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ACP - Technical note

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Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/12985/2024/acp-24-12985-2024-avatar-web.png" data-width="600" data-height="398" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 25 Nov 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/12985/2024/">Technical note: High-resolution analyses of concentrations and sizes of refractory black carbon particles deposited in northwestern Greenland over the past 350 years – Part 1: Continuous flow analysis of the SIGMA-D ice core using the wide-range Single-Particle Soot Photometer and a high-efficiency nebulizer</a> <div class="authors">Kumiko Goto-Azuma, Remi Dallmayr, Yoshimi Ogawa-Tsukagawa, Nobuhiro Moteki, Tatsuhiro Mori, Sho Ohata, Yutaka Kondo, Makoto Koike, Motohiro Hirabayashi, Jun Ogata, Kyotaro Kitamura, Kenji Kawamura, Koji Fujita, Sumito Matoba, Naoko Nagatsuka, Akane Tsushima, Kaori Fukuda, and Teruo Aoki</div> <div class="citation">Atmos. Chem. Phys., 24, 12985&ndash;13000, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-12985-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-12985-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120372" data-show=".short_summary_120372" data-hide=".short_summary_button_120372" >Short summary</span> <div class="j-widget__max short_summary short_summary_120372" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We developed a continuous flow analysis system to analyze an ice core from northwestern Greenland and coupled it with an improved refractory black carbon (rBC) measurement technique. This allowed accurate high-resolution analyses of size distributions and concentrations of rBC particles with diameters of 70&thinsp;nm&ndash;4&thinsp;&mu;m for the past 350 years. Our results provide crucial insights into rBC's climatic effects. We also found previous ice core studies substantially underestimated rBC mass concentrations. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120372" data-show=".short_summary_button_120372">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/12985/2024/acp-24-12985-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/12985/2024/acp-24-12985-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/12985/2024/acp-24-12985-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="398" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-0 in-range paperList-discussion" data-diff="0"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 25 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2776/">Technical note: Reconstructing surface missing aerosol elemental carbon data in long-term series with ensemble learning</a> <div class="authors">Qingxiao Meng, Yunjiang Zhang, Sheng Zhong, Jie Fang, Lili Tang, Yongcai Rao, Minfeng Zhou, Jian Qiu, Xiaofeng Xu, Jean-Eudes Petit, Olivier Favez, and Xinlei Ge</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2776,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2776,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for ACP</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123166" data-show=".short_summary_123166" data-hide=".short_summary_button_123166" >Short summary</span> <div class="j-widget__max short_summary short_summary_123166" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We developed a new method to reconstruct missing elemental carbon (EC) data in four Chinese cities from 2013 to 2023. Using machine learning, we accurately filled data gaps and introduced a new approach to analyze EC trends. Our findings reveal a significant decline in EC due to stricter pollution controls, though this slowed after 2020. This study provides a versatile framework for addressing data gaps and supports strategies to reduce urban air pollution and its climate impacts. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123166" data-show=".short_summary_button_123166">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/11637/2024/acp-24-11637-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/11637/2024/acp-24-11637-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/11637/2024/acp-24-11637-2024-avatar-web.png" data-width="480" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 17 Oct 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/11637/2024/">Technical note: On the ice microphysics of isolated thunderstorms and non-thunderstorms in southern China – a radar polarimetric perspective</a> <div class="authors">Chuanhong Zhao, Yijun Zhang, Dong Zheng, Haoran Li, Sai Du, Xueyan Peng, Xiantong Liu, Pengguo Zhao, Jiafeng Zheng, and Juan Shi</div> <div class="citation">Atmos. Chem. Phys., 24, 11637&ndash;11651, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-11637-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-11637-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_119042" data-show=".short_summary_119042" data-hide=".short_summary_button_119042" >Short summary</span> <div class="j-widget__max short_summary short_summary_119042" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Understanding lightning activity is important for meteorology and atmospheric chemistry. However, the occurrence of lightning activity in clouds is uncertain. In this study, we quantified the difference between isolated thunderstorms and non-thunderstorms. We showed that lightning activity was more likely to occur with more graupel volume and/or riming. A deeper Z<sub>DR</sub> column was associated with lightning occurrence. This information can aid in a deeper understanding of lighting physics.</p> <div>&nbsp;</div> <div>&nbsp;</div> <div>&nbsp;</div> </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_119042" data-show=".short_summary_button_119042">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/11637/2024/acp-24-11637-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/11637/2024/acp-24-11637-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/11637/2024/acp-24-11637-2024-avatar-web.png" data-width="480" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="600" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/10965/2024/acp-24-10965-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/10965/2024/acp-24-10965-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/10965/2024/acp-24-10965-2024-avatar-web.png" data-width="527" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 27 Sep 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/10965/2024/">Technical note: Nighttime OH and HO<sub>2</sub> chemical equilibria in the mesosphere–lower thermosphere</a> <div class="authors">Mikhail Yu. Kulikov, Mikhail V. Belikovich, Aleksey G. Chubarov, Svetlana O. Dementyeva, and Alexander M. Feigin</div> <div class="citation">Atmos. Chem. Phys., 24, 10965&ndash;10983, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-10965-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-10965-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118478" data-show=".short_summary_118478" data-hide=".short_summary_button_118478" >Short summary</span> <div class="j-widget__max short_summary short_summary_118478" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The assumption of chemical equilibrium is widely used to derive information about poorly measured characteristics of the mesosphere&ndash;lower thermosphere from rocket and satellite data and to study the physicochemical processes at these altitudes. In this work, we analyze the fundamental aspects of chemical equilibria of two important trace gases and discuss their possible applications. