a rel="nofollow" class="external text" href="https://books.google.com/books?id=SO48AAAAIAAJ&pg=PA6">The Giant Planet Jupiter</a>. Cambridge University Press. p. 6. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-521-41008-3" title="Special:BookSources/978-0-521-41008-3"><bdi>978-0-521-41008-3</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=The+Giant+Planet+Jupiter&rft.pages=6&rft.pub=Cambridge+University+Press&rft.date=1995&rft.isbn=978-0-521-41008-3&rft.aulast=Rogers&rft.aufirst=John+Hubert&rft_id=https%3A%2F%2Fbooks.google.com%2Fbooks%3Fid%3DSO48AAAAIAAJ%26pg%3DPA6&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-86"><a href="#cite_ref-86">^</a> <a href="#Graney">Graney</a> (2010), p. 266. </li> <li id="cite_note-87"><a href="#cite_ref-87">^</a> <a href="#Smith">Smith et al. (1979)</a>, p. 954. </li> <li id="cite_note-Irwin171-88"><a href="#cite_ref-Irwin171_88-0">^</a> <a href="#Irwin2003">Irwin</a>, 2003, p. 171 </li> <li id="cite_note-89"><a href="#cite_ref-89">^</a> <a href="#Beatty">Beatty (2002)</a> </li> <li id="cite_note-90"><a href="#cite_ref-90">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFBritt2009" class="citation web cs1">Britt, Robert Roy (2009-03-09). <a rel="nofollow" class="external text" href="http://www.space.com/scienceastronomy/090309-mm-jupiter-great-red-spot.html">"Jupiter's Great Red Spot Is Shrinking"</a>. Space.com. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20090311235511/http://www.space.com/scienceastronomy/090309-mm-jupiter-great-red-spot.html">Archived</a> from the original on 11 March 2009. Retrieved 2009-02-04.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Jupiter%27s+Great+Red+Spot+Is+Shrinking&rft.pub=Space.com&rft.date=2009-03-09&rft.aulast=Britt&rft.aufirst=Robert+Roy&rft_id=http%3A%2F%2Fwww.space.com%2Fscienceastronomy%2F090309-mm-jupiter-great-red-spot.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-91"><a href="#cite_ref-91">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 191. </li> <li id="cite_note-92"><a href="#cite_ref-92">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 194–196. </li> <li id="cite_note-93"><a href="#cite_ref-93">^</a> <a href="#Beebe">Beebe (1997)</a>, p. 35. </li> <li id="cite_note-94"><a href="#cite_ref-94">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 195. </li> <li id="cite_note-95"><a href="#cite_ref-95">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFRogers2006" class="citation web cs1">Rogers, John (30 July 2006). <a rel="nofollow" class="external text" href="http://www.britastro.org/jupiter/2006report09.htm">"Interim reports on STB (Oval BA passing GRS), STropB, GRS (internal rotation measured), EZ(S. Eq. Disturbance; dramatic darkening; NEB interactions), & NNTB"</a>. British Astronomical Association. Retrieved 2007-06-15.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Interim+reports+on+STB+%28Oval+BA+passing+GRS%29%2C+STropB%2C+GRS+%28internal+rotation+measured%29%2C+EZ%28S.+Eq.+Disturbance%3B+dramatic+darkening%3B+NEB+interactions%29%2C+%26+NNTB&rft.pub=British+Astronomical+Association&rft.date=2006-07-30&rft.aulast=Rogers&rft.aufirst=John&rft_id=http%3A%2F%2Fwww.britastro.org%2Fjupiter%2F2006report09.htm&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Fletcher2010-96">^ <a href="#cite_ref-Fletcher2010_96-0">a</a> <a href="#cite_ref-Fletcher2010_96-1">b</a> <a href="#Flecther2010">Fletcher (2010)</a>, p. 306 </li> <li id="cite_note-97"><a href="#cite_ref-97">^</a> <a href="#Reese">Reese and Gordon (1966)</a> </li> <li id="cite_note-98"><a href="#cite_ref-98">^</a> <a href="#Rogers">Rogers (1995)</a>, 192–193. </li> <li id="cite_note-99"><a href="#cite_ref-99">^</a> <a href="#Stone">Stone (1974)</a> </li> <li id="cite_note-100"><a href="#cite_ref-100">^</a> <a href="#Rogers">Rogers (1995)</a>, pp. 48, 193. </li> <li id="cite_note-101"><a href="#cite_ref-101">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 193. </li> <li id="cite_note-Beebe1-102">^ <a href="#cite_ref-Beebe1_102-0">a</a> <a href="#cite_ref-Beebe1_102-1">b</a> <a href="#Beebe">Beebe (1997)</a>, pp. 38–41. </li> <li id="cite_note-103"><a href="#cite_ref-103">^</a> <a rel="nofollow" class="external text" href="https://science.nasa.gov/science-news/science-at-nasa/2014/28nov_sunburn/">Is Jupiter's Great Red Spot a Sunburn?</a> NASA.com November 28, 2014 </li> <li id="cite_note-104"><a href="#cite_ref-104">^</a> <a rel="nofollow" class="external text" href="https://www.nasa.gov/jpl/cassini/jupiters-red-spot-is-likely-a-sunburn-not-a-blush/">Jupiter's Red Spot is Likely a Sunburn, Not a Blush</a> <a rel="nofollow" class="external text" href="https://web.archive.org/web/20160706161328/http://www.nasa.gov/jpl/cassini/jupiters-red-spot-is-likely-a-sunburn-not-a-blush/">Archived</a> 2016-07-06 at the <a href="/wiki/Wayback_Machine" title="Wayback Machine">Wayback Machine</a> NASA.com, November 11, 2014 </li> <li id="cite_note-Hudson2018-105"><a href="#cite_ref-Hudson2018_105-0">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFLoefferHudson2018" class="citation journal cs1">Loeffer, Mark J.; Hudson, Reggie L. (2018). "Coloring Jupiter's clouds: Radiolysis of ammonium hydrosulfide (NH4SH)". Icarus. 302: 418–425. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2018Icar..302..418L">2018Icar..302..418L</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.icarus.2017.10.041">10.1016/j.icarus.2017.10.041</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=Coloring+Jupiter%27s+clouds%3A+Radiolysis+of+ammonium+hydrosulfide+%28NH4SH%29&rft.volume=302&rft.pages=418-425&rft.date=2018&rft_id=info%3Adoi%2F10.1016%2Fj.icarus.2017.10.041&rft_id=info%3Abibcode%2F2018Icar..302..418L&rft.aulast=Loeffer&rft.aufirst=Mark+J.&rft.au=Hudson%2C+Reggie+L.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-106"><a href="#cite_ref-106">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFPhillips2003" class="citation news cs1">Phillips, Tony (March 12, 2003). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20070615100054/https://science.nasa.gov/headlines/y2003/12mar_darkspot.htm">"The Great Dark Spot"</a>. Science at NASA. Archived from <a rel="nofollow" class="external text" href="https://science.nasa.gov/headlines/y2003/12mar_darkspot.htm">the original</a> on 15 June 2007. Retrieved 2007-06-20.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=The+Great+Dark+Spot&rft.date=2003-03-12&rft.aulast=Phillips&rft.aufirst=Tony&rft_id=https%3A%2F%2Fscience.nasa.gov%2Fheadlines%2Fy2003%2F12mar_darkspot.htm&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-107"><a href="#cite_ref-107">^</a> <a href="#Hammel">Hammel et al. (1995)</a>, p. 1740 </li> <li id="cite_note-Sanchez-Lavega_2001-108">^ <a href="#cite_ref-Sanchez-Lavega_2001_108-0">a</a> <a href="#cite_ref-Sanchez-Lavega_2001_108-1">b</a> <a href="#Sanchez2001">Sanchez-Lavega et al. (2001)</a> </li> <li id="cite_note-109"><a href="#cite_ref-109">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 223. </li> <li id="cite_note-go-110">^ <a href="#cite_ref-go_110-0">a</a> <a href="#cite_ref-go_110-1">b</a> <a href="#Go">Go et al. (2006)</a> </li> <li id="cite_note-111"><a href="#cite_ref-111">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFPhillips,_Tony2006" class="citation web cs1">Phillips, Tony (March 3, 2006). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20081019024917/https://science.nasa.gov/headlines/y2006/02mar_redjr.htm">"Jupiter's New Red Spot"</a>. NASA. Archived from <a rel="nofollow" class="external text" href="https://science.nasa.gov/headlines/y2006/02mar_redjr.htm">the original</a> on 19 October 2008. Retrieved 2008-10-16.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Jupiter%27s+New+Red+Spot&rft.pub=NASA&rft.date=2006-03-03&rft.au=Phillips%2C+Tony&rft_id=https%3A%2F%2Fscience.nasa.gov%2Fheadlines%2Fy2006%2F02mar_redjr.htm&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Tony-112">^ <a href="#cite_ref-Tony_112-0">a</a> <a href="#cite_ref-Tony_112-1">b</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFPhillips2006" class="citation web cs1">Phillips, Tony (June 5, 2006). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20070202190145/https://science.nasa.gov/headlines/y2006/05jun_redperil.htm">"Huge Storms Converge"</a>. Science@NASA. Archived from <a rel="nofollow" class="external text" href="https://science.nasa.gov/headlines/y2006/05jun_redperil.htm">the original</a> on 2 February 2007. Retrieved 2007-01-08.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Huge+Storms+Converge&rft.pub=Science%40NASA&rft.date=2006-06-05&rft.aulast=Phillips&rft.aufirst=Tony&rft_id=https%3A%2F%2Fscience.nasa.gov%2Fheadlines%2Fy2006%2F05jun_redperil.htm&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-113"><a href="#cite_ref-113">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMichaud2006" class="citation news cs1">Michaud, Peter (July 20, 2006). <a rel="nofollow" class="external text" href="http://www.gemini.edu/index.php?option=content&task=view&id=196">"Gemini Captures Close Encounter of Jupiter's Red Spots"</a>. Gemini Observatory. Retrieved 2007-06-15.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Gemini+Captures+Close+Encounter+of+Jupiter%27s+Red+Spots&rft.date=2006-07-20&rft.aulast=Michaud&rft.aufirst=Peter&rft_id=http%3A%2F%2Fwww.gemini.edu%2Findex.php%3Foption%3Dcontent%26task%3Dview%26id%3D196&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-basque-114">^ <a href="#cite_ref-basque_114-0">a</a> <a href="#cite_ref-basque_114-1">b</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite class="citation web cs1"><a rel="nofollow" class="external text" href="https://www.sciencedaily.com/releases/2008/09/080922100452.htm">"Diffusion Caused Jupiter's Red Spot Junior To Color Up"</a>. ScienceDaily. September 26, 2008. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20080930054916/https://www.sciencedaily.com/releases/2008/09/080922100452.htm">Archived</a> from the original on 30 September 2008. Retrieved 2008-10-16.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Diffusion+Caused+Jupiter%27s+Red+Spot+Junior+To+Color+Up&rft.pub=ScienceDaily&rft.date=2008-09-26&rft_id=https%3A%2F%2Fwww.sciencedaily.com%2Freleases%2F2008%2F09%2F080922100452.htm&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-NYTimes-115">^ <a href="#cite_ref-NYTimes_115-0">a</a> <a href="#cite_ref-NYTimes_115-1">b</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFFountain2008" class="citation web cs1">Fountain, Henry (July 22, 2008). <a rel="nofollow" class="external text" href="https://www.nytimes.com/2008/07/22/science/space/22obspot.html">"On Jupiter, a Battle of the Red Spots, With the Baby Losing"</a>. The New York Times. Retrieved 2010-06-18.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=The+New+York+Times&rft.atitle=On+Jupiter%2C+a+Battle+of+the+Red+Spots%2C+With+the+Baby+Losing&rft.date=2008-07-22&rft.aulast=Fountain&rft.aufirst=Henry&rft_id=https%3A%2F%2Fwww.nytimes.com%2F2008%2F07%2F22%2Fscience%2Fspace%2F22obspot.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-116"><a href="#cite_ref-116">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFBuckley,_M.2008" class="citation web cs1">Buckley, M. (May 20, 2008). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20120325063447/http://www.jhuapl.edu/newscenter/pressreleases/2008/080520.asp">"Storm Winds Blow in Jupiter's Little Red Spot"</a>. Johns Hopkins Applied Physics Laboratory. Archived from <a rel="nofollow" class="external text" href="http://www.jhuapl.edu/newscenter/pressreleases/2008/080520.asp">the original</a> on March 25, 2012. Retrieved October 16, 2008.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Storm+Winds+Blow+in+Jupiter%27s+Little+Red+Spot&rft.pub=Johns+Hopkins+Applied+Physics+Laboratory&rft.date=2008-05-20&rft.au=Buckley%2C+M.&rft_id=http%3A%2F%2Fwww.jhuapl.edu%2Fnewscenter%2Fpressreleases%2F2008%2F080520.asp&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-117"><a href="#cite_ref-117">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFSteigerwald,_Bill2006" class="citation web cs1">Steigerwald, Bill (October 10, 2006). <a rel="nofollow" class="external text" href="https://www.nasa.gov/centers/goddard/news/topstory/2006/little_red_spot.html">"Jupiter's Little Red Spot Growing Stronger"</a>. NASA Goddard Space Center. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20081101075527/http://www.nasa.gov/centers/goddard/news/topstory/2006/little_red_spot.html">Archived</a> from the original on 1 November 2008. Retrieved 2008-10-16.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Jupiter%27s+Little+Red+Spot+Growing+Stronger&rft.pub=NASA+Goddard+Space+Center&rft.date=2006-10-10&rft.au=Steigerwald%2C+Bill&rft_id=http%3A%2F%2Fwww.nasa.gov%2Fcenters%2Fgoddard%2Fnews%2Ftopstory%2F2006%2Flittle_red_spot.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Rogers2008-118">^ <a href="#cite_ref-Rogers2008_118-0">a</a> <a href="#cite_ref-Rogers2008_118-1">b</a> <a href="#cite_ref-Rogers2008_118-2">c</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFRogers,_John_H.2008" class="citation web cs1">Rogers, John H. (August 8, 2008). <a rel="nofollow" class="external text" href="http://www.britastro.org/jupiter/2008report05.htm">"The collision of the Little Red Spot and Great Red Spot: Part 2"</a>. British Astronomical Association. Retrieved 2008-11-29.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=The+collision+of+the+Little+Red+Spot+and+Great+Red+Spot%3A+Part+2&rft.pub=British+Astronomical+Association&rft.date=2008-08-08&rft.au=Rogers%2C+John+H.&rft_id=http%3A%2F%2Fwww.britastro.org%2Fjupiter%2F2008report05.htm&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-119"><a href="#cite_ref-119">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFShiga2008" class="citation web cs1">Shiga, David (May 22, 2008). <a rel="nofollow" class="external text" href="https://www.newscientist.com/article/dn13963-third-red-spot-erupts-on-jupiter.html">"Third red spot erupts on Jupiter"</a>. New Scientist. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20080705223517/http://space.newscientist.com/article/dn13963-third-red-spot-erupts-on-jupiter.html">Archived</a> from the original on 5 July 2008. Retrieved 2008-05-23.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Third+red+spot+erupts+on+Jupiter&rft.pub=New+Scientist&rft.date=2008-05-22&rft.aulast=Shiga&rft.aufirst=David&rft_id=https%3A%2F%2Fwww.newscientist.com%2Farticle%2Fdn13963-third-red-spot-erupts-on-jupiter.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-NYT-20170525-120"><a href="#cite_ref-NYT-20170525_120-0">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFChang2017" class="citation news cs1">Chang, Kenneth (May 25, 2017). <a rel="nofollow" class="external text" href="https://www.nytimes.com/2017/05/25/science/nasa-juno-spacecraft-jupiter-storms.html">"NASA's Jupiter Mission Reveals the "Brand-New and Unexpected""</a>. <a href="/wiki/The_New_York_Times" title="The New York Times">The New York Times</a>. Retrieved May 27, 2017.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+New+York+Times&rft.atitle=NASA%27s+Jupiter+Mission+Reveals+the+%22Brand-New+and+Unexpected%22&rft.date=2017-05-25&rft.aulast=Chang&rft.aufirst=Kenneth&rft_id=https%3A%2F%2Fwww.nytimes.com%2F2017%2F05%2F25%2Fscience%2Fnasa-juno-spacecraft-jupiter-storms.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-1982Vasavada-121">^ <a href="#cite_ref-1982Vasavada_121-0">a</a> <a href="#cite_ref-1982Vasavada_121-1">b</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1982, 1985–1987 </li> <li id="cite_note-Sanchez-Lavega2008-437-122">^ <a href="#cite_ref-Sanchez-Lavega2008-437_122-0">a</a> <a href="#cite_ref-Sanchez-Lavega2008-437_122-1">b</a> <a href="#cite_ref-Sanchez-Lavega2008-437_122-2">c</a> <a href="#Sanchez2008">Sanchez-Lavega et al. (2008)</a>, pp. 437–438 </li> <li id="cite_note-1983Vasavada-123">^ <a href="#cite_ref-1983Vasavada_123-0">a</a> <a href="#cite_ref-1983Vasavada_123-1">b</a> <a href="#Vasavada">Vasavada (2005)</a>, pp. 1983–1985 </li> <li id="cite_note-FOOTNOTEBaines_Simon-Miller_et_al.2007226-124"><a href="#cite_ref-FOOTNOTEBaines_Simon-Miller_et_al.2007226_124-0">^</a> <a href="#CITEREFBaines_Simon-Miller_et_al.2007">Baines Simon-Miller et al. 2007</a>, p. 226. </li> <li id="cite_note-125"><a href="#cite_ref-125">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMuraScaricaGrassiAdriani2022" class="citation journal cs1">Mura, A.; Scarica, P.; Grassi, D.; Adriani, A.; Bracco, A.; Piccioni, G.; Sindoni, G.; Moriconi, M. L.; Plainaki, C.; Ingersoll, A.; Altieri, F.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A. (2022). <a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2022JE007241">"Five Years of Observations of the Circumpolar Cyclones of Jupiter"</a>. Journal of Geophysical Research: Planets. 127 (9). <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2022JGRE..12707241M">2022JGRE..12707241M</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2022JE007241">10.1029/2022JE007241</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/2169-9097">2169-9097</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:252099924">252099924</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+Geophysical+Research%3A+Planets&rft.atitle=Five+Years+of+Observations+of+the+Circumpolar+Cyclones+of+Jupiter&rft.volume=127&rft.issue=9&rft.date=2022&rft_id=info%3Adoi%2F10.1029%2F2022JE007241&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A252099924%23id-name%3DS2CID&rft.issn=2169-9097&rft_id=info%3Abibcode%2F2022JGRE..12707241M&rft.aulast=Mura&rft.aufirst=A.&rft.au=Scarica%2C+P.&rft.au=Grassi%2C+D.&rft.au=Adriani%2C+A.&rft.au=Bracco%2C+A.&rft.au=Piccioni%2C+G.&rft.au=Sindoni%2C+G.&rft.au=Moriconi%2C+M.+L.&rft.au=Plainaki%2C+C.&rft.au=Ingersoll%2C+A.&rft.au=Altieri%2C+F.&rft.au=Cicchetti%2C+A.&rft.au=Dinelli%2C+B.+M.&rft.au=Filacchione%2C+G.&rft.au=Migliorini%2C+A.&rft_id=https%3A%2F%2Fdoi.org%2F10.1029%252F2022JE007241&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-126"><a href="#cite_ref-126">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFTabataba-VakiliRogersEichstädtOrton2020" class="citation journal cs1">Tabataba-Vakili, F.; Rogers, J.H.; Eichstädt, G.; Orton, G.S.; Hansen, C.J.; Momary, T.W.; Sinclair, J.A.; Giles, R.S.; Caplinger, M.A.; Ravine, M.A.; Bolton, S.J. (January 2020). "Long-term tracking of circumpolar cyclones on Jupiter from polar observations with JunoCam". Icarus. 335: 113405. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2020Icar..33513405T">2020Icar..33513405T</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.icarus.2019.113405">10.1016/j.icarus.2019.113405</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0019-1035">0019-1035</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:202132980">202132980</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=Long-term+tracking+of+circumpolar+cyclones+on+Jupiter+from+polar+observations+with+JunoCam&rft.volume=335&rft.pages=113405&rft.date=2020-01&rft_id=info%3Adoi%2F10.1016%2Fj.icarus.2019.113405&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A202132980%23id-name%3DS2CID&rft.issn=0019-1035&rft_id=info%3Abibcode%2F2020Icar..33513405T&rft.aulast=Tabataba-Vakili&rft.aufirst=F.&rft.au=Rogers%2C+J.H.&rft.au=Eichst%C3%A4dt%2C+G.&rft.au=Orton%2C+G.S.&rft.au=Hansen%2C+C.J.&rft.au=Momary%2C+T.W.&rft.au=Sinclair%2C+J.A.&rft.au=Giles%2C+R.S.&rft.au=Caplinger%2C+M.A.&rft.au=Ravine%2C+M.A.&rft.au=Bolton%2C+S.J.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-127"><a href="#cite_ref-127">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGrassiAdrianiMoriconiMura2018" class="citation journal cs1">Grassi, D.; Adriani, A.; Moriconi, M. L.; Mura, A.; Tabataba-Vakili, F.; Ingersoll, A.; Orton, G.; Hansen, C.; Altieri, F.; Filacchione, G.; Sindoni, G. (June 2018). <a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2018JE005555">"First Estimate of Wind Fields in the Jupiter Polar Regions From JIRAM-Juno Images"</a>. Journal of Geophysical Research: Planets. 123 (6): 1511–1524. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2018JGRE..123.1511G">2018JGRE..123.1511G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2018JE005555">10.1029/2018JE005555</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/2027.42%2F145242">2027.42/145242</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/2169-9097">2169-9097</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:133852380">133852380</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+Geophysical+Research%3A+Planets&rft.atitle=First+Estimate+of+Wind+Fields+in+the+Jupiter+Polar+Regions+From+JIRAM-Juno+Images&rft.volume=123&rft.issue=6&rft.pages=1511-1524&rft.date=2018-06&rft_id=info%3Ahdl%2F2027.42%2F145242&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A133852380%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2018JGRE..123.1511G&rft.issn=2169-9097&rft_id=info%3Adoi%2F10.1029%2F2018JE005555&rft.aulast=Grassi&rft.aufirst=D.&rft.au=Adriani%2C+A.&rft.au=Moriconi%2C+M.+L.&rft.au=Mura%2C+A.&rft.au=Tabataba-Vakili%2C+F.&rft.au=Ingersoll%2C+A.&rft.au=Orton%2C+G.&rft.au=Hansen%2C+C.&rft.au=Altieri%2C+F.&rft.au=Filacchione%2C+G.&rft.au=Sindoni%2C+G.&rft_id=https%3A%2F%2Fdoi.org%2F10.1029%252F2018JE005555&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-128"><a href="#cite_ref-128">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGavrielKaspi2021" class="citation journal cs1">Gavriel, Nimrod; Kaspi, Yohai (August 2021). <a rel="nofollow" class="external text" href="https://www.nature.com/articles/s41561-021-00781-6">"The number and location of Jupiter's circumpolar cyclones explained by vorticity dynamics"</a>. Nature Geoscience. 14 (8): 559–563. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2110.09422">2110.09422</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021NatGe..14..559G">2021NatGe..14..559G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fs41561-021-00781-6">10.1038/s41561-021-00781-6</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1752-0894">1752-0894</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:236096014">236096014</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature+Geoscience&rft.atitle=The+number+and+location+of+Jupiter%27s+circumpolar+cyclones+explained+by+vorticity+dynamics&rft.volume=14&rft.issue=8&rft.pages=559-563&rft.date=2021-08&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A236096014%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2021NatGe..14..559G&rft_id=info%3Aarxiv%2F2110.09422&rft.issn=1752-0894&rft_id=info%3Adoi%2F10.1038%2Fs41561-021-00781-6&rft.aulast=Gavriel&rft.aufirst=Nimrod&rft.au=Kaspi%2C+Yohai&rft_id=https%3A%2F%2Fwww.nature.com%2Farticles%2Fs41561-021-00781-6&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-129"><a href="#cite_ref-129">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFAdrianiMuraOrtonHansen2018" class="citation journal cs1">Adriani, A.; Mura, A.; Orton, G.; Hansen, C.; Altieri, F.; Moriconi, M. L.; Rogers, J.; Eichstädt, G.; Momary, T.; Ingersoll, A. P.; Filacchione, G. (March 2018). <a rel="nofollow" class="external text" href="http://www.nature.com/articles/nature25491">"Clusters of cyclones encircling Jupiter's poles"</a>. Nature. 555 (7695): 216–219. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2018Natur.555..216A">2018Natur.555..216A</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fnature25491">10.1038/nature25491</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0028-0836">0028-0836</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/29516997">29516997</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:4438233">4438233</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Clusters+of+cyclones+encircling+Jupiter%27s+poles&rft.volume=555&rft.issue=7695&rft.pages=216-219&rft.date=2018-03&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A4438233%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2018Natur.555..216A&rft.issn=0028-0836&rft_id=info%3Adoi%2F10.1038%2Fnature25491&rft_id=info%3Apmid%2F29516997&rft.aulast=Adriani&rft.aufirst=A.&rft.au=Mura%2C+A.&rft.au=Orton%2C+G.&rft.au=Hansen%2C+C.&rft.au=Altieri%2C+F.&rft.au=Moriconi%2C+M.+L.&rft.au=Rogers%2C+J.&rft.au=Eichst%C3%A4dt%2C+G.&rft.au=Momary%2C+T.&rft.au=Ingersoll%2C+A.+P.&rft.au=Filacchione%2C+G.&rft_id=http%3A%2F%2Fwww.nature.com%2Farticles%2Fnature25491&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-130"><a href="#cite_ref-130">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFADEM1956" class="citation journal cs1">ADEM, JULIÁN (August 1956). <a rel="nofollow" class="external text" href="https://dx.doi.org/10.1111/j.2153-3490.1956.tb01234.x">"A Series Solution for the Barotropic Vorticity Equation and its Application in the Study of Atmospheric Vortices"</a>. Tellus. 8 (3): 364–372. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1956Tell....8..364A">1956Tell....8..364A</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1111%2Fj.2153-3490.1956.tb01234.x">10.1111/j.2153-3490.1956.tb01234.x</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0040-2826">0040-2826</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Tellus&rft.atitle=A+Series+Solution+for+the+Barotropic+Vorticity+Equation+and+its+Application+in+the+Study+of+Atmospheric+Vortices&rft.volume=8&rft.issue=3&rft.pages=364-372&rft.date=1956-08&rft.issn=0040-2826&rft_id=info%3Adoi%2F10.1111%2Fj.2153-3490.1956.tb01234.x&rft_id=info%3Abibcode%2F1956Tell....8..364A&rft.aulast=ADEM&rft.aufirst=JULI%C3%81N&rft_id=http%3A%2F%2Fdx.doi.org%2F10.1111%2Fj.2153-3490.1956.tb01234.x&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-131"><a href="#cite_ref-131">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFScott2010" class="citation journal cs1">Scott, R.K. (2010-09-15). <a rel="nofollow" class="external text" href="https://dx.doi.org/10.1080/03091929.2010.509927">"Polar accumulation of cyclonic vorticity"</a>. Geophysical & Astrophysical Fluid Dynamics. 105 (4–5): 409–420. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1080%2F03091929.2010.509927">10.1080/03091929.2010.509927</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0309-1929">0309-1929</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:2050846">2050846</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Geophysical+%26+Astrophysical+Fluid+Dynamics&rft.atitle=Polar+accumulation+of+cyclonic+vorticity&rft.volume=105&rft.issue=4%E2%80%935&rft.pages=409-420&rft.date=2010-09-15&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A2050846%23id-name%3DS2CID&rft.issn=0309-1929&rft_id=info%3Adoi%2F10.1080%2F03091929.2010.509927&rft.aulast=Scott&rft.aufirst=R.K.&rft_id=http%3A%2F%2Fdx.doi.org%2F10.1080%2F03091929.2010.509927&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-132"><a href="#cite_ref-132">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFO'NeillEmanuelFlierl2015" class="citation journal cs1">O'Neill, Morgan E; Emanuel, Kerry A.; Flierl, Glenn R. (2015-06-15). <a rel="nofollow" class="external text" href="https://dx.doi.org/10.1038/ngeo2459">"Polar vortex formation in giant-planet atmospheres due to moist convection"</a>. Nature Geoscience. 8 (7): 523–526. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2015NatGe...8..523O">2015NatGe...8..523O</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fngeo2459">10.1038/ngeo2459</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/1721.1%2F100773">1721.1/100773</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1752-0894">1752-0894</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature+Geoscience&rft.atitle=Polar+vortex+formation+in+giant-planet+atmospheres+due+to+moist+convection&rft.volume=8&rft.issue=7&rft.pages=523-526&rft.date=2015-06-15&rft_id=info%3Ahdl%2F1721.1%2F100773&rft.issn=1752-0894&rft_id=info%3Adoi%2F10.1038%2Fngeo2459&rft_id=info%3Abibcode%2F2015NatGe...8..523O&rft.aulast=O%27Neill&rft.aufirst=Morgan+E&rft.au=Emanuel%2C+Kerry+A.&rft.au=Flierl%2C+Glenn+R.&rft_id=http%3A%2F%2Fdx.doi.org%2F10.1038%2Fngeo2459&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-:1-133">^ <a href="#cite_ref-:1_133-0">a</a> <a href="#cite_ref-:1_133-1">b</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGavrielKaspi2021" class="citation journal cs1">Gavriel, Nimrod; Kaspi, Yohai (August 2021). <a rel="nofollow" class="external text" href="https://www.nature.com/articles/s41561-021-00781-6">"The number and location of Jupiter's circumpolar cyclones explained by vorticity dynamics"</a>. Nature Geoscience. 14 (8): 559–563. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2110.09422">2110.09422</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021NatGe..14..559G">2021NatGe..14..559G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fs41561-021-00781-6">10.1038/s41561-021-00781-6</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/1752-0908">1752-0908</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:236096014">236096014</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature+Geoscience&rft.atitle=The+number+and+location+of+Jupiter%27s+circumpolar+cyclones+explained+by+vorticity+dynamics&rft.volume=14&rft.issue=8&rft.pages=559-563&rft.date=2021-08&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A236096014%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2021NatGe..14..559G&rft_id=info%3Aarxiv%2F2110.09422&rft.issn=1752-0908&rft_id=info%3Adoi%2F10.1038%2Fs41561-021-00781-6&rft.aulast=Gavriel&rft.aufirst=Nimrod&rft.au=Kaspi%2C+Yohai&rft_id=https%3A%2F%2Fwww.nature.com%2Farticles%2Fs41561-021-00781-6&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-134"><a href="#cite_ref-134">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFLiIngersollKlipfelBrettle2020" class="citation journal cs1">Li, Cheng; Ingersoll, Andrew P.; Klipfel, Alexandra P.; Brettle, Harriet (2020-09-08). <a rel="nofollow" class="external text" href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7533696">"Modeling the stability of polygonal patterns of vortices at the poles of Jupiter as revealed by the Juno spacecraft"</a>. Proceedings of the National Academy of Sciences. 117 (39): 24082–24087. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2020PNAS..11724082L">2020PNAS..11724082L</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1073%2Fpnas.2008440117">10.1073/pnas.2008440117</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0027-8424">0027-8424</a>. <a href="/wiki/PMC_(identifier)" class="mw-redirect" title="PMC (identifier)">PMC</a> <a rel="nofollow" class="external text" href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7533696">7533696</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/32900956">32900956</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Proceedings+of+the+National+Academy+of+Sciences&rft.atitle=Modeling+the+stability+of+polygonal+patterns+of+vortices+at+the+poles+of+Jupiter+as+revealed+by+the+Juno+spacecraft&rft.volume=117&rft.issue=39&rft.pages=24082-24087&rft.date=2020-09-08&rft_id=https%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpmc%2Farticles%2FPMC7533696%23id-name%3DPMC&rft_id=info%3Abibcode%2F2020PNAS..11724082L&rft_id=info%3Apmid%2F32900956&rft_id=info%3Adoi%2F10.1073%2Fpnas.2008440117&rft.issn=0027-8424&rft.aulast=Li&rft.aufirst=Cheng&rft.au=Ingersoll%2C+Andrew+P.&rft.au=Klipfel%2C+Alexandra+P.&rft.au=Brettle%2C+Harriet&rft_id=https%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpmc%2Farticles%2FPMC7533696&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-135"><a href="#cite_ref-135">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMuraScaricaGrassiAdriani2022" class="citation journal cs1">Mura, A.; Scarica, P.; Grassi, D.; Adriani, A.; Bracco, A.; Piccioni, G.; Sindoni, G.; Moriconi, M. L.; Plainaki, C.; Ingersoll, A.; Altieri, F.