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118478" data-show=".short_summary_button_118478">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/10965/2024/acp-24-10965-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/10965/2024/acp-24-10965-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/10965/2024/acp-24-10965-2024-avatar-web.png" data-width="527" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="600" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-3 in-range paperList-discussion" data-diff="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 12 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2782/">Technical Note: Recommendations for Diagnosing Cloud Feedbacks and Rapid Cloud Adjustments Using Cloud Radiative Kernels</a> <div class="authors">Mark Zelinka, Li-Wei Chao, Timothy Myers, Yi Qin, and Stephen Klein</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2782,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2782,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for ACP</span> <nobr>(discussion: final response, 3 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123192" data-show=".short_summary_123192" data-hide=".short_summary_button_123192" >Short summary</span> <div class="j-widget__max short_summary short_summary_123192" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Clouds lie at the heart of uncertainty in both climate sensitivity and radiative forcing, making it imperative to properly diagnose their radiative effects. Here we provide a recommended methodology and code base for the community to use in performing such diagnoses using cloud radiative kernels. We show that properly accounting for changes in obscuration of lower-level clouds by upper-level is important for accurate diagnosis and attribution of cloud feedbacks and adjustments. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123192" data-show=".short_summary_button_123192">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div> <div class="grid-container paperlist-object type-1 in-range paperList-discussion" data-diff="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 09 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2596/">Technical note: A comparative study of chemistry schemes for volcanic sulfur dioxide in Lagrangian transport simulations: a case study of the 2019 Raikoke eruption</a> <div class="authors">Mingzhao Liu, Lars Hoffmann, Jens-Uwe Grooß, Zhongyin Cai, Sabine Grießbach, and Yi Heng</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2596,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2596,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for ACP</span> <nobr>(discussion: final response, 2 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122629" data-show=".short_summary_122629" data-hide=".short_summary_button_122629" >Short summary</span> <div class="j-widget__max short_summary short_summary_122629" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We studied the transport and chemical decomposition of volcanic SO<sub>2</sub>, focusing on the 2019 Raikoke event. By comparing two different chemistry modeling schemes, we found that including complex chemical reactions leads to a more accurate prediction of how long SO<sub>2</sub> stays in the atmosphere. This research helps improve our understanding of volcanic pollution and its impact on air quality and climate, providing better tools for scientists to track and predict the movement of these pollutants. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122629" data-show=".short_summary_button_122629">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/9475/2024/acp-24-9475-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/9475/2024/acp-24-9475-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/9475/2024/acp-24-9475-2024-avatar-web.png" data-width="600" data-height="583" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 29 Aug 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/9475/2024/">Technical note: Evaluation of the Copernicus Atmosphere Monitoring Service Cy48R1 upgrade of June 2023</a> <div class="authors">Henk Eskes, Athanasios Tsikerdekis, Melanie Ades, Mihai Alexe, Anna Carlin Benedictow, Yasmine Bennouna, Lewis Blake, Idir Bouarar, Simon Chabrillat, Richard Engelen, Quentin Errera, Johannes Flemming, Sebastien Garrigues, Jan Griesfeller, Vincent Huijnen, Luka Ilić, Antje Inness, John Kapsomenakis, Zak Kipling, Bavo Langerock, Augustin Mortier, Mark Parrington, Isabelle Pison, Mikko Pitkänen, Samuel Remy, Andreas Richter, Anja Schoenhardt, Michael Schulz, Valerie Thouret, Thorsten Warneke, Christos Zerefos, and Vincent-Henri Peuch</div> <div class="citation">Atmos. Chem. Phys., 24, 9475&ndash;9514, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-9475-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-9475-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_117246" data-show=".short_summary_117246" data-hide=".short_summary_button_117246" >Short summary</span> <div class="j-widget__max short_summary short_summary_117246" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The Copernicus Atmosphere Monitoring Service (CAMS) provides global analyses and forecasts of aerosols and trace gases in the atmosphere. On 27 June 2023 a major upgrade, Cy48R1, became operational. Comparisons with in situ, surface remote sensing, aircraft, and balloon and satellite observations show that the new CAMS system is a significant improvement. The results quantify the skill of CAMS to forecast impactful events, such as wildfires, dust storms and air pollution peaks. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_117246" data-show=".short_summary_button_117246">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/9475/2024/acp-24-9475-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/9475/2024/acp-24-9475-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/9475/2024/acp-24-9475-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="583" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/9419/2024/acp-24-9419-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/9419/2024/acp-24-9419-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/9419/2024/acp-24-9419-2024-avatar-web.png" data-width="600" data-height="192" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 28 Aug 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/9419/2024/">Technical note: Posterior uncertainty estimation via a Monte Carlo procedure specialized for 4D-Var data assimilation</a> <div class="authors">Michael Stanley, Mikael Kuusela, Brendan Byrne, and Junjie Liu</div> <div class="citation">Atmos. Chem. Phys., 24, 9419&ndash;9433, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-9419-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-9419-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115942" data-show=".short_summary_115942" data-hide=".short_summary_button_115942" >Short summary</span> <div class="j-widget__max short_summary short_summary_115942" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> To serve the uncertainty quantification (UQ) needs of 4D-Var data assimilation (DA) practitioners, we describe and justify a UQ algorithm from carbon flux inversion and incorporate its sampling uncertainty into the final reported UQ. The algorithm is mathematically proved, and its performance is shown for a carbon flux observing system simulation experiment. These results legitimize and generalize this algorithm's current use and make available this effective algorithm to new DA domains. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115942" data-show=".short_summary_button_115942">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/9419/2024/acp-24-9419-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/9419/2024/acp-24-9419-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/9419/2024/acp-24-9419-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="192" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-3 in-range paperList-discussion" data-diff="5"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 18 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1846/">Technical note: Towards atmospheric compound identification in chemical ionization mass spectrometry with machine learning</a> <div class="authors">Federica Bortolussi, Hilda Sandström, Fariba Partovi, Joona Mikkilä, Patrick Rinke, and Matti Rissanen</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1846,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1846,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for ACP</span> <nobr>(discussion: final response, 3 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121194" data-show=".short_summary_121194" data-hide=".short_summary_button_121194" >Short summary</span> <div class="j-widget__max short_summary short_summary_121194" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Chemical ionization mass spectrometry (CIMS) is widely used in atmospheric chemistry studies. We still have a limited understanding of the complex functioning of the instrument, therefore, we applied machine learning to provide insights from CIMS analyses. We were able to predict both detection and signal intensity with a fair error and we found out the most important structural fragments for negative ionization schemes (NH and OH) and positive ones (nitrogen-containing groups). </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121194" data-show=".short_summary_button_121194">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div> <div class="grid-container paperlist-object type-3 in-range paperList-discussion" data-diff="5"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 11 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1390/">Technical note: Quantified organic aerosol subsaturated hygroscopicity by a simple optical scatter monitor system through field measurements</a> <div class="authors">Jie Zhang, Tianyu Zhu, Alexandra Catena, Yaowei Li, Margaret Schwab, Pengfei Liu, Akua Asa-Awuku, and James Schwab</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1390,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1390,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for ACP</span> <nobr>(discussion: final response, 8 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120083" data-show=".short_summary_120083" data-hide=".short_summary_button_120083" >Short summary</span> <div class="j-widget__max short_summary short_summary_120083" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This study shows the derived organic aerosol hygroscopicity under high humidity conditions based on a simple optical scatter monitor system, including two nephelometric monitors (pDR-1500), after knowing the aerosol chemical composition. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120083" data-show=".short_summary_button_120083">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="5"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/7559/2024/acp-24-7559-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/7559/2024/acp-24-7559-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/7559/2024/acp-24-7559-2024-avatar-web.png" data-width="526" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 04 Jul 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/7559/2024/">Technical note: Retrieval of the supercooled liquid fraction in mixed-phase clouds from Himawari-8 observations</a> <div class="authors">Ziming Wang, Husi Letu, Huazhe Shang, and Luca Bugliaro</div> <div class="citation">Atmos. Chem. Phys., 24, 7559&ndash;7574, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-7559-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-7559-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115930" data-show=".short_summary_115930" data-hide=".short_summary_button_115930" >Short summary</span> <div class="j-widget__max short_summary short_summary_115930" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The supercooled liquid fraction (SLF) in mixed-phase clouds is retrieved for the first time using passive geostationary satellite observations based on differences in liquid droplet and ice particle radiative properties. The retrieved results are comparable to global distributions observed by active instruments, and the feasibility of the retrieval method to analyze the observed trends of the SLF has been validated. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115930" data-show=".short_summary_button_115930">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/7559/2024/acp-24-7559-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/7559/2024/acp-24-7559-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/7559/2024/acp-24-7559-2024-avatar-web.png" data-width="526" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="600" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="6"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/7001/2024/acp-24-7001-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/7001/2024/acp-24-7001-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/7001/2024/acp-24-7001-2024-avatar-web.png" data-width="600" data-height="278" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 18 Jun 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/7001/2024/">Technical note: Determining chemical composition of atmospheric single particles by a standard-free mass calibration algorithm</a> <div class="authors">Shao Shi, Jinghao Zhai, Xin Yang, Yechun Ruan, Yuanlong Huang, Xujian Chen, Antai Zhang, Jianhuai Ye, Guomao Zheng, Baohua Cai, Yaling Zeng, Yixiang Wang, Chunbo Xing, Yujie Zhang, Tzung-May Fu, Lei Zhu, Huizhong Shen, and Chen Wang</div> <div class="citation">Atmos. Chem. Phys., 24, 7001&ndash;7012, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-7001-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-7001-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115838" data-show=".short_summary_115838" data-hide=".short_summary_button_115838" >Short summary</span> <div class="j-widget__max short_summary short_summary_115838" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The determination of ions in the mass spectra of individual particles remains uncertain. We have developed a standard-free mass calibration algorithm applicable to more than 98&thinsp;% of ambient particles. With our algorithm, ions with ~&thinsp;0.05&thinsp;Th mass difference could be determined. Therefore, many more atmospheric species could be determined and involved in the source apportionment of aerosols, the study of chemical reaction mechanisms, and the analysis of single-particle mixing states. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115838" data-show=".short_summary_button_115838">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/7001/2024/acp-24-7001-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/7001/2024/acp-24-7001-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/7001/2024/acp-24-7001-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="278" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-3 in-range paperList-discussion" data-diff="6"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 17 Jun 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1516/">Technical note: Applicability of physics-based and machine-learning-based algorithms of geostationary satellite in retrieving the diurnal cycle of cloud base height</a> <div class="authors">Mengyuan Wang, Min Min, Jun Li, Han Lin, Yongen Liang, Binlong Chen, Zhigang Yao, Na Xu, and Miao Zhang</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1516,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1516,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for ACP</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120401" data-show=".short_summary_120401" data-hide=".short_summary_button_120401" >Short summary</span> <div class="j-widget__max short_summary short_summary_120401" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Although machine learning technology is advanced in the field of satellite remote sensing, the physical inversion algorithm based on cloud base height can better capture the daily variation characteristics of cloud base. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120401" data-show=".short_summary_button_120401">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="6"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/6583/2024/acp-24-6583-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/6583/2024/acp-24-6583-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://acp.copernicus.org/articles/24/6583/2024/acp-24-6583-2024-avatar-web.png" data-width="600" data-height="569" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 06 Jun 2024</div> <a class="article-title" target="_parent" href="https://acp.copernicus.org/articles/24/6583/2024/">Technical note: Influence of different averaging metrics and temporal resolutions on the aerosol pH calculated by thermodynamic modeling</a> <div class="authors">Haoqi Wang, Xiao Tian, Wanting Zhao, Jiacheng Li, Haoyu Yu, Yinchang Feng, and Shaojie Song</div> <div class="citation">Atmos. Chem. Phys., 24, 6583&ndash;6592, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/acp-24-6583-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/acp-24-6583-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118258" data-show=".short_summary_118258" data-hide=".short_summary_button_118258" >Short summary</span> <div class="j-widget__max short_summary short_summary_118258" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> pH is a key property of ambient aerosols, which affect many atmospheric processes. As aerosol pH is a non-conservative parameter, diverse averaging metrics and temporal resolutions may influence the pH values calculated by thermodynamic models. This technical note seeks to quantitatively evaluate the average pH using varied metrics and resolutions. The ultimate goal is to establish standardized reporting practices in future research endeavors. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118258" data-show=".short_summary_button_118258">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> <a class="paperlist-avatar" target="_blank" href="https://acp.copernicus.org/articles/24/6583/2024/acp-24-6583-2024-avatar-web.png"> <img class="img-responsive" src="https://acp.copernicus.org/articles/24/6583/2024/acp-24-6583-2024-avatar-thumb80.png" data-web="https://acp.copernicus.org/articles/24/6583/2024/acp-24-6583-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="569" width="80" height="80"> </a> </div> </div> <!-- Root element of PhotoSwipe. Must have class pswp. --> <div class="pswp" tabindex="-1" role="dialog" aria-hidden="true" > <!-- Background of PhotoSwipe. 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