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A. (2022). <a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2022JE007241">"Five Years of Observations of the Circumpolar Cyclones of Jupiter"</a>. Journal of Geophysical Research: Planets. 127 (9). <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2022JGRE..12707241M">2022JGRE..12707241M</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2022JE007241">10.1029/2022JE007241</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/2169-9097">2169-9097</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:252099924">252099924</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+Geophysical+Research%3A+Planets&rft.atitle=Five+Years+of+Observations+of+the+Circumpolar+Cyclones+of+Jupiter&rft.volume=127&rft.issue=9&rft.date=2022&rft_id=info%3Adoi%2F10.1029%2F2022JE007241&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A252099924%23id-name%3DS2CID&rft.issn=2169-9097&rft_id=info%3Abibcode%2F2022JGRE..12707241M&rft.aulast=Mura&rft.aufirst=A.&rft.au=Scarica%2C+P.&rft.au=Grassi%2C+D.&rft.au=Adriani%2C+A.&rft.au=Bracco%2C+A.&rft.au=Piccioni%2C+G.&rft.au=Sindoni%2C+G.&rft.au=Moriconi%2C+M.+L.&rft.au=Plainaki%2C+C.&rft.au=Ingersoll%2C+A.&rft.au=Altieri%2C+F.&rft.au=Cicchetti%2C+A.&rft.au=Dinelli%2C+B.+M.&rft.au=Filacchione%2C+G.&rft.au=Migliorini%2C+A.&rft_id=https%3A%2F%2Fdoi.org%2F10.1029%252F2022JE007241&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-136"><a href="#cite_ref-136">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFRogersEichstädtHansenOrton2021" class="citation journal cs1">Rogers, John; Eichstädt, Gerald; Hansen, Candice; Orton, Glenn; Momary, Thomas (2021). <a rel="nofollow" class="external text" href="https://meetingorganizer.copernicus.org/EPSC2021/EPSC2021-57.html">"Behaviour of Jupiter's polar polygons over 4 years"</a>. European Planetary Science Congress Abstracts. 15. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021EPSC...15...57R">2021EPSC...15...57R</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.5194%2Fepsc2021-57">10.5194/epsc2021-57</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:241446672">241446672</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=European+Planetary+Science+Congress+Abstracts&rft.atitle=Behaviour+of+Jupiter%27s+polar+polygons+over+4+years&rft.volume=15&rft.date=2021&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A241446672%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.5194%2Fepsc2021-57&rft_id=info%3Abibcode%2F2021EPSC...15...57R&rft.aulast=Rogers&rft.aufirst=John&rft.au=Eichst%C3%A4dt%2C+Gerald&rft.au=Hansen%2C+Candice&rft.au=Orton%2C+Glenn&rft.au=Momary%2C+Thomas&rft_id=https%3A%2F%2Fmeetingorganizer.copernicus.org%2FEPSC2021%2FEPSC2021-57.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-137"><a href="#cite_ref-137">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGavrielKaspi2022" class="citation journal cs1">Gavriel, Nimrod; Kaspi, Yohai (2022-08-16). <a rel="nofollow" class="external text" href="https://onlinelibrary.wiley.com/doi/10.1029/2022GL098708">"The Oscillatory Motion of Jupiter's Polar Cyclones Results From Vorticity Dynamics"</a>. Geophysical Research Letters. 49 (15). <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2209.00309">2209.00309</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2022GeoRL..4998708G">2022GeoRL..4998708G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2022GL098708">10.1029/2022GL098708</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0094-8276">0094-8276</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:249810436">249810436</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Geophysical+Research+Letters&rft.atitle=The+Oscillatory+Motion+of+Jupiter%27s+Polar+Cyclones+Results+From+Vorticity+Dynamics&rft.volume=49&rft.issue=15&rft.date=2022-08-16&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A249810436%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2022GeoRL..4998708G&rft_id=info%3Aarxiv%2F2209.00309&rft.issn=0094-8276&rft_id=info%3Adoi%2F10.1029%2F2022GL098708&rft.aulast=Gavriel&rft.aufirst=Nimrod&rft.au=Kaspi%2C+Yohai&rft_id=https%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1029%2F2022GL098708&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-138"><a href="#cite_ref-138">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFGavrielKaspi2022" class="citation journal cs1">Gavriel, Nimrod; Kaspi, Yohai (2022-08-16). <a rel="nofollow" class="external text" href="https://onlinelibrary.wiley.com/doi/10.1029/2022GL098708">"The Oscillatory Motion of Jupiter's Polar Cyclones Results From Vorticity Dynamics"</a>. Geophysical Research Letters. 49 (15). <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/2209.00309">2209.00309</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2022GeoRL..4998708G">2022GeoRL..4998708G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2022GL098708">10.1029/2022GL098708</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0094-8276">0094-8276</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:249810436">249810436</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Geophysical+Research+Letters&rft.atitle=The+Oscillatory+Motion+of+Jupiter%27s+Polar+Cyclones+Results+From+Vorticity+Dynamics&rft.volume=49&rft.issue=15&rft.date=2022-08-16&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A249810436%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2022GeoRL..4998708G&rft_id=info%3Aarxiv%2F2209.00309&rft.issn=0094-8276&rft_id=info%3Adoi%2F10.1029%2F2022GL098708&rft.aulast=Gavriel&rft.aufirst=Nimrod&rft.au=Kaspi%2C+Yohai&rft_id=https%3A%2F%2Fonlinelibrary.wiley.com%2Fdoi%2F10.1029%2F2022GL098708&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-139"><a href="#cite_ref-139">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMuraAdrianiBraccoMoriconi2021" class="citation journal cs1">Mura, A.; Adriani, A.; Bracco, A.; Moriconi, M. L.; Grassi, D.; Plainaki, C.; Ingersoll, A.; Bolton, S.; Sordini, R.; Altieri, F.; Ciarravano, A.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A. (2021-07-28). <a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2021GL094235">"Oscillations and Stability of the Jupiter Polar Cyclones"</a>. Geophysical Research Letters. 48 (14). <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021GeoRL..4894235M">2021GeoRL..4894235M</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F2021GL094235">10.1029/2021GL094235</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0094-8276">0094-8276</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:237698857">237698857</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Geophysical+Research+Letters&rft.atitle=Oscillations+and+Stability+of+the+Jupiter+Polar+Cyclones&rft.volume=48&rft.issue=14&rft.date=2021-07-28&rft_id=info%3Adoi%2F10.1029%2F2021GL094235&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A237698857%23id-name%3DS2CID&rft.issn=0094-8276&rft_id=info%3Abibcode%2F2021GeoRL..4894235M&rft.aulast=Mura&rft.aufirst=A.&rft.au=Adriani%2C+A.&rft.au=Bracco%2C+A.&rft.au=Moriconi%2C+M.+L.&rft.au=Grassi%2C+D.&rft.au=Plainaki%2C+C.&rft.au=Ingersoll%2C+A.&rft.au=Bolton%2C+S.&rft.au=Sordini%2C+R.&rft.au=Altieri%2C+F.&rft.au=Ciarravano%2C+A.&rft.au=Cicchetti%2C+A.&rft.au=Dinelli%2C+B.+M.&rft.au=Filacchione%2C+G.&rft.au=Migliorini%2C+A.&rft_id=https%3A%2F%2Fdoi.org%2F10.1029%252F2021GL094235&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-140"><a href="#cite_ref-140">^</a> <a href="#McKim">McKim (1997)</a> </li> <li id="cite_note-141"><a href="#cite_ref-141">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMiller1953" class="citation journal cs1">Miller, Stanley L. (1953-05-15). <a rel="nofollow" class="external text" href="https://www.science.org/doi/10.1126/science.117.3046.528">"A Production of Amino Acids Under Possible Primitive Earth Conditions"</a>. Science. 117 (3046): 528–529. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1953Sci...117..528M">1953Sci...117..528M</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.117.3046.528">10.1126/science.117.3046.528</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0036-8075">0036-8075</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/13056598">13056598</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=A+Production+of+Amino+Acids+Under+Possible+Primitive+Earth+Conditions&rft.volume=117&rft.issue=3046&rft.pages=528-529&rft.date=1953-05-15&rft_id=info%3Adoi%2F10.1126%2Fscience.117.3046.528&rft.issn=0036-8075&rft_id=info%3Apmid%2F13056598&rft_id=info%3Abibcode%2F1953Sci...117..528M&rft.aulast=Miller&rft.aufirst=Stanley+L.&rft_id=https%3A%2F%2Fwww.science.org%2Fdoi%2F10.1126%2Fscience.117.3046.528&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-Ingersoll10-142"><a href="#cite_ref-Ingersoll10_142-0">^</a> <a href="#Ingersoll">Ingersoll (2004)</a>, p. 2 </li> <li id="cite_note-Noll1995-143"><a href="#cite_ref-Noll1995_143-0">^</a> <a href="#Noll1995">Noll (1995)</a>, p. 1307 </li> <li id="cite_note-144"><a href="#cite_ref-144">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 6. </li> <li id="cite_note-Rogers2008b-145"><a href="#cite_ref-Rogers2008b_145-0">^</a> <a href="#Rogers2008b">Rogers (2008)</a>, pp.111–112 </li> <li id="cite_note-Rogers188-146">^ <a href="#cite_ref-Rogers188_146-0">a</a> <a href="#cite_ref-Rogers188_146-1">b</a> <a href="#Rogers">Rogers (1995)</a>, p. 188 </li> <li id="cite_note-Hockey1-147">^ <a href="#cite_ref-Hockey1_147-0">a</a> <a href="#cite_ref-Hockey1_147-1">b</a> <a href="#Hockey1999">Hockey, 1999</a>, pp. 40–41. </li> <li id="cite_note-148"><a href="#cite_ref-148">^</a> <a href="#Smith">Smith et al. (1979)</a>, pp. 951–972. </li> <li id="cite_note-Rogers3-149">^ <a href="#cite_ref-Rogers3_149-0">a</a> <a href="#cite_ref-Rogers3_149-1">b</a> <a href="#Rogers">Rogers (1995)</a>, pp. 224–5. </li> <li id="cite_note-150"><a href="#cite_ref-150">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 226–227. </li> <li id="cite_note-151"><a href="#cite_ref-151">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 226. </li> <li id="cite_note-152"><a href="#cite_ref-152">^</a> <a href="#Rogers">Rogers (1995)</a>, p. 225. </li> <li id="cite_note-153"><a href="#cite_ref-153">^</a> <a href="#Beebe">Beebe (1997)</a>, p. 43. </li> <li id="cite_note-154"><a href="#cite_ref-154">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite class="citation web cs1"><a rel="nofollow" class="external text" href="https://web.archive.org/web/20230329014357/http://www.nasa.gov/image-feature/a-new-view-of-jupiters-storms/">"A New View of Jupiter's Storms"</a>. NASA. 17 September 2020. Archived from <a rel="nofollow" class="external text" href="https://www.nasa.gov/image-feature/a-new-view-of-jupiters-storms">the original</a> on 29 March 2023. Retrieved 25 September 2020.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=NASA&rft.atitle=A+New+View+of+Jupiter%27s+Storms&rft.date=2020-09-17&rft_id=https%3A%2F%2Fwww.nasa.gov%2Fimage-feature%2Fa-new-view-of-jupiters-storms&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> <li id="cite_note-155"><a href="#cite_ref-155">^</a> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFCheng_LiAndrew_P._IngersollAlexandra_P._KlipfelHarriet_Brettle2020" class="citation journal cs1">Cheng Li; Andrew P. Ingersoll; Alexandra P. Klipfel; Harriet Brettle (2020). <a rel="nofollow" class="external text" href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7533696">"Modeling the stability of polygonal patterns of vortices at the poles of Jupiter as revealed by the Juno spacecraft"</a>. PNAS. 117 (39): 24082–24087. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2020PNAS..11724082L">2020PNAS..11724082L</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1073%2Fpnas.2008440117">10.1073/pnas.2008440117</a>. <a href="/wiki/PMC_(identifier)" class="mw-redirect" title="PMC (identifier)">PMC</a> <a rel="nofollow" class="external text" href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7533696">7533696</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/32900956">32900956</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=PNAS&rft.atitle=Modeling+the+stability+of+polygonal+patterns+of+vortices+at+the+poles+of+Jupiter+as+revealed+by+the+Juno+spacecraft&rft.volume=117&rft.issue=39&rft.pages=24082-24087&rft.date=2020&rft_id=https%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpmc%2Farticles%2FPMC7533696%23id-name%3DPMC&rft_id=info%3Apmid%2F32900956&rft_id=info%3Adoi%2F10.1073%2Fpnas.2008440117&rft_id=info%3Abibcode%2F2020PNAS..11724082L&rft.au=Cheng+Li&rft.au=Andrew+P.+Ingersoll&rft.au=Alexandra+P.+Klipfel&rft.au=Harriet+Brettle&rft_id=https%3A%2F%2Fwww.ncbi.nlm.nih.gov%2Fpmc%2Farticles%2FPMC7533696&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"> </li> </ol></div> <div class="mw-heading mw-heading2"><h2 id="Cited_sources">Cited sources</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=25" title="Edit section: Cited sources">edit</a>]</div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1239549316"><div class="refbegin refbegin-columns references-column-width" style="column-width: 30em"> <ul><li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFAtreya_Wong_Owen_et_al.1999" class="citation journal cs1">Atreya, Sushil K.; Wong, M. H.; Owen, T. C.; Mahaffy, P. R.; Niemann, H. B.; de Pater, I.; Drossart, P.; <a href="/wiki/Th%C3%A9r%C3%A8se_Encrenaz" title="Thérèse Encrenaz">Encrenaz, T.</a> (October–November 1999). "A comparison of the atmospheres of Jupiter and Saturn: Deep atmospheric composition, cloud structure, vertical mixing, and origin". <a href="/wiki/Planetary_and_Space_Science" title="Planetary and Space Science">Planetary and Space Science</a>. 47 (10–11): 1243–1262. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1999P&SS...47.1243A">1999P&SS...47.1243A</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2FS0032-0633%2899%2900047-1">10.1016/S0032-0633(99)00047-1</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0032-0633">0032-0633</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/11543193">11543193</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Planetary+and+Space+Science&rft.atitle=A+comparison+of+the+atmospheres+of+Jupiter+and+Saturn%3A+Deep+atmospheric+composition%2C+cloud+structure%2C+vertical+mixing%2C+and+origin&rft.volume=47&rft.issue=10%E2%80%9311&rft.pages=1243-1262&rft.date=1999-10%2F1999-11&rft_id=info%3Adoi%2F10.1016%2FS0032-0633%2899%2900047-1&rft.issn=0032-0633&rft_id=info%3Apmid%2F11543193&rft_id=info%3Abibcode%2F1999P%26SS...47.1243A&rft.aulast=Atreya&rft.aufirst=Sushil+K.&rft.au=Wong%2C+M.+H.&rft.au=Owen%2C+T.+C.&rft.au=Mahaffy%2C+P.+R.&rft.au=Niemann%2C+H.+B.&rft.au=de+Pater%2C+I.&rft.au=Drossart%2C+P.&rft.au=Encrenaz%2C+T.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFAtreya_Mahaffy_Niemann_et_al.2003" class="citation journal cs1">Atreya, Sushil K.; Mahaffy, P. R.; Niemann, H. B.; Wong, M. H.; Owen, T. C. (February 2003). "Composition and origin of the atmosphere of Jupiter—an update, and implications for the extrasolar giant planets". <a href="/wiki/Planetary_and_Space_Science" title="Planetary and Space Science">Planetary and Space Science</a>. 51 (2): 105–112. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003P&SS...51..105A">2003P&SS...51..105A</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2FS0032-0633%2802%2900144-7">10.1016/S0032-0633(02)00144-7</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0032-0633">0032-0633</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Planetary+and+Space+Science&rft.atitle=Composition+and+origin+of+the+atmosphere+of+Jupiter%E2%80%94an+update%2C+and+implications+for+the+extrasolar+giant+planets&rft.volume=51&rft.issue=2&rft.pages=105-112&rft.date=2003-02&rft.issn=0032-0633&rft_id=info%3Adoi%2F10.1016%2FS0032-0633%2802%2900144-7&rft_id=info%3Abibcode%2F2003P%26SS...51..105A&rft.aulast=Atreya&rft.aufirst=Sushil+K.&rft.au=Mahaffy%2C+P.+R.&rft.au=Niemann%2C+H.+B.&rft.au=Wong%2C+M.+H.&rft.au=Owen%2C+T.+C.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFAtreyaWong2005" class="citation journal cs1">Atreya, Sushil K.; Wong, Ah-San (2005). <a rel="nofollow" class="external text" href="http://www-personal.umich.edu/~atreya/Chapters/2005_JovianCloud_Multiprobes.pdf">"Coupled Clouds and Chemistry of the Giant Planets — A Case for Multiprobes"</a> (PDF). Space Science Reviews. 116 (1–2): 121–136. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005SSRv..116..121A">2005SSRv..116..121A</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1007%2Fs11214-005-1951-5">10.1007/s11214-005-1951-5</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/2027.42%2F43766">2027.42/43766</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0032-0633">0032-0633</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:31037195">31037195</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Space+Science+Reviews&rft.atitle=Coupled+Clouds+and+Chemistry+of+the+Giant+Planets+%E2%80%94+A+Case+for+Multiprobes&rft.volume=116&rft.issue=1%E2%80%932&rft.pages=121-136&rft.date=2005&rft_id=info%3Ahdl%2F2027.42%2F43766&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A31037195%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2005SSRv..116..121A&rft.issn=0032-0633&rft_id=info%3Adoi%2F10.1007%2Fs11214-005-1951-5&rft.aulast=Atreya&rft.aufirst=Sushil+K.&rft.au=Wong%2C+Ah-San&rft_id=http%3A%2F%2Fwww-personal.umich.edu%2F~atreya%2FChapters%2F2005_JovianCloud_Multiprobes.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFAtreya_Wong_Baines_et_al.2005" class="citation journal cs1">Atreya, Sushil K.; Wong, Ah-San; Baines, K. H.; Wong, M. H.; Owen, T. C. (2005). <a rel="nofollow" class="external text" href="http://www-personal.umich.edu/~atreya/Articles/2005_Jupiters_Ammonia.pdf">"Jupiter's ammonia clouds—localized or ubiquitous?"</a> (PDF). <a href="/wiki/Planetary_and_Space_Science" title="Planetary and Space Science">Planetary and Space Science</a>. 53 (5): 498–507. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005P&SS...53..498A">2005P&SS...53..498A</a>. <a href="/wiki/CiteSeerX_(identifier)" class="mw-redirect" title="CiteSeerX (identifier)">CiteSeerX</a> <a rel="nofollow" class="external text" href="https://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.553.8220">10.1.1.553.8220</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.pss.2004.04.002">10.1016/j.pss.2004.04.002</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0032-0633">0032-0633</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Planetary+and+Space+Science&rft.atitle=Jupiter%27s+ammonia+clouds%E2%80%94localized+or+ubiquitous%3F&rft.volume=53&rft.issue=5&rft.pages=498-507&rft.date=2005&rft_id=https%3A%2F%2Fciteseerx.ist.psu.edu%2Fviewdoc%2Fsummary%3Fdoi%3D10.1.1.553.8220%23id-name%3DCiteSeerX&rft.issn=0032-0633&rft_id=info%3Adoi%2F10.1016%2Fj.pss.2004.04.002&rft_id=info%3Abibcode%2F2005P%26SS...53..498A&rft.aulast=Atreya&rft.aufirst=Sushil+K.&rft.au=Wong%2C+Ah-San&rft.au=Baines%2C+K.+H.&rft.au=Wong%2C+M.+H.&rft.au=Owen%2C+T.+C.&rft_id=http%3A%2F%2Fwww-personal.umich.edu%2F~atreya%2FArticles%2F2005_Jupiters_Ammonia.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFBaines_Simon-Miller_et_al.2007" class="citation journal cs1">Baines, Kevin H.; Simon-Miller, Amy A; Orton, Glenn S.; Weaver, Harold A.; Lunsford, Allen; Momary, Thomas W.; Spencer, John; Cheng, Andrew F.; Reuter, Dennis C. (12 October 2007). "Polar Lightning and Decadal-Scale Cloud Variability on Jupiter". <a href="/wiki/Science_(journal)" title="Science (journal)">Science</a>. 318 (5848): 226–229. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2007Sci...318..226B">2007Sci...318..226B</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.1147912">10.1126/science.1147912</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/17932285">17932285</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:28540751">28540751</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=Polar+Lightning+and+Decadal-Scale+Cloud+Variability+on+Jupiter&rft.volume=318&rft.issue=5848&rft.pages=226-229&rft.date=2007-10-12&rft_id=info%3Adoi%2F10.1126%2Fscience.1147912&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A28540751%23id-name%3DS2CID&rft_id=info%3Apmid%2F17932285&rft_id=info%3Abibcode%2F2007Sci...318..226B&rft.aulast=Baines&rft.aufirst=Kevin+H.&rft.au=Simon-Miller%2C+Amy+A&rft.au=Orton%2C+Glenn+S.&rft.au=Weaver%2C+Harold+A.&rft.au=Lunsford%2C+Allen&rft.au=Momary%2C+Thomas+W.&rft.au=Spencer%2C+John&rft.au=Cheng%2C+Andrew+F.&rft.au=Reuter%2C+Dennis+C.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Beatty" class="citation journal cs1">Beatty, J.K. (2002). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20110527081602/http://www.saburchill.com/HOS/astronomy/034.html">"Jupiter's Shrinking Red Spot"</a>. <a href="/wiki/Sky_and_Telescope" class="mw-redirect" title="Sky and Telescope">Sky and Telescope</a>. 103 (4): 24. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2002S&T...103d..24B">2002S&T...103d..24B</a>. Archived from <a rel="nofollow" class="external text" href="http://www.saburchill.com/HOS/astronomy/034.html">the original</a> on 2011-05-27. Retrieved 2008-08-10.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Sky+and+Telescope&rft.atitle=Jupiter%27s+Shrinking+Red+Spot&rft.volume=103&rft.issue=4&rft.pages=24&rft.date=2002&rft_id=info%3Abibcode%2F2002S%26T...103d..24B&rft.aulast=Beatty&rft.aufirst=J.K.&rft_id=http%3A%2F%2Fwww.saburchill.com%2FHOS%2Fastronomy%2F034.html&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Beebe" class="citation book cs1">Beebe, R. (1997). Jupiter the Giant Planet (2nd ed.). Washington: <a href="/wiki/Smithsonian_Books" class="mw-redirect" title="Smithsonian Books">Smithsonian Books</a>. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-1-56098-685-0" title="Special:BookSources/978-1-56098-685-0"><bdi>978-1-56098-685-0</bdi></a>. <a href="/wiki/OCLC_(identifier)" class="mw-redirect" title="OCLC (identifier)">OCLC</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/oclc/224014042">224014042</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Jupiter+the+Giant+Planet&rft.place=Washington&rft.edition=2nd&rft.pub=Smithsonian+Books&rft.date=1997&rft_id=info%3Aoclcnum%2F224014042&rft.isbn=978-1-56098-685-0&rft.aulast=Beebe&rft.aufirst=R.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFBhardwajGladstone2000" class="citation journal cs1">Bhardwaj, Anil; Gladstone, G. Randall (2000). <a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F1998RG000046">"Auroral emissions of the giant planets"</a>. <a href="/wiki/Reviews_of_Geophysics" title="Reviews of Geophysics">Reviews of Geophysics</a>. 38 (3): 295–353. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2000RvGeo..38..295B">2000RvGeo..38..295B</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F1998RG000046">10.1029/1998RG000046</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Reviews+of+Geophysics&rft.atitle=Auroral+emissions+of+the+giant+planets&rft.volume=38&rft.issue=3&rft.pages=295-353&rft.date=2000&rft_id=info%3Adoi%2F10.1029%2F1998RG000046&rft_id=info%3Abibcode%2F2000RvGeo..38..295B&rft.aulast=Bhardwaj&rft.aufirst=Anil&rft.au=Gladstone%2C+G.+Randall&rft_id=https%3A%2F%2Fdoi.org%2F10.1029%252F1998RG000046&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Busse" class="citation journal cs1">Busse, F.H. (1976). "A simple model of convection in the Jovian atmosphere". <a href="/wiki/Icarus_(journal)" title="Icarus (journal)">Icarus</a>. 29 (2): 255–260. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1976Icar...29..255B">1976Icar...29..255B</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2F0019-1035%2876%2990053-1">10.1016/0019-1035(76)90053-1</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=A+simple+model+of+convection+in+the+Jovian+atmosphere&rft.volume=29&rft.issue=2&rft.pages=255-260&rft.date=1976&rft_id=info%3Adoi%2F10.1016%2F0019-1035%2876%2990053-1&rft_id=info%3Abibcode%2F1976Icar...29..255B&rft.aulast=Busse&rft.aufirst=F.H.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFEncrenaz2003" class="citation journal cs1"><a href="/wiki/Th%C3%A9r%C3%A8se_Encrenaz" title="Thérèse Encrenaz">Encrenaz, Thérèse</a> (February 2003). "ISO observations of the giant planets and Titan: what have we learnt?". Planetary and Space Science. 51 (2): 89–103. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003P&SS...51...89E">2003P&SS...51...89E</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2FS0032-0633%2802%2900145-9">10.1016/S0032-0633(02)00145-9</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Planetary+and+Space+Science&rft.atitle=ISO+observations+of+the+giant+planets+and+Titan%3A+what+have+we+learnt%3F&rft.volume=51&rft.issue=2&rft.pages=89-103&rft.date=2003-02&rft_id=info%3Adoi%2F10.1016%2FS0032-0633%2802%2900145-9&rft_id=info%3Abibcode%2F2003P%26SS...51...89E&rft.aulast=Encrenaz&rft.aufirst=Th%C3%A9r%C3%A8se&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Fletcher2010" class="citation journal cs1">Fletcher, Leigh N.; Orton, G.S.; Mousis, O.; Yanamandra-Fisher, P.; et al. (2010). <a rel="nofollow" class="external text" href="http://www.eso.org/public/archives/releases/sciencepapers/eso1010/eso1010.pdf">"Thermal structure and composition of Jupiter's Great Red Spot from high-resolution thermal imaging"</a> (PDF). Icarus. 208 (1): 306–328. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2010Icar..208..306F">2010Icar..208..306F</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.icarus.2010.01.005">10.1016/j.icarus.2010.01.005</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=Thermal+structure+and+composition+of+Jupiter%27s+Great+Red+Spot+from+high-resolution+thermal+imaging&rft.volume=208&rft.issue=1&rft.pages=306-328&rft.date=2010&rft_id=info%3Adoi%2F10.1016%2Fj.icarus.2010.01.005&rft_id=info%3Abibcode%2F2010Icar..208..306F&rft.aulast=Fletcher&rft.aufirst=Leigh+N.&rft.au=Orton%2C+G.S.&rft.au=Mousis%2C+O.&rft.au=Yanamandra-Fisher%2C+P.&rft.au=Parrish%2C+P.D.&rft.au=Irwin%2C+P.G.J.&rft.au=Fisher%2C+B.M.&rft.au=Vanzi%2C+L.&rft.au=Fujiyoshi%2C+T.&rft_id=http%3A%2F%2Fwww.eso.org%2Fpublic%2Farchives%2Freleases%2Fsciencepapers%2Feso1010%2Feso1010.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Go" class="citation journal cs1">Go, C.Y.; de Pater, I.; Wong, M.; Lockwood, S.; Marcus, P.; Asay-Davis, X.; Shetty, S. (2006). "Evolution Of The Oval Ba During 2004–2005". <a href="/wiki/Bulletin_of_the_American_Astronomical_Society" title="Bulletin of the American Astronomical Society">Bulletin of the American Astronomical Society</a>. 38: 495. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2006DPS....38.1102G">2006DPS....38.1102G</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Bulletin+of+the+American+Astronomical+Society&rft.atitle=Evolution+Of+The+Oval+Ba+During+2004%E2%80%932005&rft.volume=38&rft.pages=495&rft.date=2006&rft_id=info%3Abibcode%2F2006DPS....38.1102G&rft.aulast=Go&rft.aufirst=C.Y.&rft.au=de+Pater%2C+I.&rft.au=Wong%2C+M.&rft.au=Lockwood%2C+S.&rft.au=Marcus%2C+P.&rft.au=Asay-Davis%2C+X.&rft.au=Shetty%2C+S.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Graney" class="citation journal cs1">Graney, C. M. (2010). "Changes in the Cloud Belts of Jupiter, 1630–1664, as reported in the 1665 Astronomia Reformata of Giovanni Battista Riccioli". <a href="/wiki/Baltic_Astronomy" class="mw-redirect" title="Baltic Astronomy">Baltic Astronomy</a>. 19 (3–4): 266. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/1008.0566">1008.0566</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2010BaltA..19..265G">2010BaltA..19..265G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1515%2Fastro-2017-0425">10.1515/astro-2017-0425</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:117677021">117677021</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Baltic+Astronomy&rft.atitle=Changes+in+the+Cloud+Belts+of+Jupiter%2C+1630%E2%80%931664%2C+as+reported+in+the+1665+Astronomia+Reformata+of+Giovanni+Battista+Riccioli&rft.volume=19&rft.issue=3%E2%80%934&rft.pages=266&rft.date=2010&rft_id=info%3Aarxiv%2F1008.0566&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A117677021%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1515%2Fastro-2017-0425&rft_id=info%3Abibcode%2F2010BaltA..19..265G&rft.aulast=Graney&rft.aufirst=C.+M.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Guillot" class="citation journal cs1">Guillot, T. (1999). <a rel="nofollow" class="external text" href="https://cds.cern.ch/record/394768">"A comparison of the interiors of Jupiter and Saturn"</a>. <a href="/wiki/Planetary_and_Space_Science" title="Planetary and Space Science">Planetary and Space Science</a>. 47 (10–11): 1183–1200. <a href="/wiki/ArXiv_(identifier)" class="mw-redirect" title="ArXiv (identifier)">arXiv</a>:<a rel="nofollow" class="external text" href="https://arxiv.org/abs/astro-ph/9907402">astro-ph/9907402</a>. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1999P&SS...47.1183G">1999P&SS...47.1183G</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2FS0032-0633%2899%2900043-4">10.1016/S0032-0633(99)00043-4</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:19024073">19024073</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Planetary+and+Space+Science&rft.atitle=A+comparison+of+the+interiors+of+Jupiter+and+Saturn&rft.volume=47&rft.issue=10%E2%80%9311&rft.pages=1183-1200&rft.date=1999&rft_id=info%3Aarxiv%2Fastro-ph%2F9907402&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A19024073%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1016%2FS0032-0633%2899%2900043-4&rft_id=info%3Abibcode%2F1999P%26SS...47.1183G&rft.aulast=Guillot&rft.aufirst=T.&rft_id=https%3A%2F%2Fcds.cern.ch%2Frecord%2F394768&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Hammel" class="citation journal cs1">Hammel, H.B.; Lockwood, G.W.; Mills, J.R.; Barnet, C.D. (1995). "Hubble Space Telescope Imaging of Neptune's Cloud Structure in 1994". <a href="/wiki/Science_(journal)" title="Science (journal)">Science</a>. 268 (5218): 1740–1742. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1995Sci...268.1740H">1995Sci...268.1740H</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.268.5218.1740">10.1126/science.268.5218.1740</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/17834994">17834994</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:11688794">11688794</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=Hubble+Space+Telescope+Imaging+of+Neptune%27s+Cloud+Structure+in+1994&rft.volume=268&rft.issue=5218&rft.pages=1740-1742&rft.date=1995&rft_id=info%3Adoi%2F10.1126%2Fscience.268.5218.1740&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A11688794%23id-name%3DS2CID&rft_id=info%3Apmid%2F17834994&rft_id=info%3Abibcode%2F1995Sci...268.1740H&rft.aulast=Hammel&rft.aufirst=H.B.&rft.au=Lockwood%2C+G.W.&rft.au=Mills%2C+J.R.&rft.au=Barnet%2C+C.D.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Heimpel2005" class="citation journal cs1">Heimpel, M.; Aurnou, J.; Wicht, J. (2005). <a rel="nofollow" class="external text" href="https://escholarship.org/uc/item/8x49t27b">"Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model"</a>. <a href="/wiki/Nature_(journal)" title="Nature (journal)">Nature</a>. 438 (7065): 193–196. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005Natur.438..193H">2005Natur.438..193H</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fnature04208">10.1038/nature04208</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/16281029">16281029</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:4414668">4414668</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Simulation+of+equatorial+and+high-latitude+jets+on+Jupiter+in+a+deep+convection+model&rft.volume=438&rft.issue=7065&rft.pages=193-196&rft.date=2005&rft_id=info%3Adoi%2F10.1038%2Fnature04208&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A4414668%23id-name%3DS2CID&rft_id=info%3Apmid%2F16281029&rft_id=info%3Abibcode%2F2005Natur.438..193H&rft.aulast=Heimpel&rft.aufirst=M.&rft.au=Aurnou%2C+J.&rft.au=Wicht%2C+J.&rft_id=https%3A%2F%2Fescholarship.org%2Fuc%2Fitem%2F8x49t27b&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Hockey1999" class="citation book cs1">Hockey, T. (1999). Galileo's Planet: Observing Jupiter Before Photography. Bristol, Philadelphia: <a href="/wiki/Institute_of_Physics_Publishing" class="mw-redirect" title="Institute of Physics Publishing">Institute of Physics Publishing</a>. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-7503-0448-1" title="Special:BookSources/978-0-7503-0448-1"><bdi>978-0-7503-0448-1</bdi></a>. <a href="/wiki/OCLC_(identifier)" class="mw-redirect" title="OCLC (identifier)">OCLC</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/oclc/39733730">39733730</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Galileo%27s+Planet%3A+Observing+Jupiter+Before+Photography&rft.place=Bristol%2C+Philadelphia&rft.pub=Institute+of+Physics+Publishing&rft.date=1999&rft_id=info%3Aoclcnum%2F39733730&rft.isbn=978-0-7503-0448-1&rft.aulast=Hockey&rft.aufirst=T.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Ingersoll" class="citation encyclopaedia cs1">Ingersoll, A.P.; Dowling, T.E.; Gierasch, P.J.; et al. (2004). <a rel="nofollow" class="external text" href="http://www.lpl.arizona.edu/~showman/publications/ingersolletal-2004.pdf">"Dynamics of Jupiter's Atmosphere"</a> (PDF). In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.). Jupiter: The Planet, Satellites and Magnetosphere. Cambridge: <a href="/wiki/Cambridge_University_Press" title="Cambridge University Press">Cambridge University Press</a>. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-521-81808-7" title="Special:BookSources/978-0-521-81808-7"><bdi>978-0-521-81808-7</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=Dynamics+of+Jupiter%27s+Atmosphere&rft.btitle=Jupiter%3A+The+Planet%2C+Satellites+and+Magnetosphere&rft.place=Cambridge&rft.pub=Cambridge+University+Press&rft.date=2004&rft.isbn=978-0-521-81808-7&rft.aulast=Ingersoll&rft.aufirst=A.P.&rft.au=Dowling%2C+T.E.&rft.au=Gierasch%2C+P.J.&rft_id=http%3A%2F%2Fwww.lpl.arizona.edu%2F~showman%2Fpublications%2Fingersolletal-2004.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Ingersoll1969" class="citation journal cs1">Ingersoll, A.P.; Cuzzi, J.N. (1969). <a rel="nofollow" class="external text" href="https://authors.library.caltech.edu/3986/1/INGjas69b.pdf">"Dynamics of Jupiter's cloud bands"</a> (PDF). <a href="/wiki/Journal_of_the_Atmospheric_Sciences" title="Journal of the Atmospheric Sciences">Journal of the Atmospheric Sciences</a>. 26 (5): 981–985. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1969JAtS...26..981I">1969JAtS...26..981I</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%281969%29026%3C0981%3ADOJCB%3E2.0.CO%3B2">10.1175/1520-0469(1969)026<0981:DOJCB>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Dynamics+of+Jupiter%27s+cloud+bands&rft.volume=26&rft.issue=5&rft.pages=981-985&rft.date=1969&rft_id=info%3Adoi%2F10.1175%2F1520-0469%281969%29026%3C0981%3ADOJCB%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F1969JAtS...26..981I&rft.aulast=Ingersoll&rft.aufirst=A.P.&rft.au=Cuzzi%2C+J.N.&rft_id=https%3A%2F%2Fauthors.library.caltech.edu%2F3986%2F1%2FINGjas69b.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Irwin2003" class="citation book cs1">Irwin, P. (2003). Giant Planets of Our Solar System. Atmospheres, Composition, and Structure. <a href="/wiki/Springer_(publisher)" class="mw-redirect" title="Springer (publisher)">Springer</a> and <a href="/w/index.php?title=Praxis_Publishing&action=edit&redlink=1" class="new" title="Praxis Publishing (page does not exist)">Praxis</a>. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-3-540-00681-7" title="Special:BookSources/978-3-540-00681-7"><bdi>978-3-540-00681-7</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Giant+Planets+of+Our+Solar+System.+Atmospheres%2C+Composition%2C+and+Structure&rft.pub=Springer+and+Praxis&rft.date=2003&rft.isbn=978-3-540-00681-7&rft.aulast=Irwin&rft.aufirst=P.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Kunde" class="citation journal cs1">Kunde, V.G.; Flasar, F.M.; Jennings, D.E.; et al. (2004). <a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.1100240">"Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment"</a>. <a href="/wiki/Science_(journal)" title="Science (journal)">Science</a>. 305 (5690): 1582–1586. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2004Sci...305.1582K">2004Sci...305.1582K</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.1100240">10.1126/science.1100240</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/15319491">15319491</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:45296656">45296656</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=Jupiter%27s+Atmospheric+Composition+from+the+Cassini+Thermal+Infrared+Spectroscopy+Experiment&rft.volume=305&rft.issue=5690&rft.pages=1582-1586&rft.date=2004&rft_id=info%3Adoi%2F10.1126%2Fscience.1100240&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A45296656%23id-name%3DS2CID&rft_id=info%3Apmid%2F15319491&rft_id=info%3Abibcode%2F2004Sci...305.1582K&rft.aulast=Kunde&rft.aufirst=V.G.&rft.au=Flasar%2C+F.M.&rft.au=Jennings%2C+D.E.&rft_id=https%3A%2F%2Fdoi.org%2F10.1126%252Fscience.1100240&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Low" class="citation journal cs1">Low, F.J. (1966). "Observations of Venus, Jupiter, and Saturn at λ20 μ". <a href="/wiki/Astronomical_Journal" class="mw-redirect" title="Astronomical Journal">Astronomical Journal</a>. 71: 391. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1966AJ.....71R.391L">1966AJ.....71R.391L</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1086%2F110110">10.1086/110110</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Astronomical+Journal&rft.atitle=Observations+of+Venus%2C+Jupiter%2C+and+Saturn+at+%CE%BB20+%CE%BC&rft.volume=71&rft.pages=391&rft.date=1966&rft_id=info%3Adoi%2F10.1086%2F110110&rft_id=info%3Abibcode%2F1966AJ.....71R.391L&rft.aulast=Low&rft.aufirst=F.J.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="McKim" class="citation journal cs1">McKim, R.J. (1997). "P. B. Molesworth's discovery of the great South Tropical Disturbance on Jupiter, 1901". <a href="/wiki/Journal_of_the_British_Astronomical_Association" title="Journal of the British Astronomical Association">Journal of the British Astronomical Association</a>. 107 (5): 239–245. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1997JBAA..107..239M">1997JBAA..107..239M</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+British+Astronomical+Association&rft.atitle=P.+B.+Molesworth%27s+discovery+of+the+great+South+Tropical+Disturbance+on+Jupiter%2C+1901&rft.volume=107&rft.issue=5&rft.pages=239-245&rft.date=1997&rft_id=info%3Abibcode%2F1997JBAA..107..239M&rft.aulast=McKim&rft.aufirst=R.J.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFMiller_Aylward_et_al.2005" class="citation journal cs1">Miller, Steve; Aylward, Alan; Millward, George (January 2005). "Giant Planet Ionospheres and Thermospheres: The Importance of Ion-Neutral Coupling". Space Science Reviews. 116 (1–2): 319–343. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005SSRv..116..319M">2005SSRv..116..319M</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1007%2Fs11214-005-1960-4">10.1007/s11214-005-1960-4</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:119906560">119906560</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Space+Science+Reviews&rft.atitle=Giant+Planet+Ionospheres+and+Thermospheres%3A+The+Importance+of+Ion-Neutral+Coupling&rft.volume=116&rft.issue=1%E2%80%932&rft.pages=319-343&rft.date=2005-01&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A119906560%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1007%2Fs11214-005-1960-4&rft_id=info%3Abibcode%2F2005SSRv..116..319M&rft.aulast=Miller&rft.aufirst=Steve&rft.au=Aylward%2C+Alan&rft.au=Millward%2C+George&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Noll1995" class="citation journal cs1">Noll, K.S.; McGrath, M.A.; Weaver, H.A.; Yelle, R.V.; et al. (1995). "HST Spectroscopic Observations of Jupiter Following the Impact of Comet Shoemaker-Levy 9". Science. 267 (5202): 1307–1313. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1995Sci...267.1307N">1995Sci...267.1307N</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.7871428">10.1126/science.7871428</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/7871428">7871428</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:37686143">37686143</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=HST+Spectroscopic+Observations+of+Jupiter+Following+the+Impact+of+Comet+Shoemaker-Levy+9&rft.volume=267&rft.issue=5202&rft.pages=1307-1313&rft.date=1995&rft_id=info%3Adoi%2F10.1126%2Fscience.7871428&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A37686143%23id-name%3DS2CID&rft_id=info%3Apmid%2F7871428&rft_id=info%3Abibcode%2F1995Sci...267.1307N&rft.aulast=Noll&rft.aufirst=K.S.&rft.au=McGrath%2C+M.A.&rft.au=Weaver%2C+H.A.&rft.au=Yelle%2C+R.V.&rft.au=Trafton%2C+L.M.&rft.au=Atreya%2C+S.K.&rft.au=Caldwell%2C+J.J.&rft.au=Barnet%2C+C.&rft.au=Edgington%2C+S.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFPearl_Conrath_et_al.1990" class="citation journal cs1">Pearl, J. C.; Conrath, B. J.; Hanel, R. A.; Pirraglia, J. A.; Coustenis, A. (March 1990). "The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data". Icarus. 84 (1): 12–28. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1990Icar...84...12P">1990Icar...84...12P</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2F0019-1035%2890%2990155-3">10.1016/0019-1035(90)90155-3</a>. <a href="/wiki/ISSN_(identifier)" class="mw-redirect" title="ISSN (identifier)">ISSN</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/issn/0019-1035">0019-1035</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=The+albedo%2C+effective+temperature%2C+and+energy+balance+of+Uranus%2C+as+determined+from+Voyager+IRIS+data&rft.volume=84&rft.issue=1&rft.pages=12-28&rft.date=1990-03&rft.issn=0019-1035&rft_id=info%3Adoi%2F10.1016%2F0019-1035%2890%2990155-3&rft_id=info%3Abibcode%2F1990Icar...84...12P&rft.aulast=Pearl&rft.aufirst=J.+C.&rft.au=Conrath%2C+B.+J.&rft.au=Hanel%2C+R.+A.&rft.au=Pirraglia%2C+J.+A.&rft.au=Coustenis%2C+A.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Reese" class="citation journal cs1">Reese, E.J.; Solberg, H.G. (1966). "Recent measures of the latitude and longitude of Jupiter's red spot". <a href="/wiki/Icarus_(journal)" title="Icarus (journal)">Icarus</a>. 5 (1–6): 266–273. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1966Icar....5..266R">1966Icar....5..266R</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2F0019-1035%2866%2990036-4">10.1016/0019-1035(66)90036-4</a>. <a href="/wiki/Hdl_(identifier)" class="mw-redirect" title="Hdl (identifier)">hdl</a>:<a rel="nofollow" class="external text" href="https://hdl.handle.net/2060%2F19650022425">2060/19650022425</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=Recent+measures+of+the+latitude+and+longitude+of+Jupiter%27s+red+spot&rft.volume=5&rft.issue=1%E2%80%936&rft.pages=266-273&rft.date=1966&rft_id=info%3Ahdl%2F2060%2F19650022425&rft_id=info%3Adoi%2F10.1016%2F0019-1035%2866%2990036-4&rft_id=info%3Abibcode%2F1966Icar....5..266R&rft.aulast=Reese&rft.aufirst=E.J.&rft.au=Solberg%2C+H.G.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Ridpath" class="citation book cs1">Ridpath, I. (1998). Norton's Star Atlas and Reference Handbook (19th ed.). Harlow: <a href="/wiki/Addison_Wesley" class="mw-redirect" title="Addison Wesley">Addison Wesley</a> <a href="/wiki/Longman" title="Longman">Longman</a>. p. 107. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-582-35655-9" title="Special:BookSources/978-0-582-35655-9"><bdi>978-0-582-35655-9</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Norton%27s+Star+Atlas+and+Reference+Handbook&rft.place=Harlow&rft.pages=107&rft.edition=19th&rft.pub=Addison+Wesley+Longman&rft.date=1998&rft.isbn=978-0-582-35655-9&rft.aulast=Ridpath&rft.aufirst=I.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Rogers" class="citation book cs1">Rogers, J.H. (1995). The Giant Planet Jupiter. Cambridge: <a href="/wiki/Cambridge_University_Press" title="Cambridge University Press">Cambridge University Press</a>. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-521-41008-3" title="Special:BookSources/978-0-521-41008-3"><bdi>978-0-521-41008-3</bdi></a>. <a href="/wiki/OCLC_(identifier)" class="mw-redirect" title="OCLC (identifier)">OCLC</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/oclc/219591510">219591510</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=The+Giant+Planet+Jupiter&rft.place=Cambridge&rft.pub=Cambridge+University+Press&rft.date=1995&rft_id=info%3Aoclcnum%2F219591510&rft.isbn=978-0-521-41008-3&rft.aulast=Rogers&rft.aufirst=J.H.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Rogers2001" class="citation journal cs1">Rogers, J.H.; Metig, H.J. (2001). <a rel="nofollow" class="external text" href="http://www.britastro.org/jupiter/JBAA111_Jup98.pdf">"Jupiter in 1998/99"</a> (PDF). <a href="/wiki/Journal_of_the_British_Astronomical_Association" title="Journal of the British Astronomical Association">Journal of the British Astronomical Association</a>. 111 (6): 321–332. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2001JBAA..111..321R">2001JBAA..111..321R</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+British+Astronomical+Association&rft.atitle=Jupiter+in+1998%2F99&rft.volume=111&rft.issue=6&rft.pages=321-332&rft.date=2001&rft_id=info%3Abibcode%2F2001JBAA..111..321R&rft.aulast=Rogers&rft.aufirst=J.H.&rft.au=Metig%2C+H.J.&rft_id=http%3A%2F%2Fwww.britastro.org%2Fjupiter%2FJBAA111_Jup98.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Rogers2003" class="citation journal cs1">Rogers, J.H. (2003). <a rel="nofollow" class="external text" href="http://www.britastro.org/jupiter/JBAA113-Jup9900_II-IR.pdf">"Jupiter in 1999/2000. II: Infrared wavelengths"</a> (PDF). <a href="/wiki/Journal_of_the_British_Astronomical_Association" title="Journal of the British Astronomical Association">Journal of the British Astronomical Association</a>. 113 (3): 136–140. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003JBAA..113..136R">2003JBAA..113..136R</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+British+Astronomical+Association&rft.atitle=Jupiter+in+1999%2F2000.+II%3A+Infrared+wavelengths&rft.volume=113&rft.issue=3&rft.pages=136-140&rft.date=2003&rft_id=info%3Abibcode%2F2003JBAA..113..136R&rft.aulast=Rogers&rft.aufirst=J.H.&rft_id=http%3A%2F%2Fwww.britastro.org%2Fjupiter%2FJBAA113-Jup9900_II-IR.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Rogers2008b" class="citation journal cs1">Rogers, J.H. (2008). <a rel="nofollow" class="external text" href="http://www.britastro.org/jupiter/JBAA-118-1_GRS-paper.pdf">"The accelerating circulation of Jupiter's Great Red Spot"</a> (PDF). <a href="/wiki/Journal_of_the_British_Astronomical_Association" title="Journal of the British Astronomical Association">Journal of the British Astronomical Association</a>. 118 (1): 14–20. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2008JBAA..118...14R">2008JBAA..118...14R</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+British+Astronomical+Association&rft.atitle=The+accelerating+circulation+of+Jupiter%27s+Great+Red+Spot&rft.volume=118&rft.issue=1&rft.pages=14-20&rft.date=2008&rft_id=info%3Abibcode%2F2008JBAA..118...14R&rft.aulast=Rogers&rft.aufirst=J.H.&rft_id=http%3A%2F%2Fwww.britastro.org%2Fjupiter%2FJBAA-118-1_GRS-paper.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Sanchez2001" class="citation journal cs1">Sanchez-Lavega, A.; Orton, G.S.; Morales R.; et al. (2001). "The Merger of Two Giant Anticyclones in the Atmosphere of Jupiter". <a href="/wiki/Icarus_(journal)" title="Icarus (journal)">Icarus</a>. 149 (2): 491–495. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2001Icar..149..491S">2001Icar..149..491S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1006%2Ficar.2000.6548">10.1006/icar.2000.6548</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=The+Merger+of+Two+Giant+Anticyclones+in+the+Atmosphere+of+Jupiter&rft.volume=149&rft.issue=2&rft.pages=491-495&rft.date=2001&rft_id=info%3Adoi%2F10.1006%2Ficar.2000.6548&rft_id=info%3Abibcode%2F2001Icar..149..491S&rft.aulast=Sanchez-Lavega&rft.aufirst=A.&rft.au=Orton%2C+G.S.&rft.au=Morales+R.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Sanchez2008" class="citation journal cs1">Sanchez-Lavega, A.; Orton, G.S.; Hueso, S.; et al. (2008). <a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fnature06533">"Depth of the strong Jovian jet from a planetary scale disturbance driven by storms"</a>. <a href="/wiki/Nature_(journal)" title="Nature (journal)">Nature</a>. 451 (7177): 437–440. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2008Natur.451..437S">2008Natur.451..437S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fnature06533">10.1038/nature06533</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/18216848">18216848</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Depth+of+the+strong+Jovian+jet+from+a+planetary+scale+disturbance+driven+by+storms&rft.volume=451&rft.issue=7177&rft.pages=437-440&rft.date=2008&rft_id=info%3Apmid%2F18216848&rft_id=info%3Adoi%2F10.1038%2Fnature06533&rft_id=info%3Abibcode%2F2008Natur.451..437S&rft.aulast=Sanchez-Lavega&rft.aufirst=A.&rft.au=Orton%2C+G.S.&rft.au=Hueso%2C+S.&rft_id=https%3A%2F%2Fdoi.org%2F10.1038%252Fnature06533&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Sieff" class="citation journal cs1">Seiff, A.; Kirk, D.B.; Knight, T.C.D.; et al. (1998). "Thermal structure of Jupiter's atmosphere near the edge of a 5-μm hot spot in the north equatorial belt". <a href="/wiki/Journal_of_Geophysical_Research" title="Journal of Geophysical Research">Journal of Geophysical Research</a>. 103 (E10): 22857–22889. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1998JGR...10322857S">1998JGR...10322857S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F98JE01766">10.1029/98JE01766</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+Geophysical+Research&rft.atitle=Thermal+structure+of+Jupiter%27s+atmosphere+near+the+edge+of+a+5-%CE%BCm+hot+spot+in+the+north+equatorial+belt&rft.volume=103&rft.issue=E10&rft.pages=22857-22889&rft.date=1998&rft_id=info%3Adoi%2F10.1029%2F98JE01766&rft_id=info%3Abibcode%2F1998JGR...10322857S&rft.aulast=Seiff&rft.aufirst=A.&rft.au=Kirk%2C+D.B.&rft.au=Knight%2C+T.C.D.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Smith" class="citation journal cs1">Smith, B.A.; Soderblom, L.A.; Johnson, T.V.; et al. (1979). "The Jupiter system through the eyes of Voyager 1". <a href="/wiki/Science_(journal)" title="Science (journal)">Science</a>. 204 (4396): 951–957, 960–972. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1979Sci...204..951S">1979Sci...204..951S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1126%2Fscience.204.4396.951">10.1126/science.204.4396.951</a>. <a href="/wiki/PMID_(identifier)" class="mw-redirect" title="PMID (identifier)">PMID</a> <a rel="nofollow" class="external text" href="https://pubmed.ncbi.nlm.nih.gov/17800430">17800430</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:33147728">33147728</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Science&rft.atitle=The+Jupiter+system+through+the+eyes+of+Voyager+1&rft.volume=204&rft.issue=4396&rft.pages=951-957%2C+960-972&rft.date=1979&rft_id=info%3Adoi%2F10.1126%2Fscience.204.4396.951&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A33147728%23id-name%3DS2CID&rft_id=info%3Apmid%2F17800430&rft_id=info%3Abibcode%2F1979Sci...204..951S&rft.aulast=Smith&rft.aufirst=B.A.&rft.au=Soderblom%2C+L.A.&rft.au=Johnson%2C+T.V.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Stone" class="citation journal cs1">Stone, P.H. (1974). <a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%281974%29031%3C1471%3AOJROR%3E2.0.CO%3B2">"On Jupiter's Rate of Rotation"</a>. <a href="/wiki/Journal_of_the_Atmospheric_Sciences" title="Journal of the Atmospheric Sciences">Journal of the Atmospheric Sciences</a>. 31 (5): 1471–1472. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1974JAtS...31.1471S">1974JAtS...31.1471S</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%281974%29031%3C1471%3AOJROR%3E2.0.CO%3B2">10.1175/1520-0469(1974)031<1471:OJROR>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=On+Jupiter%27s+Rate+of+Rotation&rft.volume=31&rft.issue=5&rft.pages=1471-1472&rft.date=1974&rft_id=info%3Adoi%2F10.1175%2F1520-0469%281974%29031%3C1471%3AOJROR%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F1974JAtS...31.1471S&rft.aulast=Stone&rft.aufirst=P.H.&rft_id=https%3A%2F%2Fdoi.org%2F10.1175%252F1520-0469%25281974%2529031%253C1471%253AOJROR%253E2.0.CO%253B2&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Vasavada" class="citation journal cs1">Vasavada, A.R.; Showman, A. (2005). "Jovian atmospheric dynamics: An update after Galileo and Cassini". <a href="/wiki/Reports_on_Progress_in_Physics" title="Reports on Progress in Physics">Reports on Progress in Physics</a>. 68 (8): 1935–1996. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005RPPh...68.1935V">2005RPPh...68.1935V</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1088%2F0034-4885%2F68%2F8%2FR06">10.1088/0034-4885/68/8/R06</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:53596671">53596671</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Reports+on+Progress+in+Physics&rft.atitle=Jovian+atmospheric+dynamics%3A+An+update+after+Galileo+and+Cassini&rft.volume=68&rft.issue=8&rft.pages=1935-1996&rft.date=2005&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A53596671%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1088%2F0034-4885%2F68%2F8%2FR06&rft_id=info%3Abibcode%2F2005RPPh...68.1935V&rft.aulast=Vasavada&rft.aufirst=A.R.&rft.au=Showman%2C+A.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="West" class="citation book cs1">West, R.A.; Baines, K.H.; Friedson, A.J.; et al. (2004). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20140823091421/http://www.gps.caltech.edu/~ulyana/www_papers/west_Ch5_us.pdf">"Jovian Clouds and Haze"</a> (PDF). In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.). Jupiter: The Planet, Satellites and Magnetosphere. Cambridge: <a href="/wiki/Cambridge_University_Press" title="Cambridge University Press">Cambridge University Press</a>. Archived from <a rel="nofollow" class="external text" href="http://www.gps.caltech.edu/~ulyana/www_papers/west_Ch5_us.pdf">the original</a> (PDF) on 2014-08-23. Retrieved 2010-08-21.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=Jovian+Clouds+and+Haze&rft.btitle=Jupiter%3A+The+Planet%2C+Satellites+and+Magnetosphere&rft.place=Cambridge&rft.pub=Cambridge+University+Press&rft.date=2004&rft.aulast=West&rft.aufirst=R.A.&rft.au=Baines%2C+K.H.&rft.au=Friedson%2C+A.J.&rft_id=http%3A%2F%2Fwww.gps.caltech.edu%2F~ulyana%2Fwww_papers%2Fwest_Ch5_us.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="Yelle" class="citation encyclopaedia cs1">Yelle, R.V.; Miller, S. (2004). <a rel="nofollow" class="external text" href="http://www.lpl.arizona.edu/~yelle/eprints/Yelle04c.pdf">"Jupiter's Thermosphere and Ionosphere"</a> (PDF). In Bagenal, Fran.; Dowling, Timothy E.; McKinnon, William B. (eds.). Jupiter: The Planet, Satellites and Magnetosphere. Cambridge: <a href="/wiki/Cambridge_University_Press" title="Cambridge University Press">Cambridge University Press</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=Jupiter%27s+Thermosphere+and+Ionosphere&rft.btitle=Jupiter%3A+The+Planet%2C+Satellites+and+Magnetosphere&rft.place=Cambridge&rft.pub=Cambridge+University+Press&rft.date=2004&rft.aulast=Yelle&rft.aufirst=R.V.&rft.au=Miller%2C+S.&rft_id=http%3A%2F%2Fwww.lpl.arizona.edu%2F~yelle%2Feprints%2FYelle04c.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li></ul> </div> <div class="mw-heading mw-heading2"><h2 id="Further_reading">Further reading</h2>[<a href="/w/index.php?title=Atmosphere_of_Jupiter&action=edit&section=26" title="Edit section: Further reading">edit</a>]</div> <ul><li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREF[Numerous_authors]1999" class="citation book cs1">[Numerous authors] (1999). Beatty, Kelly J.; Peterson, Carolyn Collins; Chaiki, Andrew (eds.). The New Solar System (4th ed.). Massachusetts: Sky Publishing Corporation. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-933346-86-4" title="Special:BookSources/978-0-933346-86-4"><bdi>978-0-933346-86-4</bdi></a>. <a href="/wiki/OCLC_(identifier)" class="mw-redirect" title="OCLC (identifier)">OCLC</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/oclc/39464951">39464951</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=The+New+Solar+System&rft.place=Massachusetts&rft.edition=4th&rft.pub=Sky+Publishing+Corporation&rft.date=1999&rft_id=info%3Aoclcnum%2F39464951&rft.isbn=978-0-933346-86-4&rft.au=%5BNumerous+authors%5D&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFPeek1981" class="citation book cs1"><a href="/wiki/Bertrand_Meigh_Peek" title="Bertrand Meigh Peek">Peek, Bertrand M.</a> (1981). <a rel="nofollow" class="external text" href="https://archive.org/details/planetjupiter00peek">The Planet Jupiter: The Observer's Handbook</a> (Revised ed.). London: Faber and Faber Limited. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-571-18026-4" title="Special:BookSources/978-0-571-18026-4"><bdi>978-0-571-18026-4</bdi></a>. <a href="/wiki/OCLC_(identifier)" class="mw-redirect" title="OCLC (identifier)">OCLC</a> <a rel="nofollow" class="external text" href="https://search.worldcat.org/oclc/8318939">8318939</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=The+Planet+Jupiter%3A+The+Observer%27s+Handbook&rft.place=London&rft.edition=Revised&rft.pub=Faber+and+Faber+Limited&rft.date=1981&rft_id=info%3Aoclcnum%2F8318939&rft.isbn=978-0-571-18026-4&rft.aulast=Peek&rft.aufirst=Bertrand+M.&rft_id=https%3A%2F%2Farchive.org%2Fdetails%2Fplanetjupiter00peek&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFYang2004" class="citation news cs1">Yang, Sarah (April 21, 2004). <a rel="nofollow" class="external text" href="http://www.berkeley.edu/news/media/releases/2004/04/21_jupiter.shtml">"Researcher predicts global climate change on Jupiter as giant planet's spots disappear"</a>. UC Berkeley News. <a rel="nofollow" class="external text" href="https://web.archive.org/web/20070609214744/http://www.berkeley.edu/news/media/releases/2004/04/21_jupiter.shtml">Archived</a> from the original on 9 June 2007. Retrieved 2007-06-14.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Researcher+predicts+global+climate+change+on+Jupiter+as+giant+planet%27s+spots+disappear&rft.date=2004-04-21&rft.aulast=Yang&rft.aufirst=Sarah&rft_id=http%3A%2F%2Fwww.berkeley.edu%2Fnews%2Fmedia%2Freleases%2F2004%2F04%2F21_jupiter.shtml&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFYoussef,_AshrafMarcus,_Philip_S.2003" class="citation journal cs1">Youssef, Ashraf; Marcus, Philip S. (2003). "The dynamics of jovian white ovals from formation to merger". Icarus. 162 (1): 74–93. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003Icar..162...74Y">2003Icar..162...74Y</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2FS0019-1035%2802%2900060-X">10.1016/S0019-1035(02)00060-X</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=The+dynamics+of+jovian+white+ovals+from+formation+to+merger&rft.volume=162&rft.issue=1&rft.pages=74-93&rft.date=2003&rft_id=info%3Adoi%2F10.1016%2FS0019-1035%2802%2900060-X&rft_id=info%3Abibcode%2F2003Icar..162...74Y&rft.au=Youssef%2C+Ashraf&rft.au=Marcus%2C+Philip+S.&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.1975" class="citation journal cs1">Williams, Gareth P. (1975). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw7501.pdf">"Jupiter's atmospheric circulation"</a> (PDF). Nature. 257 (5529): 778. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1975Natur.257..778W">1975Natur.257..778W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2F257778a0">10.1038/257778a0</a>. <a href="/wiki/S2CID_(identifier)" class="mw-redirect" title="S2CID (identifier)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:43539227">43539227</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=Jupiter%27s+atmospheric+circulation&rft.volume=257&rft.issue=5529&rft.pages=778&rft.date=1975&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A43539227%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1038%2F257778a0&rft_id=info%3Abibcode%2F1975Natur.257..778W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw7501.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.1978" class="citation journal cs1">Williams, Gareth P. (1978). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw7801.pdf">"Planetary Circulations: 1. Barotropic representation of Jovian and terrestrial turbulence"</a> (PDF). Journal of the Atmospheric Sciences. 35 (8): 1399–1426. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1978JAtS...35.1399W">1978JAtS...35.1399W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%281978%29035%3C1399%3APCBROJ%3E2.0.CO%3B2">10.1175/1520-0469(1978)035<1399:PCBROJ>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Planetary+Circulations%3A+1.+Barotropic+representation+of+Jovian+and+terrestrial+turbulence&rft.volume=35&rft.issue=8&rft.pages=1399-1426&rft.date=1978&rft_id=info%3Adoi%2F10.1175%2F1520-0469%281978%29035%3C1399%3APCBROJ%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F1978JAtS...35.1399W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw7801.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.1985" class="citation book cs1">Williams, Gareth P. (1985). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw8502.pdf">"Jovian and Comparative Atmospheric Modeling Gareth"</a> (PDF). Jovian and comparative atmospheric modeling. Advances in Geophysics. Vol. 28A. pp. 381–429. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1985AdGeo..28..381W">1985AdGeo..28..381W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2FS0065-2687%2808%2960231-9">10.1016/S0065-2687(08)60231-9</a>. <a href="/wiki/ISBN_(identifier)" class="mw-redirect" title="ISBN (identifier)">ISBN</a> <a href="/wiki/Special:BookSources/978-0-12-018828-4" title="Special:BookSources/978-0-12-018828-4"><bdi>978-0-12-018828-4</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=Jovian+and+Comparative+Atmospheric+Modeling+Gareth&rft.btitle=Jovian+and+comparative+atmospheric+modeling&rft.series=Advances+in+Geophysics&rft.pages=381-429&rft.date=1985&rft_id=info%3Adoi%2F10.1016%2FS0065-2687%2808%2960231-9&rft_id=info%3Abibcode%2F1985AdGeo..28..381W&rft.isbn=978-0-12-018828-4&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw8502.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.1997" class="citation journal cs1">Williams, Gareth P. (1997). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw9701.pdf">"Planetary vortices and Jupiter's vertical structure"</a> (PDF). Journal of Geophysical Research. 102 (E4): 9303–9308. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1997JGR...102.9303W">1997JGR...102.9303W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1029%2F97JE00520">10.1029/97JE00520</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+Geophysical+Research&rft.atitle=Planetary+vortices+and+Jupiter%27s+vertical+structure&rft.volume=102&rft.issue=E4&rft.pages=9303-9308&rft.date=1997&rft_id=info%3Adoi%2F10.1029%2F97JE00520&rft_id=info%3Abibcode%2F1997JGR...102.9303W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw9701.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.1996" class="citation journal cs1">Williams, Gareth P. (1996). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw9601.pdf">"Jovian Dynamics. Part I: Vortex stability, structure, and genesis"</a> (PDF). Journal of the Atmospheric Sciences. 53 (18): 2685–2734. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1996JAtS...53.2685W">1996JAtS...53.2685W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%281996%29053%3C2685%3AJDPVSS%3E2.0.CO%3B2">10.1175/1520-0469(1996)053<2685:JDPVSS>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Jovian+Dynamics.+Part+I%3A+Vortex+stability%2C+structure%2C+and+genesis&rft.volume=53&rft.issue=18&rft.pages=2685-2734&rft.date=1996&rft_id=info%3Adoi%2F10.1175%2F1520-0469%281996%29053%3C2685%3AJDPVSS%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F1996JAtS...53.2685W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw9601.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.2002" class="citation journal cs1">Williams, Gareth P. (2002). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gpw0201.pdf">"Jovian Dynamics.Part II: The genesis and equilibration of vortex sets"</a> (PDF). Journal of the Atmospheric Sciences. 59 (8): 1356–1370. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2002JAtS...59.1356W">2002JAtS...59.1356W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%282002%29059%3C1356%3AJDPITG%3E2.0.CO%3B2">10.1175/1520-0469(2002)059<1356:JDPITG>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Jovian+Dynamics.Part+II%3A+The+genesis+and+equilibration+of+vortex+sets&rft.volume=59&rft.issue=8&rft.pages=1356-1370&rft.date=2002&rft_id=info%3Adoi%2F10.1175%2F1520-0469%282002%29059%3C1356%3AJDPITG%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F2002JAtS...59.1356W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgpw0201.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.2003" class="citation journal cs1">Williams, Gareth P. (2003). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw0301.pdf">"Jovian Dynamics, Part III: Multiple, migrating, and equatorial jets"</a> (PDF). Journal of the Atmospheric Sciences. 60 (10): 1270–1296. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003JAtS...60.1270W">2003JAtS...60.1270W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%282003%2960%3C1270%3AJDPIMM%3E2.0.CO%3B2">10.1175/1520-0469(2003)60<1270:JDPIMM>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Jovian+Dynamics%2C+Part+III%3A+Multiple%2C+migrating%2C+and+equatorial+jets&rft.volume=60&rft.issue=10&rft.pages=1270-1296&rft.date=2003&rft_id=info%3Adoi%2F10.1175%2F1520-0469%282003%2960%3C1270%3AJDPIMM%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F2003JAtS...60.1270W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw0301.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.2003" class="citation journal cs1">Williams, Gareth P. (2003). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw0304.pdf">"Super Circulations"</a> (PDF). Bulletin of the American Meteorological Society. 84 (9): 1190.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Bulletin+of+the+American+Meteorological+Society&rft.atitle=Super+Circulations&rft.volume=84&rft.issue=9&rft.pages=1190&rft.date=2003&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw0304.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.2003" class="citation journal cs1">Williams, Gareth P. (2003). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw0303.pdf">"Barotropic instability and equatorial superrotation"</a> (PDF). Journal of the Atmospheric Sciences. 60 (17): 2136–2152. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003JAtS...60.2136W">2003JAtS...60.2136W</a>. <a href="/wiki/CiteSeerX_(identifier)" class="mw-redirect" title="CiteSeerX (identifier)">CiteSeerX</a> <a rel="nofollow" class="external text" href="https://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.144.5975">10.1.1.144.5975</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2F1520-0469%282003%29060%3C2136%3ABIAES%3E2.0.CO%3B2">10.1175/1520-0469(2003)060<2136:BIAES>2.0.CO;2</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Atmospheric+Sciences&rft.atitle=Barotropic+instability+and+equatorial+superrotation&rft.volume=60&rft.issue=17&rft.pages=2136-2152&rft.date=2003&rft_id=https%3A%2F%2Fciteseerx.ist.psu.edu%2Fviewdoc%2Fsummary%3Fdoi%3D10.1.1.144.5975%23id-name%3DCiteSeerX&rft_id=info%3Adoi%2F10.1175%2F1520-0469%282003%29060%3C2136%3ABIAES%3E2.0.CO%3B2&rft_id=info%3Abibcode%2F2003JAtS...60.2136W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw0303.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.2003" class="citation journal cs1">Williams, Gareth P. (2003). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw0302.pdf">"Jet sets"</a> (PDF). Journal of the Meteorological Society of Japan. 81 (3): 439–476. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003JMeSJ..81..439W">2003JMeSJ..81..439W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.2151%2Fjmsj.81.439">10.2151/jmsj.81.439</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Journal+of+the+Meteorological+Society+of+Japan&rft.atitle=Jet+sets&rft.volume=81&rft.issue=3&rft.pages=439-476&rft.date=2003&rft_id=info%3Adoi%2F10.2151%2Fjmsj.81.439&rft_id=info%3Abibcode%2F2003JMeSJ..81..439W&rft.au=Williams%2C+Gareth+P.&rft_id=http%3A%2F%2Fwww.gfdl.noaa.gov%2Fbibliography%2Frelated_files%2Fgw0302.pdf&rfr_id=info%3Asid%2Fen.wikipedia.org%3AAtmosphere+of+Jupiter" class="Z3988"></li> <li><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1238218222"><cite id="CITEREFWilliams,_Gareth_P.2006" class="citation journal cs1">Williams, Gareth P. (2006). <a rel="nofollow" class="external text" href="http://www.gfdl.noaa.gov/bibliography/related_files/gw0601.pdf">"Equatorial Superrotation and Barotropic Instability: Static Stability Variants"</a> (PDF). Journal of the Atmospheric Sciences. 63 (5): 1548–1557. <a href="/wiki/Bibcode_(identifier)" class="mw-redirect" title="Bibcode (identifier)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2006JAtS...63.1548W">2006JAtS...63.1548W</a>. <a href="/wiki/Doi_(identifier)" class="mw-redirect" title="Doi (identifier)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1175%2FJAS3711.1">10.1175/JAS3711.1</a>.</cite><span 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.portal-bar{font-size:88%;font-weight:bold;display:flex;flex-flow:column wrap;align-items:baseline}.mw-parser-output .portal-bar-header{text-align:center;flex:0;padding-left:0.5em;margin:0 auto}.mw-parser-output .portal-bar-related{font-size:100%;align-items:flex-start}.mw-parser-output .portal-bar-content{display:flex;flex-flow:row wrap;align-items:center;flex:0;column-gap:1em;border-top:1px solid #a2a9b1;margin:0 auto;list-style:none}.mw-parser-output .portal-bar-content-related{border-top:none;margin:0;list-style:none}}.mw-parser-output .navbox+link+.portal-bar,.mw-parser-output .navbox+style+.portal-bar,.mw-parser-output .navbox+link+.portal-bar-bordered,.mw-parser-output .navbox+style+.portal-bar-bordered,.mw-parser-output .sister-bar+link+.portal-bar,.mw-parser-output .sister-bar+style+.portal-bar,.mw-parser-output .portal-bar+.navbox-styles+.navbox,.mw-parser-output .portal-bar+.navbox-styles+.sister-bar{margin-top:-1px}</style><div class="portal-bar noprint metadata noviewer portal-bar-bordered" role="navigation" aria-label="Portals"><a href="/wiki/Wikipedia:Contents/Portals" title="Wikipedia:Contents/Portals">Portals</a>:<ul class="portal-bar-content"><li class="portal-bar-item"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/19px-Crab_Nebula.jpg" decoding="async" width="19" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/29px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/38px-Crab_Nebula.jpg 2x" data-file-width="3864" data-file-height="3864" /> <a href="/wiki/Portal:Astronomy" title="Portal:Astronomy">Astronomy</a></li><li class="portal-bar-item"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/RocketSunIcon.svg/19px-RocketSunIcon.svg.png" decoding="async" width="19" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/RocketSunIcon.svg/29px-RocketSunIcon.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d6/RocketSunIcon.svg/38px-RocketSunIcon.svg.png 2x" data-file-width="128" data-file-height="128" /> <a href="/wiki/Portal:Spaceflight" title="Portal:Spaceflight">Spaceflight</a></li><li class="portal-bar-item"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/15px-Solar_system.jpg" decoding="async" width="15" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/23px-Solar_system.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/30px-Solar_system.jpg 2x" data-file-width="4500" data-file-height="5600" /> <a href="/wiki/Portal:Solar_System" title="Portal:Solar System">Solar System</a></li><li class="portal-bar-item"><a href="/wiki/File:Cumulus_clouds_in_fair_weather.jpeg" class="mw-file-description"><img alt="icon" src="//upload.wikimedia.org/wikipedia/commons/thumb/b/b5/Cumulus_clouds_in_fair_weather.jpeg/21px-Cumulus_clouds_in_fair_weather.jpeg" decoding="async" width="21" height="16" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/b5/Cumulus_clouds_in_fair_weather.jpeg/32px-Cumulus_clouds_in_fair_weather.jpeg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/b5/Cumulus_clouds_in_fair_weather.jpeg/42px-Cumulus_clouds_in_fair_weather.jpeg 2x" data-file-width="800" data-file-height="600" /></a> <a href="/wiki/Portal:Weather" title="Portal:Weather">Weather</a></li><li class="portal-bar-item"><a href="/wiki/File:Nuvola_apps_kalzium.svg" class="mw-file-description"><img alt="icon" src="//upload.wikimedia.org/wikipedia/commons/thumb/8/8b/Nuvola_apps_kalzium.svg/19px-Nuvola_apps_kalzium.svg.png" decoding="async" width="19" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/8b/Nuvola_apps_kalzium.svg/29px-Nuvola_apps_kalzium.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/8b/Nuvola_apps_kalzium.svg/38px-Nuvola_apps_kalzium.svg.png 2x" data-file-width="128" data-file-height="128" /></a> <a href="/wiki/Portal:Science" title="Portal:Science">Science</a></li><li class="portal-bar-item"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/5/5c/Earth-moon.jpg/21px-Earth-moon.jpg" decoding="async" width="21" height="17" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5c/Earth-moon.jpg/32px-Earth-moon.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5c/Earth-moon.jpg/42px-Earth-moon.jpg 2x" data-file-width="3000" data-file-height="2400" /> <a href="/wiki/Portal:Outer_space" title="Portal:Outer space">Outer space</a></li></ul></div> <div class="navbox-styles"><style data-mw-deduplicate="TemplateStyles:r1129693374">.mw-parser-output .hlist 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.hlist td ol,.mw-parser-output .navbox .hlist td ul,.mw-parser-output .navbox td.hlist dl,.mw-parser-output .navbox td.hlist ol,.mw-parser-output .navbox td.hlist ul{padding:0.125em 0}.mw-parser-output .navbox .navbar{display:block;font-size:100%}.mw-parser-output .navbox-title .navbar{float:left;text-align:left;margin-right:0.5em}body.skin--responsive .mw-parser-output .navbox-image img{max-width:none!important}@media print{body.ns-0 .mw-parser-output .navbox{display:none!important}}</style></div><div role="navigation" class="navbox" aria-labelledby="Jupiter" style="padding:3px"><table class="nowraplinks hlist mw-collapsible autocollapse navbox-inner" style="border-spacing:0;background:transparent;color:inherit"><tbody><tr><th scope="col" class="navbox-title" colspan="3"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1129693374"><style data-mw-deduplicate="TemplateStyles:r1239400231">.mw-parser-output .navbar{display:inline;font-size:88%;font-weight:normal}.mw-parser-output .navbar-collapse{float:left;text-align:left}.mw-parser-output .navbar-boxtext{word-spacing:0}.mw-parser-output .navbar ul{display:inline-block;white-space:nowrap;line-height:inherit}.mw-parser-output .navbar-brackets::before{margin-right:-0.125em;content:"[ "}.mw-parser-output .navbar-brackets::after{margin-left:-0.125em;content:" ]"}.mw-parser-output .navbar li{word-spacing:-0.125em}.mw-parser-output .navbar a>span,.mw-parser-output .navbar a>abbr{text-decoration:inherit}.mw-parser-output .navbar-mini abbr{font-variant:small-caps;border-bottom:none;text-decoration:none;cursor:inherit}.mw-parser-output .navbar-ct-full{font-size:114%;margin:0 7em}.mw-parser-output .navbar-ct-mini{font-size:114%;margin:0 4em}html.skin-theme-clientpref-night .mw-parser-output .navbar li a abbr{color:var(--color-base)!important}@media(prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .navbar li a abbr{color:var(--color-base)!important}}@media print{.mw-parser-output .navbar{display:none!important}}</style><div class="navbar plainlinks hlist navbar-mini"><ul><li class="nv-view"><a href="/wiki/Template:Jupiter" title="Template:Jupiter"><abbr title="View this template">v</abbr></a></li><li class="nv-talk"><a href="/wiki/Template_talk:Jupiter" title="Template talk:Jupiter"><abbr title="Discuss this template">t</abbr></a></li><li class="nv-edit"><a href="/wiki/Special:EditPage/Template:Jupiter" title="Special:EditPage/Template:Jupiter"><abbr title="Edit this template">e</abbr></a></li></ul></div><div id="Jupiter" style="font-size:114%;margin:0 4em"><a href="/wiki/Jupiter" title="Jupiter">Jupiter</a></div></th></tr><tr><td class="navbox-abovebelow" colspan="3"><div> <ul><li><a href="/wiki/Outline_of_Jupiter" title="Outline of Jupiter">Outline of Jupiter</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Geography</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a class="mw-selflink selflink">Atmosphere</a> <ul><li><a href="/wiki/Great_Red_Spot" title="Great Red Spot">Great Red Spot</a></li></ul></li> <li><a href="/wiki/Magnetosphere_of_Jupiter" title="Magnetosphere of Jupiter">Magnetosphere</a></li> <li><a href="/wiki/Rings_of_Jupiter" title="Rings of Jupiter">Rings</a></li> <li><a href="/wiki/Jupiter%27s_North_Pole" title="Jupiter's North Pole">Jupiter's North Pole</a></li> <li><a href="/wiki/Jupiter%27s_South_Pole" title="Jupiter's South Pole">Jupiter's South Pole</a></li></ul> </div></td><td class="noviewer navbox-image" rowspan="5" style="width:1px;padding:0 0 0 2px"><div><a href="/wiki/File:Portrait_of_Jupiter_from_Cassini.jpg" class="mw-file-description" title="NASA image of Jupiter"><img alt="NASA image of Jupiter" src="//upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/100px-Portrait_of_Jupiter_from_Cassini.jpg" decoding="async" width="100" height="125" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/150px-Portrait_of_Jupiter_from_Cassini.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/75/Portrait_of_Jupiter_from_Cassini.jpg/200px-Portrait_of_Jupiter_from_Cassini.jpg 2x" data-file-width="1920" data-file-height="2400" /></a></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Moons_of_Jupiter" title="Moons of Jupiter">Moons</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th scope="row" class="navbox-group" style="width:1%">Inner</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Metis_(moon)" title="Metis (moon)">Metis</a></li> <li><a href="/wiki/Adrastea_(moon)" title="Adrastea (moon)">Adrastea</a></li> <li><a href="/wiki/Amalthea_(moon)" title="Amalthea (moon)">Amalthea</a></li> <li><a href="/wiki/Thebe_(moon)" title="Thebe (moon)">Thebe</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Galilean_moons" title="Galilean moons">Galilean</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Io_(moon)" title="Io (moon)">Io</a></li> <li><a href="/wiki/Europa_(moon)" title="Europa (moon)">Europa</a></li> <li><a href="/wiki/Ganymede_(moon)" title="Ganymede (moon)">Ganymede</a></li> <li><a href="/wiki/Callisto_(moon)" title="Callisto (moon)">Callisto</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Irregular</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Himalia_group" title="Himalia group">Himalia group</a></li> <li><a href="/wiki/Themisto_(moon)" title="Themisto (moon)">Themisto</a></li> <li><a href="/wiki/Carpo_(moon)" title="Carpo (moon)">Carpo</a> group</li> <li><a href="/wiki/Valetudo_(moon)" title="Valetudo (moon)">Valetudo</a></li> <li><a href="/wiki/Ananke_group" title="Ananke group">Ananke group</a></li> <li><a href="/wiki/Carme_group" title="Carme group">Carme group</a></li> <li><a href="/wiki/Pasiphae_group" title="Pasiphae group">Pasiphae group</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Astronomy</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th scope="row" class="navbox-group" style="width:1%">General</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/List_of_Jupiter-crossing_minor_planets" title="List of Jupiter-crossing minor planets">Jupiter-crossing minor planets</a></li> <li><a href="/wiki/Solar_eclipses_on_Jupiter" title="Solar eclipses on Jupiter">Solar eclipses</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Jupiter_trojan" title="Jupiter trojan">Trojans</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/List_of_Jupiter_trojans_(Greek_camp)" title="List of Jupiter trojans (Greek camp)">Greek camp</a></li> <li><a href="/wiki/List_of_Jupiter_trojans_(Trojan_camp)" title="List of Jupiter trojans (Trojan camp)">Trojan camp</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Impact_events_on_Jupiter" title="Impact events on Jupiter">Impacts</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Comet_Shoemaker%E2%80%93Levy_9" title="Comet Shoemaker–Levy 9">Comet Shoemaker–Levy 9</a></li> <li><a href="/wiki/2009_Jupiter_impact_event" title="2009 Jupiter impact event">2009 Jupiter impact event</a></li> <li><a href="/wiki/2010_Jupiter_impact_event" title="2010 Jupiter impact event">2010 Jupiter impact event</a></li> <li><a href="/wiki/2016_Jupiter_impact_event" title="2016 Jupiter impact event">2016 Jupiter impact event</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Exploration_of_Jupiter" title="Exploration of Jupiter">Exploration</a>, orbital missions</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th scope="row" class="navbox-group" style="width:1%">Current</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Juno_(spacecraft)" title="Juno (spacecraft)">Juno</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Past</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Cassini%E2%80%93Huygens" title="Cassini–Huygens">Cassini–Huygens</a></li> <li><a href="/wiki/Galileo_project" title="Galileo project">Galileo project</a> <ul><li><a href="/wiki/Galileo_(spacecraft)" title="Galileo (spacecraft)">Galileo</a></li></ul></li> <li><a href="/wiki/New_Horizons" title="New Horizons">New Horizons</a></li> <li><a href="/wiki/Pioneer_program" title="Pioneer program">Pioneer program</a> <ul><li><a href="/wiki/Pioneer_10" title="Pioneer 10">Pioneer 10</a></li> <li><a href="/wiki/Pioneer_11" title="Pioneer 11">Pioneer 11</a></li></ul></li> <li><a href="/wiki/Ulysses_(spacecraft)" title="Ulysses (spacecraft)">Ulysses</a></li> <li><a href="/wiki/Voyager_program" title="Voyager program">Voyager program</a> <ul><li><a href="/wiki/Voyager_1" title="Voyager 1">Voyager 1</a></li> <li><a href="/wiki/Voyager_2" title="Voyager 2">Voyager 2</a></li></ul></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Future</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Jupiter_Icy_Moons_Explorer" title="Jupiter Icy Moons Explorer">Jupiter Icy Moons Explorer</a> (2023, en route)</li> <li><a href="/wiki/Europa_Clipper" title="Europa Clipper">Europa Clipper</a> (2024, en route)</li> <li><a href="/wiki/Tianwen-4" title="Tianwen-4">Tianwen-4</a> (2029)</li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Proposed</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Laplace-P" title="Laplace-P">Laplace-P</a> (2023)</li> <li><a href="/wiki/Shensuo_(spacecraft)" title="Shensuo (spacecraft)">Shensuo</a> (2024)</li> <li><a href="/wiki/Io_Volcano_Observer" title="Io Volcano Observer">Io Volcano Observer</a> (2026)</li> <li><a href="/wiki/SMARA_(spacecraft)" title="SMARA (spacecraft)">SMARA</a> (2030)</li> <li><a href="/wiki/Enceladus_Orbilander" title="Enceladus Orbilander">Enceladus Orbilander</a> (2038)</li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">Related</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Jupiter_in_fiction" title="Jupiter in fiction">Fiction</a></li> <li><a href="/wiki/Jupiter_(mythology)" class="mw-redirect" title="Jupiter (mythology)">Mythology</a></li></ul> </div></td></tr><tr><td class="navbox-abovebelow" colspan="3"><div> <ul><li><img alt="" src="//upload.wikimedia.org/wikipedia/en/thumb/9/96/Symbol_category_class.svg/16px-Symbol_category_class.svg.png" decoding="async" width="16" height="16" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/en/thumb/9/96/Symbol_category_class.svg/23px-Symbol_category_class.svg.png 1.5x, //upload.wikimedia.org/wikipedia/en/thumb/9/96/Symbol_category_class.svg/31px-Symbol_category_class.svg.png 2x" data-file-width="180" data-file-height="185" /> <a href="/wiki/Category:Jupiter" title="Category:Jupiter">Category</a></li> <li><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/22px-Solar_system.jpg" decoding="async" width="22" height="28" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/34px-Solar_system.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/Solar_system.jpg/45px-Solar_system.jpg 2x" data-file-width="4500" data-file-height="5600" /> <a href="/wiki/Portal:Solar_System" title="Portal:Solar System">Solar System portal</a></li></ul> </div></td></tr></tbody></table></div> <div class="navbox-styles"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1129693374"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1236075235"></div><div role="navigation" class="navbox" aria-labelledby="Atmospheres" style="padding:3px"><table class="nowraplinks hlist mw-collapsible autocollapse navbox-inner" style="border-spacing:0;background:transparent;color:inherit"><tbody><tr><th scope="col" class="navbox-title" colspan="3" style="text-align: center;"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1129693374"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1239400231"><div class="navbar plainlinks hlist navbar-mini"><ul><li class="nv-view"><a href="/wiki/Template:Atmospheres" title="Template:Atmospheres"><abbr title="View this template">v</abbr></a></li><li class="nv-talk"><a href="/wiki/Template_talk:Atmospheres" title="Template talk:Atmospheres"><abbr title="Discuss this template">t</abbr></a></li><li class="nv-edit"><a href="/wiki/Special:EditPage/Template:Atmospheres" title="Special:EditPage/Template:Atmospheres"><abbr title="Edit this template">e</abbr></a></li></ul></div><div id="Atmospheres" style="font-size:114%;margin:0 4em"><a href="/wiki/Atmosphere" title="Atmosphere">Atmospheres</a></div></th></tr><tr><th scope="row" class="navbox-group" style="text-align: center;;width:1%"><a href="/wiki/Star" title="Star">Stars</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Stellar_atmosphere" title="Stellar atmosphere">Sun</a></li></ul> </div></td><td class="noviewer navbox-image" rowspan="6" style="width:1px;padding:0 0 0 2px"><div><a href="/wiki/File:Chaotic_Clouds_of_Jupiter.jpg" class="mw-file-description" title="The violent storms of Jupiter's atmosphere"><img alt="The violent storms of Jupiter's atmosphere" src="//upload.wikimedia.org/wikipedia/commons/thumb/d/dc/Chaotic_Clouds_of_Jupiter.jpg/150px-Chaotic_Clouds_of_Jupiter.jpg" decoding="async" width="150" height="150" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/dc/Chaotic_Clouds_of_Jupiter.jpg/225px-Chaotic_Clouds_of_Jupiter.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/dc/Chaotic_Clouds_of_Jupiter.jpg/300px-Chaotic_Clouds_of_Jupiter.jpg 2x" data-file-width="1080" data-file-height="1080" /></a></div></td></tr><tr><th scope="row" class="navbox-group" style="text-align: center;;width:1%"><a href="/wiki/Planet" title="Planet">Planets</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Atmosphere_of_Mercury" title="Atmosphere of Mercury">Mercury</a></li> <li><a href="/wiki/Atmosphere_of_Venus" title="Atmosphere of Venus">Venus</a></li> <li><a href="/wiki/Atmosphere_of_Earth" title="Atmosphere of Earth">Earth</a></li> <li><a href="/wiki/Atmosphere_of_Mars" title="Atmosphere of Mars">Mars</a></li> <li><a class="mw-selflink selflink">Jupiter</a></li> <li><a href="/wiki/Saturn#Atmosphere" title="Saturn">Saturn</a></li> <li><a href="/wiki/Atmosphere_of_Uranus" title="Atmosphere of Uranus">Uranus</a></li> <li><a href="/wiki/Neptune#Atmosphere" title="Neptune">Neptune</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="text-align: center;;width:1%"><a href="/wiki/Dwarf_planet" title="Dwarf planet">Dwarf planets</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Ceres_(dwarf_planet)#Atmosphere" title="Ceres (dwarf planet)">Ceres</a></li> <li><a href="/wiki/Atmosphere_of_Pluto" title="Atmosphere of Pluto">Pluto</a></li> <li><a href="/wiki/Makemake#Atmosphere" title="Makemake">Makemake</a></li> <li><a href="/wiki/Eris_(dwarf_planet)#Surface_and_atmosphere" title="Eris (dwarf planet)">Eris</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="text-align: center;;width:1%"><a href="/wiki/Natural_satellite" title="Natural satellite">Natural satellites</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Atmosphere_of_the_Moon" title="Atmosphere of the Moon">Moon</a></li> <li><a href="/wiki/Atmosphere_of_Io" title="Atmosphere of Io">Io</a></li> <li><a href="/wiki/Europa_(moon)#Atmosphere" title="Europa (moon)">Europa</a></li> <li><a href="/wiki/Ganymede_(moon)#Atmosphere_and_ionosphere" title="Ganymede (moon)">Ganymede</a></li> <li><a href="/wiki/Callisto_(moon)#Atmosphere_and_ionosphere" title="Callisto (moon)">Callisto</a></li> <li><a href="/wiki/Enceladus#Atmosphere" title="Enceladus">Enceladus</a></li> <li><a href="/wiki/Dione_(moon)#Atmosphere" title="Dione (moon)">Dione</a></li> <li><a href="/wiki/Rhea_(moon)#Atmosphere" title="Rhea (moon)">Rhea</a></li> <li><a href="/wiki/Atmosphere_of_Titan" title="Atmosphere of Titan">Titan</a></li> <li><a href="/wiki/Atmosphere_of_Triton" title="Atmosphere of Triton">Triton</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="text-align: center;;width:1%"><a href="/wiki/Exoplanet" title="Exoplanet">Exoplanets</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/GJ_1132_b#Atmosphere" title="GJ 1132 b">GJ 1132 b</a></li> <li><a href="/wiki/HD_209458_b#Stratosphere_and_upper_clouds" title="HD 209458 b">HD 209458 b</a></li> <li><a href="/wiki/Kepler-7b#Cloud_mapping" title="Kepler-7b">Kepler-7b</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="text-align: center;;width:1%">See also</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Prebiotic_atmosphere" title="Prebiotic atmosphere">Prebiotic atmosphere</a></li> <li><a href="/wiki/Coma_(cometary)" class="mw-redirect" title="Coma (cometary)">Coma</a></li> <li><a href="/wiki/Extraterrestrial_atmosphere" title="Extraterrestrial atmosphere">Extraterrestrial atmosphere</a></li> <li><a href="/wiki/Stellar_atmosphere" title="Stellar atmosphere">Stellar atmosphere</a></li></ul> </div></td></tr><tr><td class="navbox-abovebelow" colspan="3" style="text-align: center;"><div>Atmospheres in boldface are significant atmospheres; atmospheres in italics are unconfirmed atmospheres.</div></td></tr></tbody></table></div> <div class="navbox-styles"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1129693374"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1236075235"></div><div role="navigation" class="navbox authority-control" aria-label="Navbox" style="padding:3px"><table class="nowraplinks hlist navbox-inner" style="border-spacing:0;background:transparent;color:inherit"><tbody><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Help:Authority_control" title="Help:Authority control">Authority control databases</a>: National <a href="https://www.wikidata.org/wiki/Q3045#identifiers" title="Edit this at Wikidata"><img alt="Edit this at Wikidata" src="//upload.wikimedia.org/wikipedia/en/thumb/8/8a/OOjs_UI_icon_edit-ltr-progressive.svg/10px-OOjs_UI_icon_edit-ltr-progressive.svg.png" 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[\"CITEREFBusse1976\"] = 1,\n [\"CITEREFChang2017\"] = 1,\n [\"CITEREFCheng_LiAndrew_P._IngersollAlexandra_P._KlipfelHarriet_Brettle2020\"] = 1,\n [\"CITEREFDuerGavrielGalantiKaspi2021\"] = 1,\n [\"CITEREFEncrenaz2003\"] = 1,\n [\"CITEREFFletcherKaspiGuillotShowman2020\"] = 1,\n [\"CITEREFFountain2008\"] = 1,\n [\"CITEREFGalantiKaspiDuerFletcher2021\"] = 1,\n [\"CITEREFGavrielKaspi2021\"] = 2,\n [\"CITEREFGavrielKaspi2022\"] = 2,\n [\"CITEREFGilesGreathouseBonfondGladstone2020\"] = 1,\n [\"CITEREFGrassiAdrianiMoriconiMura2018\"] = 1,\n [\"CITEREFHarringtonWeaverVillard2014\"] = 1,\n [\"CITEREFIngersollGieraschBanfieldVasavada2000\"] = 1,\n [\"CITEREFJames_R._Holton2004\"] = 1,\n [\"CITEREFJanssenOswaldBrownGulkis2017\"] = 1,\n [\"CITEREFKaspiGalantiHubbardStevenson2018\"] = 1,\n [\"CITEREFLiIngersollKlipfelBrettle2020\"] = 1,\n [\"CITEREFLiuSchneider2010\"] = 1,\n [\"CITEREFLoefferHudson2018\"] = 1,\n [\"CITEREFMcDowell1995\"] = 1,\n [\"CITEREFMichaud2006\"] = 1,\n [\"CITEREFMiller1953\"] = 1,\n [\"CITEREFMiller_Aylward_et_al.2005\"] = 1,\n [\"CITEREFMuraAdrianiBraccoMoriconi2021\"] = 1,\n [\"CITEREFMuraScaricaGrassiAdriani2022\"] = 2,\n [\"CITEREFNancy_Atkinson2010\"] = 1,\n [\"CITEREFO\u0026#039;NeillEmanuelFlierl2015\"] = 1,\n [\"CITEREFPearl_Conrath_et_al.1990\"] = 1,\n [\"CITEREFPeek1981\"] = 1,\n [\"CITEREFPhillips,_Tony2006\"] = 1,\n [\"CITEREFPhillips2003\"] = 1,\n [\"CITEREFPhillips2006\"] = 1,\n [\"CITEREFRogers,_John_H.2008\"] = 1,\n [\"CITEREFRogers1995\"] = 1,\n [\"CITEREFRogers2006\"] = 1,\n [\"CITEREFRogersEichstädtHansenOrton2021\"] = 1,\n [\"CITEREFSanders2010\"] = 1,\n [\"CITEREFScott2010\"] = 1,\n [\"CITEREFShiga2008\"] = 1,\n [\"CITEREFShowmande_Pater2005\"] = 1,\n [\"CITEREFSmithSoderblomJohnsonIngersoll1979\"] = 1,\n [\"CITEREFStaff2007\"] = 1,\n [\"CITEREFSteigerwald,_Bill2006\"] = 1,\n [\"CITEREFTabataba-VakiliRogersEichstädtOrton2020\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.1975\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.1978\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.1985\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.1996\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.1997\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.2002\"] = 1,\n [\"CITEREFWilliams,_Gareth_P.2003\"] = 4,\n [\"CITEREFWilliams,_Gareth_P.2006\"] = 1,\n [\"CITEREFYang2004\"] = 1,\n [\"CITEREFYoussef,_AshrafMarcus,_Philip_S.2003\"] = 1,\n [\"Fletcher2010\"] = 1,\n [\"Go\"] = 1,\n [\"Graney\"] = 1,\n [\"Guillot\"] = 1,\n [\"Hammel\"] = 1,\n [\"Heimpel2005\"] = 1,\n [\"Hockey1999\"] = 1,\n [\"Ingersoll\"] = 1,\n [\"Ingersoll1969\"] = 1,\n [\"Irwin2003\"] = 1,\n [\"Kunde\"] = 1,\n [\"Low\"] = 1,\n [\"McKim\"] = 1,\n [\"Noll1995\"] = 1,\n [\"Reese\"] = 1,\n [\"Ridpath\"] = 1,\n [\"Rogers\"] = 1,\n [\"Rogers2001\"] = 1,\n [\"Rogers2003\"] = 1,\n [\"Rogers2008b\"] = 1,\n [\"Sanchez2001\"] = 1,\n [\"Sanchez2008\"] = 1,\n [\"Sieff\"] = 1,\n [\"Smith\"] = 1,\n [\"Stone\"] = 1,\n [\"Vasavada\"] = 1,\n [\"West\"] = 1,\n [\"Yelle\"] = 1,\n}\ntemplate_list = table#1 {\n [\"Atmospheres\"] = 1,\n [\"Authority control\"] = 1,\n [\"Chem\"] = 2,\n [\"Cite book\"] = 11,\n [\"Cite encyclopedia\"] = 2,\n [\"Cite journal\"] = 73,\n [\"Cite news\"] = 4,\n [\"Cite web\"] = 19,\n [\"Clear\"] = 1,\n [\"Commons category\"] = 1,\n [\"Convert\"] = 1,\n [\"DEFAULTSORT:Atmosphere Of Jupiter\"] = 1,\n [\"E-sp\"] = 18,\n [\"Featured article\"] = 1,\n [\"Jupiter\"] = 1,\n [\"Main\"] = 2,\n [\"Multiple image\"] = 1,\n [\"Note label\"] = 4,\n [\"Nowrap\"] = 10,\n [\"Portal\"] = 1,\n [\"Portal bar\"] = 1,\n [\"Ref label\"] = 4,\n [\"Refbegin\"] = 2,\n [\"Refend\"] = 3,\n [\"Reflist\"] = 1,\n [\"Sfn\"] = 36,\n [\"SfnRef\"] = 6,\n [\"Short description\"] = 1,\n [\"Webarchive\"] = 1,\n}\narticle_whitelist = table#1 {\n}\ntable#1 {\n}\n","limitreport-profile":[["?","220","22.0"],["MediaWiki\\Extension\\Scribunto\\Engines\\LuaSandbox\\LuaSandboxCallback::callParserFunction","220","22.0"],["dataWrapper 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