SE - Research article

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Please try again later.</div> </div> </div> </div> </div>  <div class="modal " id="templateSearchLoadingModal" role="dialog" aria-labelledby="Search results" aria-hidden="true"> <div class="modal-dialog modal-sm modal-dialog-centered"> <div class="modal-content p-3 co_LoadingDotsContainer"> <div class="modal-body"> <div class="text">Searching</div> <div class="dots d-flex justify-content-center"><div class="dot"></div><div class="dot"></div><div class="dot"></div></div></div> </div> </div> </div> </div> <style> /*.modal {*/ /* background: rgba(255, 255, 255, 0.8);*/ /*}*/ .modal-header--sticky { position: sticky; top: 0; background-color: inherit; z-index: 1055; } .grid-container { margin-bottom: 1em; /*padding-left: 0;*/ /*padding-right: 0;*/ } #templateSearchInfo{ display: none; background-color: var(--background-color-primary); margin-top: 1px; z-index: 5; border: 1px solid var(--color-primary); opacity: .8; font-size: .7rem; border-radius: .25rem; } #templateSearchLoadingModal .co_LoadingDotsContainer { z-index: 1000; 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} #templateSearchResultTerm { font-weight: bold; } #resultsSearchHeader { display: block !important; } #scrolltopmodal { font-size: 3.0em; margin-top: 0 !important; margin-right: 15px; } @-webkit-keyframes animation_dots_breath { 50% { -webkit-transform: scale(1); transform: scale(1); opacity: 1; } 100% { opacity: 0; } } @keyframes animation_dots_breath { 50% { -webkit-transform: scale(1); transform: scale(1); opacity: 1; } 100% { opacity: 0; } } @media (min-width: 768px) and (max-width: 991px) { #templateSearchResultModal .modal-dialog { max-width: 90%; } } </style> <script> if(document.querySelector('meta[name="global_moBaseURL"]').content == "https://meetingorganizer.copernicus.org/") FINDER_URL = document.querySelector('meta[name="global_moBaseURL"]').content.replace('meetingorganizer', 'finder-app')+"search/library.php"; else FINDER_URL = document.querySelector('meta[name="global_moBaseURL"]').content.replace('meetingorganizer', 'finder')+"search/library.php"; SEARCH_INPUT = document.getElementById('search_query_solr'); SEARCH_INPUT_MODAL = document.getElementById('search_query_modal'); searchRunning = false; offset = 20; INITIAL_OFFSET = 20; var MutationObserver = window.MutationObserver || window.WebKitMutationObserver || window.MozMutationObserver; const targetNodeSearchModal = document.getElementById("templateSearchResultModal"); const configSearchModal = { attributes: true, childList: true, subtree: true }; // Callback function to execute when mutations are observed const callbackSearchModal = (mutationList, observer) => { for (const mutation of mutationList) { if (mutation.type === "childList") { // console.log("A child node has been added or removed."); picturesGallery(); } else if (mutation.type === "attributes") { // console.log(`The ${mutation.attributeName} attribute was modified.`); } } }; // Create an observer instance linked to the callback function const observer = new MutationObserver(callbackSearchModal); // Start observing the target node for configured mutations observer.observe(targetNodeSearchModal, configSearchModal); function _addEventListener() { document.getElementById('search_query_solr').addEventListener('keypress', (e) => { if (e.key === 'Enter') _runSearch(); }); document.getElementById('start_site_search_solr').addEventListener('click', (e) => { _runSearch(); e.stopPropagation(); e.stopImmediatePropagation(); return false; }); $('#templateSearchResultModal').scroll(function() { if ($(this).scrollTop()) { $('#scrolltopmodal:hidden').stop(true, true).fadeIn().css("display","inline-block"); } else { $('#scrolltopmodal').stop(true, true).fadeOut(); } }); } function scrollModalTop() { $('#templateSearchResultModal').animate({ scrollTop: 0 }, 'slow'); // $('#templateSearchResultModal').scrollTop(0); } function picturesGallery() { $('body').off('click', '.paperlist-avatar img'); $('body').off('click', '#templateSearchResultContainer .paperlist-avatar img'); searchPaperListAvatar = []; searchPaperListAvatarThumb = []; search_pswpElement = document.querySelectorAll('.pswp')[0]; if (typeof search_gallery != "undefined") { search_gallery = null; } $('body').on('click', '#templateSearchResultContainer .paperlist-avatar img', function (e) { if(searchPaperListAvatarThumb.length === 0 && searchPaperListAvatar.length === 0) { $('#templateSearchResultContainer .paperlist-avatar img').each(function () { var webversion = $(this).attr('data-web'); var width = $(this).attr('data-width'); var height = $(this).attr('data-height'); var caption = $(this).attr('data-caption'); var figure = { src: webversion, w: width, h: height, title: caption }; searchPaperListAvatarThumb.push($(this)[0]); searchPaperListAvatar.push(figure); }); } var target = $(this); var index = $('#templateSearchResultContainer .paperlist-avatar img').index(target); var options = { showHideOpacity:false, bgOpacity:0.8, index:index, spacing:0.15, history: false, focus:false, getThumbBoundsFn: function(index) { var thumbnail = searchPaperListAvatarThumb[index]; var pageYScroll = window.pageYOffset || document.documentElement.scrollTop; var rect = thumbnail.getBoundingClientRect(); return {x:rect.left, y:rect.top + pageYScroll, w:rect.width}; } }; search_gallery = new PhotoSwipe( search_pswpElement, PhotoSwipeUI_Default,[searchPaperListAvatar[index]],options); search_gallery.init(); }); } function showError(code, msg) { console.error(code, msg); $("#templateSearchLoadingModal").modal("hide"); switch(code) { case -3: // http request fail case -2: // invalid MO response case 4: // CORS case 1: // project $("#templateSearchErrorModal1").modal({}); break; case -1: // timeout $("#templateSearchErrorModal2").modal({}); break; case 2: // empty term $("#templateSearchErrorModal3").modal({}); break; case 3: // DOS $("#templateSearchErrorModal4").modal({}); break; default: $("#templateSearchErrorModal1").modal({}); break; } } function clearForm() { var myFormElement = document.getElementById("library-filters") var elements = myFormElement.elements; $(".form-check-input").prop('checked', false).change().parent().removeClass('active'); for(i=0; i<elements.length; i++) { field_type = elements[i].type.toLowerCase(); switch(field_type) { case "text": case "password": case "textarea": case "hidden": elements[i].value = ""; break; case "radio": case "checkbox": if (elements[i].checked) { elements[i].checked = false; } break; case "select-one": case "select-multi": elements[i].selectedIndex = -1; break; default: break; } } } function generateShowMoreButton(offset, term) { var code = '<button aria-label="ShowMore" id="showMore" class="btn btn-success float-right mr-2" data-offset="' + offset + '">Show more</button>'; return code; } function hideModal(id) { $("#"+id).modal('hide'); } function showModal(id) { $("#"+id).modal({}); } function prepareForPhotoSwipe() { searchPaperListAvatar = []; searchPaperListAvatarThumb = []; search_pswpElement = document.querySelectorAll('.pswp')[0]; } function _sendAjax(projectID, term) { let httpRequest = new XMLHttpRequest(); if(searchRunning) { console.log("Search running"); return; } if (!httpRequest) { console.error("Giving up :( Cannot create an XMLHTTP instance"); showError(-1); return false; } // httpRequest.timeout = 20000; // time in milliseconds httpRequest.withCredentials = false; httpRequest.ontimeout = (e) => { showError(-1, "result timeout"); searchRunning = false; }; httpRequest.onreadystatechange = function() { if (httpRequest.readyState === XMLHttpRequest.DONE) { searchRunning = false; if (httpRequest.status === 200) { let rs = JSON.parse(httpRequest.responseText); if(rs) { if(rs.isError) { showError(rs.errorCode, rs.errorMessage); } else { let html = rs.resultHTMLs; $("#modal_search_query").val(rs.term); $("#templateSearchResultTerm").html(rs.term); $("#templateSearchResultNr").html(rs.resultsNr); $("#templateRefineSearch").html(rs.filter); if(rs.filter == false) { console.log('filter empty'); $("#refineSearchModal").removeClass('d-block').addClass('d-none'); } if(rs.resultsNr==1) $("#templateSearchResultNrPlural").hide(); else $("#templateSearchResultNrPlural").show(); if(rs.resultsNr==0) { hideModal('templateSearchLoadingModal'); $("#templateSearchResultContainer").html(""); $("#templateSearchResultContainerEmpty").removeClass("d-none"); showModal('templateSearchResultModal'); } else { if((rs.resultsNr - offset)>0) { html = html + generateShowMoreButton(offset, term); } $("#templateSearchResultContainerEmpty").addClass("d-none"); if( offset == INITIAL_OFFSET) { hideModal('templateSearchLoadingModal'); $("#templateSearchResultContainer").html(html); showModal('templateSearchResultModal'); } else { $('#showMore').remove(); startHtml = $("#templateSearchResultContainer").html(); $("#templateSearchResultContainer").html(startHtml + html); } // prepareForPhotoSwipe(); } } } else { showError(-2, "invalid result"); } } else { showError(-3, "There was a problem with the request."); } } }; if(offset == INITIAL_OFFSET) { hideModal('templateSearchResultModal'); showModal('templateSearchLoadingModal'); } httpRequest.open("GET", FINDER_URL+"?project="+projectID+"&term="+encodeURI(term)+((offset>INITIAL_OFFSET)?("&offset="+(offset-INITIAL_OFFSET)) : "")); httpRequest.send(); 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var queryString = $('#library-filters').serialize(); var term = _searchTrimInput($('#modal_search_query').val()); term+='&'+queryString; if(term.length > 0) { _sendAjax(projectID, term); } else { showError(2, 'Empty search term') } } if(document.getElementById('search_query_solr')) { run(); } </script> </div></div> </div> </div> </div> </div> </header>  <main class="one-column version-2023"> <div id="content" class="container"> <div id="page_content_container" class="CMSCONTAINER row"> <div class="col"> <div class="level2Toc"> <div class="grid-container no-margin"> <div class="grid-100"> <h1>Research article</h1> </div> </div> <div class="row no-gutters auto-fixed-top-forced"> <div class="col-12 hide-on-fixed"> <div class="grid-container show-js paperList-filter" style="display: none;"> <div class="grid-100"> <form class="radio" autocomplete="off"> <div class="row no-gutters"> <div class="col-auto mr-2"> <label> <input type="radio" class="show-hide" name="paperListFilter" checked="checked" value="all" data-bubble="true" data-show=".paperList-final,.paperList-discussion"> All papers </label> </div> <div class="col-auto mr-2"> <label> <input type="radio" class="show-hide" name="paperListFilter" value="final" data-bubble="true" data-show=".paperList-final" data-hide=".paperList-discussion"> Final revised papers only </label> </div> <div class="col-auto mr-2"> <label> <input type="radio" class="show-hide" name="paperListFilter" value="discussion" data-bubble="true" data-show=".paperList-discussion" data-hide=".paperList-final"> Preprints only </label> </div> </div> </form> </div> </div> </div> <div class="col-12 pb-3 show-on-fixed recent-selection-wrapper" style="display:none;"> <button type="button" class="btn btn-primary">Filters</button> </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"> 21 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3238/">Thermodynamically admissible derivation of Biot's poroelastic equations and Gassmann's equations from conservation laws</a> <div class="authors">Yury Alkhimenkov and Yury Y. Podladchikov</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3238,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3238,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_124077" data-show=".short_summary_124077" data-hide=".short_summary_button_124077" >Short summary</span> <div class="j-widget__max short_summary short_summary_124077" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This paper presents a rigorous derivation of Gassmann's equations, grounded in thermodynamic principles and conservation laws, addressing gaps and potential inconsistencies in the original formulation. It also explores Biot's poroelastic equations, demonstrating that Gassmann's equations are a specific case within Biot’s framework. The study affirms the robustness of Gassmann's equations when assumptions are met, and symbolic Maple routines are provided to ensure reproducibility of the results. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_124077" data-show=".short_summary_button_124077">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-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"> 20 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3448/">Multiphysics property prediction from hyperspectral drill core data</a> <div class="authors">Akshay Kamath, Samuel Thiele, Moritz Kirsch, and Richard Gloaguen</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3448,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3448,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_124713" data-show=".short_summary_124713" data-hide=".short_summary_button_124713" >Short summary</span> <div class="j-widget__max short_summary short_summary_124713" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We developed a deep learning model that uses hyperspectral imaging data to predict key physical rock properties, specifically density, slowness, and gamma-ray values. Our model successfully learned to translate hyperspectral information into predicted physical properties. Tests on independent data gave accurate results, demonstrating the potential of hyperspectral data for mapping physical rock properties. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_124713" data-show=".short_summary_button_124713">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-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"> 19 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3097/">What do the arc magmatism trace element patterns and Sr-Nd-Pb isotopic data reflect: Insight from the Urumieh-Dokhtar magmatic arc of Iran</a> <div class="authors">Mohammad Reza Ghorbani, Meysam Akbari, Ian T. Graham, Mathieu Benoit, and Fatemeh Sepidbar</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3097,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3097,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123791" data-show=".short_summary_123791" data-hide=".short_summary_button_123791" >Short summary</span> <div class="j-widget__max short_summary short_summary_123791" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Original geochemical data for the vast Cenozoic arc magmatism of Iran introduce three distinct rock series rooted in the mantle wedge. The LILE-rich and LILE-poor series show wet-slab melt metasomatism and dry-slab melt metasomatism signatures respectively. The third series rich in incompatible elements, ITE-rich, indicate the input of asthenosphere as well. Eocene-Early Miocene ages for the three series imply that the metasomatic events predate Eocene and the three series occur intermittently. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123791" data-show=".short_summary_button_123791">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-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"> 18 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3340/">The 3D <em>Q</em><sub>p</sub> Model of the China Seismic Experiment Site (CSES-<em>Q</em>1.0) and Its Tectonic Implications</a> <div class="authors">Mengqiao Duan, Lianqing Zhou, Ying Fu, Yanru An, Jingqiong Yang, and Xiaodong Zhang</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3340,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3340,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_124437" data-show=".short_summary_124437" data-hide=".short_summary_button_124437" >Short summary</span> <div class="j-widget__max short_summary short_summary_124437" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Local seismic tomography yields the highest-resolution 3D <em>Q</em><sub>p</sub> model in CSES. Low <em>Q</em><sub>p</sub> anomalies along faults and basins indicate high medium fragmentation, thick sediments, or fluid richness. Tengchong volcano's westward dipping high attenuation suggests magma flow. Most M6+ earthquakes occur in low attenuation zones or anomaly boundaries. The 2008 Wenchuan <em>M</em><sub>S</sub> 8.0 and 2013 Lushan <em>M</em><sub>S</sub> 7.0 epicenters were separated by a low attenuation area, indicating future major earthquake risks. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_124437" data-show=".short_summary_button_124437">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="0"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1343/2024/se-15-1343-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1343/2024/se-15-1343-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1343/2024/se-15-1343-2024-avatar-web.png" data-width="600" data-height="255" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 14 Nov 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1343/2024/">The protocataclasite dilemma: in situ <sup>36</sup>Cl and REE-Y lessons from an impure limestone fault scarp at Sparta, Greece</a> <div class="authors">Bradley W. Goodfellow, Marc W. Caffee, Greg Chmiel, Ruben Fritzon, Alasdair Skelton, and Arjen P. Stroeven</div> <div class="citation">Solid Earth, 15, 1343–1363, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1343-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1343-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_113172" data-show=".short_summary_113172" data-hide=".short_summary_button_113172" >Short summary</span> <div class="j-widget__max short_summary short_summary_113172" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Reconstructions of past earthquakes are useful to assess earthquake hazard risk. We assess a limestone scarp exposed by earthquakes along the Sparta Fault, Greece, using <sup>36</sup>Cl and rare-earth elements and yttrium (REE-Y). Our analyses indicate an increase in the average scarp slip rate from 0.8–0.9 mm yr<sup>-1</sup> at 6.5–7.7 kyr ago to 1.1–1.2 mm yr<sup>-1</sup> up to the devastating 464 BCE earthquake. REE-Y indicate clays in the fault scarp; their potential use in palaeoseismicity would benefit from further study. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_113172" data-show=".short_summary_button_113172">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://se.copernicus.org/articles/15/1343/2024/se-15-1343-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1343/2024/se-15-1343-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1343/2024/se-15-1343-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="255" 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"> 11 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3219/">Origin of Changbaishan volcano inferred from simulation of the Cenozoic Pacific plate subduction using geodynamic models with data assimilation</a> <div class="authors">Tao Zhu, Yingxing Guo, Yueyang Xia, and Chao Dong</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3219,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3219,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 1 comment)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_124042" data-show=".short_summary_124042" data-hide=".short_summary_button_124042" >Short summary</span> <div class="j-widget__max short_summary short_summary_124042" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Our simulation considers the Mesozoic subduction of the Izanagi slab, which plays an irreplaceable role in the formation of stagnant Pacific slab within the MTZ. The magmas of the Changbaishan volcano may primarily originate from the super-hydrous melts caused by the Pacific slab dehydration in the MTZ. The upward escape of the entrained oceanic asthenospheric material as well as the piling up and thickening of the subducted Pacific slab may play secondary roles. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_124042" data-show=".short_summary_button_124042">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="0"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1319/2024/se-15-1319-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1319/2024/se-15-1319-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1319/2024/se-15-1319-2024-avatar-web.png" data-width="600" data-height="266" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 06 Nov 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1319/2024/">On the role of trans-lithospheric faults in the long-term seismotectonic segmentation of active margins: a case study in the Andes</a> <div class="authors">Gonzalo Yanez C., Jose Piquer R., and Orlando Rivera H.</div> <div class="citation">Solid Earth, 15, 1319–1342, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1319-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1319-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_119897" data-show=".short_summary_119897" data-hide=".short_summary_button_119897" >Short summary</span> <div class="j-widget__max short_summary short_summary_119897" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We postulate that the observed spatial distribution of large earthquakes in active convergence zones, organised in segments where large events are repeated every 100–300 years, depends on large-scale continental faults and fluid release from the subducting slab. In order to support this model, we use proxies at different spatial and temporal scales (historic seismicity, megathrust slip solutions, inter-seismic cumulative seismicity, GPS/viscous plate coupling, and coastline morphology). </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_119897" data-show=".short_summary_button_119897">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://se.copernicus.org/articles/15/1319/2024/se-15-1319-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1319/2024/se-15-1319-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1319/2024/se-15-1319-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="266" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="0"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1303/2024/se-15-1303-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1303/2024/se-15-1303-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1303/2024/se-15-1303-2024-avatar-web.png" data-width="600" data-height="530" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 04 Nov 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1303/2024/">Coda-derived source properties estimated using local earthquakes in the Sea of Marmara, Türkiye</a> <div class="authors">Berkan Özkan, Tuna Eken, Peter Gaebler, and Tuncay Taymaz</div> <div class="citation">Solid Earth, 15, 1303–1317, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1303-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1303-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118713" data-show=".short_summary_118713" data-hide=".short_summary_button_118713" >Short summary</span> <div class="j-widget__max short_summary short_summary_118713" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This study estimates source properties by analyzing seismic data of 303 earthquakes (2018–2020) in the Marmara Region, Turkey, and finds a strong correlation between moment-derived coda magnitude (<em>M</em><sub>w-coda</sub>) and moment magnitude (<em>M</em><sub>L</sub>). Moreover, the scaled energy increases with seismic moment estimates and shows non-self-similar scaling in earthquake sources. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118713" data-show=".short_summary_button_118713">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://se.copernicus.org/articles/15/1303/2024/se-15-1303-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1303/2024/se-15-1303-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1303/2024/se-15-1303-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="530" 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"> 04 Nov 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3134/">Numerical Investigation of Parameters Influencing Back-Thrust Development in Outer Wedge Fronts of Fold-and-Thrust-Belt Systems</a> <div class="authors">Saeed Mahmoodpour, Florian Duschl, and Michael C. Drews</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3134,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3134,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123872" data-show=".short_summary_123872" data-hide=".short_summary_button_123872" >Short summary</span> <div class="j-widget__max short_summary short_summary_123872" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> In some situations where the crust plates collide to each other, they deform by creating folds and thrusts. Based on thrusts development direction, they are categorized into fore- or back-thrusts. We use numerical simulation to investigate their development over geological time-scales. We examine the importance of rock strength, friction, displacement type and geometry on back-thrusting with regard to the final geometry of the deformation, as well as the distribution of porosity and stresses. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123872" data-show=".short_summary_button_123872">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="0"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1265/2024/se-15-1265-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1265/2024/se-15-1265-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1265/2024/se-15-1265-2024-avatar-web.png" data-width="600" data-height="516" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 29 Oct 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1265/2024/">Along-strike variation in volcanic addition controlling post-breakup sedimentary infill: Pelotas margin, austral South Atlantic</a> <div class="authors">Marlise C. Cassel, Nick Kusznir, Gianreto Manatschal, and Daniel Sauter</div> <div class="citation">Solid Earth, 15, 1265–1279, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1265-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1265-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115797" data-show=".short_summary_115797" data-hide=".short_summary_button_115797" >Short summary</span> <div class="j-widget__max short_summary short_summary_115797" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We investigate the along-strike variation in volcanics on the Pelotas segment of the Brazilian margin created during continental breakup and formation of the southern South Atlantic.  We show that the volume of volcanics strongly controls the amount of space available for post-breakup sedimentation. We also show that breakup varies along-strike from very magma-rich to magma-normal within a relatively short distance of less than 300 km. This is not as expected from a simple mantle plume model. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115797" data-show=".short_summary_button_115797">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://se.copernicus.org/articles/15/1265/2024/se-15-1265-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1265/2024/se-15-1265-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1265/2024/se-15-1265-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="516" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object in-range paperList-final" data-diff="0"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1281/2024/se-15-1281-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1281/2024/se-15-1281-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1281/2024/se-15-1281-2024-avatar-web.png" data-width="600" data-height="371" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 29 Oct 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1281/2024/">Localized shear and distributed strain accumulation as competing shear accommodation mechanisms in crustal shear zones: constraining their dictating factors</a> <div class="authors">Pramit Chatterjee, Arnab Roy, and Nibir Mandal</div> <div class="citation">Solid Earth, 15, 1281–1301, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1281-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1281-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_119356" data-show=".short_summary_119356" data-hide=".short_summary_button_119356" >Short summary</span> <div class="j-widget__max short_summary short_summary_119356" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Understanding strain accumulation processes in shear zones is essential for explaining failure mechanisms at great crustal depths. This study explores the rheological and kinematic factors determining the varying modes of shear accommodation in natural shear zones. Numerical simulations suggest that an interplay of parameters – initial viscosity, bulk shear rate, and internal cohesion – governs the dominance of one accommodation mechanism over another. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_119356" data-show=".short_summary_button_119356">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://se.copernicus.org/articles/15/1281/2024/se-15-1281-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1281/2024/se-15-1281-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1281/2024/se-15-1281-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="371" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 21 Oct 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2100/">Silurian syn- and post-collision granitic magmatism in the western section of the North Qinling Orogen: Implications for collisional orogenic processes</a> <div class="authors">Hao Lin, Zuochen Li, Xianzhi Pei, Shaowei Zhao, Meng Wang, Hai Zhou, Feng Gao, Mao Wang, and Li Qin</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2100,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2100,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 2 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121763" data-show=".short_summary_121763" data-hide=".short_summary_button_121763" >Short summary</span> <div class="j-widget__max short_summary short_summary_121763" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> There is still considerable controversy over the duration of the subduction-collision orogeny process of the Wushan-Shangdan Ocean. Here, we present new geochronological and geochemical data for Silurian granites from the North Qinling Orogen. The main conclusions are as follows: (1) the ocean had closed prior to 438 Ma; (2) The transition phase from syn-collision to post-collision took place between 429 and 421 Ma; (3) A three-stage tectonic model of the Wushan-Shangdan Ocean is proposed. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121763" data-show=".short_summary_button_121763">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-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 16 Oct 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2483/">Elastic anisotropy differentiation of thin shale beds and fractures using a novel hybrid rock physics model</a> <div class="authors">Haoyuan Li, Xuri Huang, Limin Sa, Lei Li, Fang Li, and Tiansheng Chen</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2483,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2483,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122428" data-show=".short_summary_122428" data-hide=".short_summary_button_122428" >Short summary</span> <div class="j-widget__max short_summary short_summary_122428" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Our research aims to accurately differentiate the elastic properties of tight sands with thin shale beds and fractures. Traditional models struggle to distinguish between these two features. We developed a hybrid rock physics model. Our model's reliability is validated against well log data, revealing distinct anisotropic characteristics for thin shale beds and fractures. This model helps identify fractures more accurately, improving geophysical exploration. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122428" data-show=".short_summary_button_122428">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-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 14 Oct 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2932/">About the Trustworthiness of Physics-Based Machine Learning – A Considerations for Geomechanical Applications</a> <div class="authors">Denise Degen, Moritz Ziegler, Oliver Heidbach, Andreas Henk, Karsten Reiter, and Florian Wellmann</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2932,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2932,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 0 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123483" data-show=".short_summary_123483" data-hide=".short_summary_button_123483" >Short summary</span> <div class="j-widget__max short_summary short_summary_123483" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Obtaining reliable estimates of the subsurface state distributions is essential to determine the location of e.g. potential nuclear waste disposal sites. However, providing these is challenging since it requires solving the problem numerous times yielding high computational cost. To overcome this, we use a physics-based machine learning method to construct surrogate models. We demonstrate how it produces physics-preserving predictions, which differentiates it from purely data-driven approaches. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123483" data-show=".short_summary_button_123483">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-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 14 Oct 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-3116/">Strike-slip kinematics from crustal to outcrop-scale: the impact of the material properties on the analogue modelling</a> <div class="authors">Luigi Massaro, Jürgen Adam, Elham Jonade, Silvia Negrão, and Yasuhiro Yamada</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-3116,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-3116,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 1 comment)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123831" data-show=".short_summary_123831" data-hide=".short_summary_button_123831" >Short summary</span> <div class="j-widget__max short_summary short_summary_123831" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> In this manuscript, we investigated the kinematics and dynamics of strike-slip damage zones using laboratory mechanical tests and analogue modelling techniques. The results underline the importance of a multi-scale approach (from crustal to outcrop-scale) to improve the understanding of such deformation processes, deriving fundamental correlations with the physical and mechanical properties of the model materials applied in the experiments. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123831" data-show=".short_summary_button_123831">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="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 10 Oct 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2734/">Hydroxyl in eclogitic garnet, orthopyroxene and oriented inclusion-bearing clinopyroxene, W Norway</a> <div class="authors">Dirk Spengler, Monika Koch-Müller, Adam Włodek, Simon J. Cuthbert, and Jarosław Majka</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2734,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2734,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122950" data-show=".short_summary_122950" data-hide=".short_summary_button_122950" >Short summary</span> <div class="j-widget__max short_summary short_summary_122950" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> West Norwegian 'diamond facies' eclogite contains tiny mineral inclusions of quartz and amphibole lamellae that are not stable in the diamond field. Low trace amounts of water in the lamellae-bearing host minerals suggest that the inclusion microstructure was not formed by fluid infiltration but by dehydration during early exhumation of these rocks. Some samples with higher water content argue that a late fluid overprint was spatially restricted and obliterated evidence of extreme metamorphism. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122950" data-show=".short_summary_button_122950">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://se.copernicus.org/articles/15/1233/2024/se-15-1233-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1233/2024/se-15-1233-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1233/2024/se-15-1233-2024-avatar-web.png" data-width="366" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 02 Oct 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1233/2024/">Influence of water on crystallographic preferred orientation patterns in a naturally deformed quartzite</a> <div class="authors">Jeffrey M. Rahl, Brendan Moehringer, Kenneth S. Befus, and John S. Singleton</div> <div class="citation">Solid Earth, 15, 1233–1240, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1233-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1233-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120487" data-show=".short_summary_120487" data-hide=".short_summary_button_120487" >Short summary</span> <div class="j-widget__max short_summary short_summary_120487" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> At the high temperatures present in the deeper crust, minerals such as quartz can flow much like silly putty. The detailed mechanisms of how atoms are reorganized depends upon several factors, such as the temperature and the rate of which the mineral changes shape. We present observations from a naturally deformed rock showing that the amount of water present also influences the type of deformation in quartz, with implications for geological interpretations. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120487" data-show=".short_summary_button_120487">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://se.copernicus.org/articles/15/1233/2024/se-15-1233-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1233/2024/se-15-1233-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1233/2024/se-15-1233-2024-avatar-web.png" data-width="366" 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="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1203/2024/se-15-1203-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1203/2024/se-15-1203-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1203/2024/se-15-1203-2024-avatar-web.png" data-width="414" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 30 Sep 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1203/2024/">Geomorphic expressions of active rifting reflect the role of structural inheritance: a new model for the evolution of the Shanxi Rift, northern China</a> <div class="authors">Malte Froemchen, Ken J. W. McCaffrey, Mark B. Allen, Jeroen van Hunen, Thomas B. Phillips, and Yueren Xu</div> <div class="citation">Solid Earth, 15, 1203–1231, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1203-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1203-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115752" data-show=".short_summary_115752" data-hide=".short_summary_button_115752" >Short summary</span> <div class="j-widget__max short_summary short_summary_115752" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The Shanxi Rift is a young, active rift in northern China that formed atop a Proterozoic orogen. The impact of these structures on active rift faults is poorly understood. Here, we quantify the landscape response to active faulting and compare it with published maps of inherited structures. We find that inherited structures played an important role in the segmentation of the Shanxi Rift and in the development of rift interaction zones, which are the most active regions in the Shanxi Rift. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115752" data-show=".short_summary_button_115752">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://se.copernicus.org/articles/15/1203/2024/se-15-1203-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1203/2024/se-15-1203-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1203/2024/se-15-1203-2024-avatar-web.png" data-width="414" 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-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 30 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2818/">Unbiased statistical length analysis of linear features: Adapting survival analysis to geological applications</a> <div class="authors">Gabriele Benedetti, Stefano Casiraghi, Daniela Bertacchi, and Andrea Luigi Paolo Bistacchi</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2818,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2818,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 3 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123261" data-show=".short_summary_123261" data-hide=".short_summary_button_123261" >Short summary</span> <div class="j-widget__max short_summary short_summary_123261" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> At any scale, the limited size of a study area introduces a bias in the interpretation of linear features, defined as right-censoring bias. We show the effects of not considering such bias and apply survival analysis techniques to obtain unbiased estimates of multiple parametrical distributions in three censored length datasets. Finally, we propose a novel approach to select the most representative model from a sensible candidate pool using the Probability Integral Transform technique. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123261" data-show=".short_summary_button_123261">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-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 26 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2975/">The Size Distributions of Faults and Earthquakes: Implications for Orogen-Internal Seismogenic Deformation</a> <div class="authors">Sandro Truttmann, Tobias Diehl, Marco Herwegh, and Stefan Wiemer</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2975,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2975,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 1 comment)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123563" data-show=".short_summary_123563" data-hide=".short_summary_button_123563" >Short summary</span> <div class="j-widget__max short_summary short_summary_123563" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Our study investigates the statistical relationship between geological faults and earthquakes in the Southwestern Swiss Alps. We analyze how the fault size and earthquake rupture are related and find differences in how faults at different depths rupture seismically. While shallow faults tend to rupture only partially, deeper faults are more likely to rupture along their entire length, potentially resulting in larger earthquakes. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123563" data-show=".short_summary_button_123563">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-0 in-range paperList-discussion" data-diff="2"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 23 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2823/">Poro-perm relations of Mesozoic carbonates and fault breccia, Araxos Promontory, NW Greece</a> <div class="authors">Sergio C. Vinciguerra, Federico Vagnon, Irene Bottero, Jerome Fortin, Angela Vita Petrullo, Dimitrios Spanos, Aristotelis Pagoulatos, and Fabrizio Agosta</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2823,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2823,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 2 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_123272" data-show=".short_summary_123272" data-hide=".short_summary_button_123272" >Short summary</span> <div class="j-widget__max short_summary short_summary_123272" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We assessed the poro-perm relations of both host rocks and fault rocks of Mesozoic carbonate rocks, by integrating a laboratory petrophysical studyn with a digital image analysis. Three different protocols were employed to compute permeability: i) Effective Medium Theory on laboratory data, ii) constant crack aperture and iii) crack density values from 2D images. Carbonate host rocks did not show a clear poro-perm trend due to the presence of stiff, sub-rounded pores and of small vugs. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_123272" data-show=".short_summary_button_123272">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="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1185/2024/se-15-1185-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1185/2024/se-15-1185-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1185/2024/se-15-1185-2024-avatar-web.png" data-width="600" data-height="542" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 20 Sep 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1185/2024/">Basic chemical composition combination rules and quantitative criterion of red beds</a> <div class="authors">Guangjun Cui, Jin Liao, Linghua Kong, Cuiying Zhou, Zhen Liu, Lei Yu, and Lihai Zhang</div> <div class="citation">Solid Earth, 15, 1185–1201, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1185-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1185-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115807" data-show=".short_summary_115807" data-hide=".short_summary_button_115807" >Short summary</span> <div class="j-widget__max short_summary short_summary_115807" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> A rapid quantitative identification criterion based on the basic chemical composition combination rules of red beds has been established, taking into account the correlation between red bed geomorphic characteristics, mineral compositions, and chemical compositions. The research results can also be applied to the quantitative identification of red beds in other fields, such as resources, ecology, environment, energy, and materials. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115807" data-show=".short_summary_button_115807">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://se.copernicus.org/articles/15/1185/2024/se-15-1185-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1185/2024/se-15-1185-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1185/2024/se-15-1185-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="542" 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://se.copernicus.org/articles/15/1155/2024/se-15-1155-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1155/2024/se-15-1155-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1155/2024/se-15-1155-2024-avatar-web.png" data-width="600" data-height="567" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 18 Sep 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1155/2024/">Anatomy of a fumarole field: drone remote-sensing and petrological approaches reveal the degassing and alteration structure at La Fossa cone, Vulcano, Italy</a> <div class="authors">Daniel Müller, Thomas R. Walter, Valentin R. Troll, Jessica Stammeier, Andreas Karlsson, Erica de Paolo, Antonino Fabio Pisciotta, Martin Zimmer, and Benjamin De Jarnatt</div> <div class="citation">Solid Earth, 15, 1155–1184, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1155-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1155-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_113473" data-show=".short_summary_113473" data-hide=".short_summary_button_113473" >Short summary</span> <div class="j-widget__max short_summary short_summary_113473" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We use uncrewed-aerial-system-derived optical and infrared data, mineralogical and geochemical analyses of rock samples, and surface degassing measurements to analyze degassing and hydrothermal alteration at the fumaroles of the La Fossa cone, Vulcano island, Italy. We give a detailed view of associated structures and dynamics, such as local alteration gradients, diffuse active units that significantly contribute to the total activity, or effects of permeability reduction and surface sealing.  </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_113473" data-show=".short_summary_button_113473">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://se.copernicus.org/articles/15/1155/2024/se-15-1155-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1155/2024/se-15-1155-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1155/2024/se-15-1155-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="567" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-0 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"> 18 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2692/">Lithologically constrained velocity–density relationships and vertical stress gradients in the North Alpine Foreland Basin, SE Germany</a> <div class="authors">Peter Obermeier, Florian Duschl, and Michael C. Drews</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2692,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2692,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 1 comment)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122841" data-show=".short_summary_122841" data-hide=".short_summary_button_122841" >Short summary</span> <div class="j-widget__max short_summary short_summary_122841" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We investigate geophysical properties and the distribution of vertical stress, which is defined by the weight of the rock column above a certain location in the subsurface, in the upper 5 km of the North Alpine Foreland Basin in Germany. Our results help to understand the present-day geological configuration and to improve safety for subsurface use, such as deep geothermal energy production in the study area. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122841" data-show=".short_summary_button_122841">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"> 18 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2637/">Passive seismic imaging of ore deposits using coda wave interferometry: a case study of Akanvaara V-Cr-PGE deposit in Northern Finland</a> <div class="authors">Nikita Afonin, Elena Kozlovskaya, Kari Moisio, Shenghong Yang, and Jouni Sarala</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2637,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2637,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 3 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122712" data-show=".short_summary_122712" data-hide=".short_summary_button_122712" >Short summary</span> <div class="j-widget__max short_summary short_summary_122712" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> In this study, we present an innovative method to study the inner structure of ore deposits using seismic waves produced by earthquakes and production blasts. Results of numerical simulations and field tests show that the proposed method can effectively detect mineralization zones inside orebodies. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122712" data-show=".short_summary_button_122712">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="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1143/2024/se-15-1143-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1143/2024/se-15-1143-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1143/2024/se-15-1143-2024-avatar-web.png" data-width="600" data-height="381" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 16 Sep 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1143/2024/">Magnesium isotope fractionation processes during seafloor serpentinization and implications for serpentinite subduction</a> <div class="authors">Sune G. Nielsen, Frieder Klein, Horst R. Marschall, Philip A. E. Pogge von Strandmann, and Maureen Auro</div> <div class="citation">Solid Earth, 15, 1143–1154, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1143-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1143-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116585" data-show=".short_summary_116585" data-hide=".short_summary_button_116585" >Short summary</span> <div class="j-widget__max short_summary short_summary_116585" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Magnesium isotope ratios of arc lavas have been proposed as a proxy for serpentinite subduction, but uncertainties remain regarding their utility. Here we show that bulk serpentinite Mg isotope ratios are identical to the mantle, whereas the serpentinite mineral brucite is enriched in heavy Mg isotopes. Thus, Mg isotope ratios may only be used as serpentinite subduction proxies if brucite is preferentially mobilized from the slab at pressures and temperatures within the arc magma source region. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116585" data-show=".short_summary_button_116585">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://se.copernicus.org/articles/15/1143/2024/se-15-1143-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1143/2024/se-15-1143-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1143/2024/se-15-1143-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="381" 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://se.copernicus.org/articles/15/1133/2024/se-15-1133-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1133/2024/se-15-1133-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1133/2024/se-15-1133-2024-avatar-web.png" data-width="600" data-height="317" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 16 Sep 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1133/2024/">Driven magmatism and crustal thinning of coastal southern China in response to subduction</a> <div class="authors">Jinbao Su, Wenbin Zhu, and Guangwei Li</div> <div class="citation">Solid Earth, 15, 1133–1141, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1133-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1133-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_119759" data-show=".short_summary_119759" data-hide=".short_summary_button_119759" >Short summary</span> <div class="j-widget__max short_summary short_summary_119759" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The late Mesozoic igneous rocks in the South China Block exhibit flare-ups and lulls, which form in compressional or extensional backgrounds. The ascending of magma forms a mush-like head and decreases crustal thickness. The presence of faults and pre-existing magmas will accelerate emplacement of underplating magma. The magmatism at different times may be formed under similar subduction conditions, and the boundary compression forces will delay magma ascent. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_119759" data-show=".short_summary_button_119759">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://se.copernicus.org/articles/15/1133/2024/se-15-1133-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1133/2024/se-15-1133-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1133/2024/se-15-1133-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="317" 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://se.copernicus.org/articles/15/1113/2024/se-15-1113-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1113/2024/se-15-1113-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1113/2024/se-15-1113-2024-avatar-web.png" data-width="600" data-height="509" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 12 Sep 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1113/2024/">How a volcanic arc influences back-arc extension: insight from 2D numerical models</a> <div class="authors">Duo Zhang and J. Huw Davies</div> <div class="citation">Solid Earth, 15, 1113–1132, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1113-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1113-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_113715" data-show=".short_summary_113715" data-hide=".short_summary_button_113715" >Short summary</span> <div class="j-widget__max short_summary short_summary_113715" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We numerically model the influence of an arc on back-arc extension. The arc is simulated by placing a hot region on the overriding plate. We investigate how plate ages and properties of the hot region affect back-arc extension and present regime diagrams illustrating the nature of back-arc extension for these models. We find that back-arc extension occurs not only in the hot region but also, surprisingly, away from it, and a hot region facilitates extension on the overriding plate. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_113715" data-show=".short_summary_button_113715">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://se.copernicus.org/articles/15/1113/2024/se-15-1113-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1113/2024/se-15-1113-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1113/2024/se-15-1113-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="509" width="80" height="80"> </a> </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"> 04 Sep 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1529/">Luminescence and a New Approach for Detecting Heat Treatment of Sapphire</a> <div class="authors">Teerarat Pluthametwisute, Lutz Nasdala, Chutimun Chanmuang N., Manfred Wildner, Eugen Libowitzky, Gerald Giester, Gamini Zoysa, Chanenkant Jakkawanvibul, Waratchanok Suwanmanee, Tasnara Sripoonjan, Thanyaporn Tengchaisri, Bhuwadol Wanthanachaisaeng, and Chakkaphan Sutthirat</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1529,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1529,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120426" data-show=".short_summary_120426" data-hide=".short_summary_button_120426" >Short summary</span> <div class="j-widget__max short_summary short_summary_120426" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> For years, mankind has heated sapphire to increase its blue color and value. Gemologists have struggled for decades to detect heat-treated sapphire. Each test costs money. High-tech instruments like FTIR are costly. As a result, luminescence under SWUV and LWUV light provides a cheaper and more practical technique for identifying heat-treated sapphire. This work highlights that blue luminescence under SWUV light could indicate heated sapphire, whereas purplish red may also be helpful. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120426" data-show=".short_summary_button_120426">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="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1087/2024/se-15-1087-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1087/2024/se-15-1087-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1087/2024/se-15-1087-2024-avatar-web.png" data-width="600" data-height="518" 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://se.copernicus.org/articles/15/1087/2024/">Selection and characterization of the target fault for fluid-induced activation and earthquake rupture experiments</a> <div class="authors">Peter Achtziger-Zupančič, Alberto Ceccato, Alba Simona Zappone, Giacomo Pozzi, Alexis Shakas, Florian Amann, Whitney Maria Behr, Daniel Escallon Botero, Domenico Giardini, Marian Hertrich, Mohammadreza Jalali, Xiaodong Ma, Men-Andrin Meier, Julian Osten, Stefan Wiemer, and Massimo Cocco</div> <div class="citation">Solid Earth, 15, 1087–1112, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1087-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1087-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118431" data-show=".short_summary_118431" data-hide=".short_summary_button_118431" >Short summary</span> <div class="j-widget__max short_summary short_summary_118431" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We detail the selection and characterization of a fault zone for earthquake experiments in the Fault Activation and Earthquake Ruptures (FEAR) project at the Bedretto Lab. FEAR, which studies earthquake processes, overcame data collection challenges near faults. The fault zone in Rotondo granite was selected based on geometry, monitorability, and hydro-mechanical properties. Remote sensing, borehole logging, and geological mapping were used to create a 3D model for precise monitoring. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118431" data-show=".short_summary_button_118431">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://se.copernicus.org/articles/15/1087/2024/se-15-1087-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1087/2024/se-15-1087-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1087/2024/se-15-1087-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="518" width="80" height="80"> </a> </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"> 29 Aug 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2399/">Paleoseismological evidence of multiple, large magnitude earthquake surface ruptures on the active Mt. Morrone normal fault, central Apennines, Italy</a> <div class="authors">Irene Puliti, Alberto Pizzi, Stefano Gori, Emanuela Falcucci, Fabrizio Galadini, Marco Moro, and Michele Saroli</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2399,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2399,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 2 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122269" data-show=".short_summary_122269" data-hide=".short_summary_button_122269" >Short summary</span> <div class="j-widget__max short_summary short_summary_122269" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We performed a paleoseismological study on the Mt. Morrone active fault, which constitutes one of the most problematic structures of the central Apennines in terms of large-earthquake probability. Information on historical seismicity is relatively few and the paleoseismological record is limited only to the northern portion of the fault. We investigated four trenches and we recovered the occurrence of three events over the last 5–6 kyrs, suggesting an average recurrence interval of 1800 years. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122269" data-show=".short_summary_button_122269">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="3"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/1065/2024/se-15-1065-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1065/2024/se-15-1065-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1065/2024/se-15-1065-2024-avatar-web.png" data-width="600" data-height="507" 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://se.copernicus.org/articles/15/1065/2024/">Evolution of fluid redox in a fault zone of the Pic de Port Vieux thrust in the Pyrenees Axial Zone (Spain)</a> <div class="authors">Delphine Charpentier, Gaétan Milesi, Pierre Labaume, Ahmed Abd Elmola, Martine Buatier, Pierre Lanari, and Manuel Muñoz</div> <div class="citation">Solid Earth, 15, 1065–1086, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1065-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1065-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118038" data-show=".short_summary_118038" data-hide=".short_summary_button_118038" >Short summary</span> <div class="j-widget__max short_summary short_summary_118038" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Understanding the fluid circulation in fault zones is essential to characterize the thermochemical evolution of hydrothermal systems in mountain ranges. The study focused on a paleo-system of the Pyrenees. Phyllosilicates permit us to constrain the evolution of temperature and redox of fluids at the scale of the fault system. A scenario is proposed and involves the circulation of a single highly reducing hydrothermal fluid (~300 °C) that evolves due to redox reactions. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118038" data-show=".short_summary_button_118038">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://se.copernicus.org/articles/15/1065/2024/se-15-1065-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1065/2024/se-15-1065-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1065/2024/se-15-1065-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="507" 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://se.copernicus.org/articles/15/1047/2024/se-15-1047-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1047/2024/se-15-1047-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1047/2024/se-15-1047-2024-avatar-web.png" data-width="600" data-height="444" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 23 Aug 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1047/2024/">Stress state at faults: the influence of rock stiffness contrast, stress orientation, and ratio</a> <div class="authors">Moritz O. Ziegler, Robin Seithel, Thomas Niederhuber, Oliver Heidbach, Thomas Kohl, Birgit Müller, Mojtaba Rajabi, Karsten Reiter, and Luisa Röckel</div> <div class="citation">Solid Earth, 15, 1047–1063, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1047-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1047-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_119405" data-show=".short_summary_119405" data-hide=".short_summary_button_119405" >Short summary</span> <div class="j-widget__max short_summary short_summary_119405" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The rotation of the principal stress axes in a fault structure because of a rock stiffness contrast has been investigated for the impact of the ratio of principal stresses, the angle between principal stress axes and fault strike, and the ratio of the rock stiffness contrast. A generic 2D geomechanical model is employed for the systematic investigation of the parameter space. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_119405" data-show=".short_summary_button_119405">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://se.copernicus.org/articles/15/1047/2024/se-15-1047-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1047/2024/se-15-1047-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1047/2024/se-15-1047-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="444" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-1 in-range paperList-discussion" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 22 Aug 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1919/">Investigation of Seismic Anisotropy in the Undisturbed Rotondo Granite</a> <div class="authors">Kathrin Behnen, Marian Hertrich, Hansruedi Maurer, Alexis Shakas, Kai Bröker, Claire Epiney, María Blanch Jover, and Domenico Giardini</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1919,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1919,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 2 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121329" data-show=".short_summary_121329" data-hide=".short_summary_button_121329" >Short summary</span> <div class="j-widget__max short_summary short_summary_121329" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Several crosshole seismic surveys in the undisturbed Rotondo granite are used to analyze the seismic anisotropy in the BedrettoLab in the Swiss alps. The P- and S1-waves show a clear trend of faster velocities in NE-SW direction and slower velocities perpendicular to it. This pattern describes a tilted transverse isotropic velocity model. The symmetry plane is mostly aligned with the direction of maximum stress but also the orientation of fractures are expected to influence the wave velocities. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121329" data-show=".short_summary_button_121329">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://se.copernicus.org/articles/15/1029/2024/se-15-1029-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1029/2024/se-15-1029-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1029/2024/se-15-1029-2024-avatar-web.png" data-width="600" data-height="522" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 15 Aug 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1029/2024/">Post-Caledonian tectonic evolution of the Precambrian and Paleozoic platform boundary zone offshore Poland based on the new and vintage multi-channel reflection seismic data</a> <div class="authors">Quang Nguyen, Michal Malinowski, Stanisław Mazur, Sergiy Stovba, Małgorzata Ponikowska, and Christian Hübscher</div> <div class="citation">Solid Earth, 15, 1029–1046, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1029-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1029-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116497" data-show=".short_summary_116497" data-hide=".short_summary_button_116497" >Short summary</span> <div class="j-widget__max short_summary short_summary_116497" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Our work demonstrates the following: (1) an efficient seismic data-processing strategy focused on suppressing shallow-water multiple reflections. (2) An improvement in the quality of legacy marine seismic data. (3) A seismic interpretation of sedimentary successions overlying the basement in the transition zone from the Precambrian to Paleozoic platforms. (4) The tectonic evolution of the Koszalin Fault and its relation to the Caledonian Deformation Front offshore Poland. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116497" data-show=".short_summary_button_116497">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://se.copernicus.org/articles/15/1029/2024/se-15-1029-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1029/2024/se-15-1029-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1029/2024/se-15-1029-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="522" 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://se.copernicus.org/articles/15/945/2024/se-15-945-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/945/2024/se-15-945-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/945/2024/se-15-945-2024-avatar-web.png" data-width="600" data-height="207" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 09 Aug 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/945/2024/">What does it take to restore geological models with “natural” boundary conditions?</a> <div class="authors">Melchior Schuh-Senlis, Guillaume Caumon, and Paul Cupillard</div> <div class="citation">Solid Earth, 15, 945–964, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-945-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-945-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_114669" data-show=".short_summary_114669" data-hide=".short_summary_button_114669" >Short summary</span> <div class="j-widget__max short_summary short_summary_114669" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This paper presents the application of a numerical method for restoring models of the subsurface to a previous state in their deformation history, acting as a numerical time machine for geological structures. The method is applied to a model based on a laboratory experiment. The results show that using force conditions in the computation of the deformation allows us to assess the value of some previously unknown physical parameters of the different materials inside the model. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_114669" data-show=".short_summary_button_114669">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://se.copernicus.org/articles/15/945/2024/se-15-945-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/945/2024/se-15-945-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/945/2024/se-15-945-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="207" 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://se.copernicus.org/articles/15/965/2024/se-15-965-2024-avatar-web.jpg"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/965/2024/se-15-965-2024-avatar-thumb80.jpg" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/965/2024/se-15-965-2024-avatar-web.jpg" data-width="600" data-height="403" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 09 Aug 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/965/2024/">Interseismic and long-term deformation of southeastern Sicily driven by the Ionian slab roll-back</a> <div class="authors">Amélie Viger, Stéphane Dominguez, Stéphane Mazzotti, Michel Peyret, Maxime Henriquet, Giovanni Barreca, Carmelo Monaco, and Adrien Damon</div> <div class="citation">Solid Earth, 15, 965–988, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-965-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-965-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_117473" data-show=".short_summary_117473" data-hide=".short_summary_button_117473" >Short summary</span> <div class="j-widget__max short_summary short_summary_117473" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> New satellite geodetic data (PS-InSAR) evidence a generalized subsidence and an eastward tilting of southeastern Sicily combined with a local relative uplift along its eastern coast. We perform flexural and elastic modeling and show that the slab pull force induced by the Ionian slab roll-back and extrado deformation reproduce the measured surface deformation. Finally, we propose an original seismic cycle model that is mainly driven by the southward migration of the Ionian slab roll-back. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_117473" data-show=".short_summary_button_117473">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://se.copernicus.org/articles/15/965/2024/se-15-965-2024-avatar-web.jpg"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/965/2024/se-15-965-2024-avatar-thumb80.jpg" data-web="https://se.copernicus.org/articles/15/965/2024/se-15-965-2024-avatar-web.jpg" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="403" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-1 in-range paperList-discussion" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 08 Aug 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1696/">Quaternary surface ruptures of the inherited mature Yangsan fault: implications for intraplate earthquakes in Southeastern Korea</a> <div class="authors">Sangmin Ha, Hee-Cheol Kang, Seongjun Lee, Yeong Bae Seong, Jeong-Heon Choi, Seok-Jin Kim, and Moon Son</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1696,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1696,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120852" data-show=".short_summary_120852" data-hide=".short_summary_button_120852" >Short summary</span> <div class="j-widget__max short_summary short_summary_120852" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Unlike episodic plate boundary earthquakes, their randomness makes predicting intraplate earthquakes challenging. This study aids seismic hazard assessment by analyzing paleoearthquake records of the Yangsan Fault in Korea. Five trench sites revealed three Quaternary surface-rupturing earthquakes, the latest 3,000 years ago, with M<sub>w</sub> 6.7–7.2. The right lateral fault has a 0.14 mm/yr slip rate, and a recurrence interval over 10,000 years, continuously active since the Quaternary. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120852" data-show=".short_summary_button_120852">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://se.copernicus.org/articles/15/921/2024/se-15-921-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/921/2024/se-15-921-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/921/2024/se-15-921-2024-avatar-web.png" data-width="600" data-height="220" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 06 Aug 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/921/2024/">Geodynamic controls on clastic-dominated base metal deposits</a> <div class="authors">Anne C. Glerum, Sascha Brune, Joseph M. Magnall, Philipp Weis, and Sarah A. Gleeson</div> <div class="citation">Solid Earth, 15, 921–944, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-921-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-921-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115688" data-show=".short_summary_115688" data-hide=".short_summary_button_115688" >Short summary</span> <div class="j-widget__max short_summary short_summary_115688" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> High-value zinc–lead deposits formed in sedimentary basins created when tectonic plates rifted apart. We use computer simulations of rifting and the associated sediment erosion and deposition to understand why they formed in some basins but not in others. Basins that contain a metal source, faults that focus fluids, and rocks that can host deposits occurred in both narrow and wide rifts for ≤ 3 Myr. The largest and the most deposits form in narrow margins of narrow asymmetric rifts. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115688" data-show=".short_summary_button_115688">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://se.copernicus.org/articles/15/921/2024/se-15-921-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/921/2024/se-15-921-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/921/2024/se-15-921-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="220" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-3 in-range paperList-discussion" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 30 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2319/">Reconciling post-orogenic faulting, paleostress evolution and structural inheritance in the seismogenic Northern Apennines (Italy): Insights from the Monti Martani Fault System</a> <div class="authors">Riccardo Asti, Selina Bonini, Giulio Viola, and Gianluca Vignaroli</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2319,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2319,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for SE</span> <nobr>(discussion: final response, 5 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_122135" data-show=".short_summary_122135" data-hide=".short_summary_button_122135" >Short summary</span> <div class="j-widget__max short_summary short_summary_122135" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This study addresses the tectonic evolution of the seismogenic Monti Martani Fault System (Northern Apennines, Italy). By applying a field-based structural geology approach, we reconstruct the evolution of the stress field and we challenge the current interpretation of the fault system both in terms of geometry and state of activity. We stress that the peculiar behavior of this system during post-orogenic extension is still significantly influenced by the pre-orogenic structural template. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_122135" data-show=".short_summary_button_122135">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-2 in-range paperList-discussion" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 24 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1515/">On crustal composition of the Sardinia-Corsica continental block inferred from receiver functions</a> <div class="authors">Fabio Cammarano, Henrique Berger Roisenberg, Alessio Conclave, Islam Fadel, and Mark van der Meijde</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1515,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1515,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript under review for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120400" data-show=".short_summary_120400" data-hide=".short_summary_button_120400" >Short summary</span> <div class="j-widget__max short_summary short_summary_120400" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Sardinia and Corsica separated and drifting in the Mediterranean Sea for 35 my due to the retreat of the Ionian plate beneath the Tyrrhenian Sea. Using in-house and public data, we measured and interpreted receiver functions based on prior geophysical and petrological studies. Our findings indicate the islands' ancient continental structure remains mostly unchanged. Alpine orogenesis about 50 million years ago influenced Corsica's crust, enriching it with water-bearing minerals </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120400" data-show=".short_summary_button_120400">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://se.copernicus.org/articles/15/895/2024/se-15-895-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/895/2024/se-15-895-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/895/2024/se-15-895-2024-avatar-web.png" data-width="452" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 23 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/895/2024/">Naturally fractured reservoir characterisation in heterogeneous sandstones: insight for uranium in situ recovery (Imouraren, Niger)</a> <div class="authors">Maxime Jamet, Gregory Ballas, Roger Soliva, Olivier Gerbeaud, Thierry Lefebvre, Christine Leredde, and Didier Loggia</div> <div class="citation">Solid Earth, 15, 895–920, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-895-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-895-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118143" data-show=".short_summary_118143" data-hide=".short_summary_button_118143" >Short summary</span> <div class="j-widget__max short_summary short_summary_118143" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This study characterizes the Tchirezrine II sandstone reservoir in northern Niger. Crucial for potential uranium in situ recovery (ISR), our multifaceted approach reveals (i) a network of homogeneously distributed orthogonal structures, (ii) the impact of clustered E–W fault structures on anisotropic fluid flow, and (iii) local changes in the matrix behaviour of the reservoir as a function of the density and nature of the deformation structure. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118143" data-show=".short_summary_button_118143">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://se.copernicus.org/articles/15/895/2024/se-15-895-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/895/2024/se-15-895-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/895/2024/se-15-895-2024-avatar-web.png" data-width="452" 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-2 in-range paperList-discussion" data-diff="4"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 23 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2003/">The role of siliceous sponges in pre-Eocene marine Si cycle from the perspective of rock mineralogy</a> <div class="authors">Agata Jurkowska, Ewa Świerczewska-Gładysz, and Szymon Kowalik Filipowicz</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2003,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2003,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript under review for SE</span> <nobr>(discussion: final response, 8 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121585" data-show=".short_summary_121585" data-hide=".short_summary_button_121585" >Short summary</span> <div class="j-widget__max short_summary short_summary_121585" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The process of siliceous sponge dissolution is an important part of Si cycle and was interpreted as a main mechanism contributing the chert formation. We presented the contradicting theory and revealed that the seawater Si concentration were the main factor controlling the siliceous rock formation in Palaeozoic and Mesozoic. This new idea highlight the use of δ<sup>30</sup>Si as possible indicator of Si origin in cherts and carbonate-siliceous rocks. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121585" data-show=".short_summary_button_121585">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://se.copernicus.org/articles/15/877/2024/se-15-877-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/877/2024/se-15-877-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/877/2024/se-15-877-2024-avatar-web.png" data-width="600" data-height="353" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 22 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/877/2024/">Extraction of pre-earthquake anomalies from borehole strain data using Graph WaveNet: a case study of the 2013 Lushan earthquake in China</a> <div class="authors">Chenyang Li, Yu Duan, Ying Han, Zining Yu, Chengquan Chi, and Dewang Zhang</div> <div class="citation">Solid Earth, 15, 877–893, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-877-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-877-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116338" data-show=".short_summary_116338" data-hide=".short_summary_button_116338" >Short summary</span> <div class="j-widget__max short_summary short_summary_116338" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This study advances the field of earthquake prediction by introducing an extraction method for pre-seismic anomalies based on the structure of Graph WaveNet networks. We believe that our study makes a significant contribution to the literature as it not only demonstrates the effectiveness of this innovative approach in integrating borehole strain data from multiple stations but also reveals distinct temporal and spatial correlations preceding earthquake events. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116338" data-show=".short_summary_button_116338">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://se.copernicus.org/articles/15/877/2024/se-15-877-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/877/2024/se-15-877-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/877/2024/se-15-877-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="353" width="80" height="80"> </a> </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://se.copernicus.org/articles/15/861/2024/se-15-861-2024-avatar-web.jpg"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/861/2024/se-15-861-2024-avatar-thumb80.jpg" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/861/2024/se-15-861-2024-avatar-web.jpg" data-width="292" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 19 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/861/2024/">Quantifying mantle mixing through configurational entropy</a> <div class="authors">Erik van der Wiel, Cedric Thieulot, and Douwe J. J. van Hinsbergen</div> <div class="citation">Solid Earth, 15, 861–875, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-861-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-861-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116424" data-show=".short_summary_116424" data-hide=".short_summary_button_116424" >Short summary</span> <div class="j-widget__max short_summary short_summary_116424" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Geodynamic models of mantle convection provide a powerful tool to study the structure and composition of the Earth's mantle. Comparing such models with other datasets is difficult. We explore the use of <q>configurational entropy</q>, which allows us to quantify mixing in models. The entropy may be used to analyse the mixed state of the mantle as a whole and may also be useful to validate numerical models against anomalies in the mantle that are obtained from seismology and geochemistry. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116424" data-show=".short_summary_button_116424">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://se.copernicus.org/articles/15/861/2024/se-15-861-2024-avatar-web.jpg"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/861/2024/se-15-861-2024-avatar-thumb80.jpg" data-web="https://se.copernicus.org/articles/15/861/2024/se-15-861-2024-avatar-web.jpg" data-width="292" 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="5"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/837/2024/se-15-837-2024-avatar-web.jpg"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/837/2024/se-15-837-2024-avatar-thumb80.jpg" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/837/2024/se-15-837-2024-avatar-web.jpg" data-width="368" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 16 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/837/2024/">Palaeoseismic crisis in the Galera Fault (southern Spain): consequences in Bronze Age settlements?</a> <div class="authors">Ivan Martin-Rojas, Ivan Medina-Cascales, Francisco Juan García-Tortosa, Maria Oliva Rodríguez-Ariza, Fernando Molina González, Juan Antonio Cámara Serrano, and Pedro Alfaro</div> <div class="citation">Solid Earth, 15, 837–860, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-837-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-837-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115447" data-show=".short_summary_115447" data-hide=".short_summary_button_115447" >Short summary</span> <div class="j-widget__max short_summary short_summary_115447" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We investigated prehistoric earthquakes produced by the Galera Fault (southern Spain) over the last 24 000 years. From this analysis, we deduced the basic parameters that allow for the characterization of the seismic hazard of this fault. Furthermore, we discuss how the Galera Fault is prone to producing seismic crises. We also propose that one of these crises could have been responsible for the abandonment of Bronze Age human settlements located near the fault. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115447" data-show=".short_summary_button_115447">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://se.copernicus.org/articles/15/837/2024/se-15-837-2024-avatar-web.jpg"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/837/2024/se-15-837-2024-avatar-thumb80.jpg" data-web="https://se.copernicus.org/articles/15/837/2024/se-15-837-2024-avatar-web.jpg" data-width="368" 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="5"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/827/2024/se-15-827-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/827/2024/se-15-827-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/827/2024/se-15-827-2024-avatar-web.png" data-width="600" data-height="277" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 15 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/827/2024/">Highlights on mantle deformation beneath the Western Alps with seismic anisotropy using CIFALPS2 data</a> <div class="authors">Silvia Pondrelli, Simone Salimbeni, Judith M. Confal, Marco G. Malusà, Anne Paul, Stephane Guillot, Stefano Solarino, Elena Eva, Coralie Aubert, and Liang Zhao</div> <div class="citation">Solid Earth, 15, 827–835, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-827-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-827-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_118236" data-show=".short_summary_118236" data-hide=".short_summary_button_118236" >Short summary</span> <div class="j-widget__max short_summary short_summary_118236" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We analyse and interpret seismic anisotropy from CIFALPS2 data that fill the gaps in the Western Alps and support a new hypothesis. Instead of a continuous mantle flow parallel to the belt, here we find a N–S mantle deformation pattern that merges first with a mantle deformed by slab steepening beneath the Central Alps and then merges with an asthenospheric flow sourced beneath the Massif Central. This new sketch supports the extinction of slab retreat beneath the Western Alps. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_118236" data-show=".short_summary_button_118236">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://se.copernicus.org/articles/15/827/2024/se-15-827-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/827/2024/se-15-827-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/827/2024/se-15-827-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="277" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-2 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"> 15 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2034/">Insights into the tectonic evolution of the Svecofennian orogeny based on <em>in situ</em> Lu-Hf dating of garnet from Olkiluoto, SW Finland</a> <div class="authors">Jon Engström, Kathryn Cutts, Stijn Glorie, Esa Heilimo, Ester M. Jolis, and Radoslaw M. Michallik</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-2034,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-2034,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript under review for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121649" data-show=".short_summary_121649" data-hide=".short_summary_button_121649" >Short summary</span> <div class="j-widget__max short_summary short_summary_121649" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This paper describes migmatites and associated rocks in SW Finland that have been studied using the new in situ garnet and apatite Lu-Hf geochronology method. The metamorphic constraints and age presented in this paper enhance our understanding of the geological evolution in SW Finland. The results reveal detailed temporal constraints for the tectonic evolution that can be linked to major events in adjacent tectonic blocks in both Finland and Sweden during the Svecofennian orogeny. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121649" data-show=".short_summary_button_121649">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://se.copernicus.org/articles/15/807/2024/se-15-807-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/807/2024/se-15-807-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/807/2024/se-15-807-2024-avatar-web.png" data-width="543" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 09 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/807/2024/">Rift and plume: a discussion on active and passive rifting mechanisms in the Afro-Arabian rift based on synthesis of geophysical data</a> <div class="authors">Ran Issachar, Peter Haas, Nico Augustin, and Jörg Ebbing</div> <div class="citation">Solid Earth, 15, 807–826, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-807-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-807-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115606" data-show=".short_summary_115606" data-hide=".short_summary_button_115606" >Short summary</span> <div class="j-widget__max short_summary short_summary_115606" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> In this contribution, we explore the causal relationship between the arrival of the Afar plume and the initiation of the Afro-Arabian rift. We mapped the rift architecture in the triple-junction region using geophysical data and reviewed the available geological data. We interpret a progressive development of the plume–rift system and suggest an interaction between active and passive mechanisms in which the plume provided a push force that changed the kinematics of the associated plates. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115606" data-show=".short_summary_button_115606">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://se.copernicus.org/articles/15/807/2024/se-15-807-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/807/2024/se-15-807-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/807/2024/se-15-807-2024-avatar-web.png" data-width="543" 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="5"> <div class="grid-100 hide-on-desktop hide-on-tablet"> <a class="paperlist-avatar" target="_blank" href="https://se.copernicus.org/articles/15/789/2024/se-15-789-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/789/2024/se-15-789-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/789/2024/se-15-789-2024-avatar-web.png" data-width="600" data-height="361" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 08 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/789/2024/">Various lithospheric deformation patterns derived from rheological contrasts between continental terranes: insights from 2-D numerical simulations</a> <div class="authors">Renxian Xie, Lin Chen, Jason P. Morgan, and Yongshun John Chen</div> <div class="citation">Solid Earth, 15, 789–806, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-789-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-789-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116069" data-show=".short_summary_116069" data-hide=".short_summary_button_116069" >Short summary</span> <div class="j-widget__max short_summary short_summary_116069" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Continental terranes have various rheological strengths due to the differences in their ages, compositions, and structures. We applied four assumed rheological models to three terranes in a collisional model and obtained four styles of lithosphere deformation patterns of collision, subduction, thickening/delamination, and replacement. These simulation patterns are seen in observed lithosphere deformation patterns and structures in East Asia. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116069" data-show=".short_summary_button_116069">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://se.copernicus.org/articles/15/789/2024/se-15-789-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/789/2024/se-15-789-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/789/2024/se-15-789-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="361" width="80" height="80"> </a> </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://se.copernicus.org/articles/15/763/2024/se-15-763-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/763/2024/se-15-763-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/763/2024/se-15-763-2024-avatar-web.png" data-width="600" data-height="599" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 08 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/763/2024/">Impact of stress regime change on the permeability of a naturally fractured carbonate buildup (Latemar, the Dolomites, northern Italy)</a> <div class="authors">Onyedika Anthony Igbokwe, Jithender J. Timothy, Ashwani Kumar, Xiao Yan, Mathias Mueller, Alessandro Verdecchia, Günther Meschke, and Adrian Immenhauser</div> <div class="citation">Solid Earth, 15, 763–787, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-763-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-763-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116031" data-show=".short_summary_116031" data-hide=".short_summary_button_116031" >Short summary</span> <div class="j-widget__max short_summary short_summary_116031" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We present a workflow that models the impact of stress regime change on the permeability of fractured Latemar carbonate buildup using a displacement-based linear elastic finite-element method (FEM) and outcrop data. Stress-dependent heterogeneous apertures and effective permeability were calculated and constrained by the study area's stress directions. Simulated far-field stresses at NW–SE subsidence deformation and N–S Alpine deformation increased the overall fracture aperture and permeability. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116031" data-show=".short_summary_button_116031">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://se.copernicus.org/articles/15/763/2024/se-15-763-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/763/2024/se-15-763-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/763/2024/se-15-763-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="599" width="80" height="80"> </a> </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://se.copernicus.org/articles/15/747/2024/se-15-747-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/747/2024/se-15-747-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/747/2024/se-15-747-2024-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"> 05 Jul 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/747/2024/">Propagating rifts: the roles of crustal damage and ascending mantle fluids</a> <div class="authors">Folarin Kolawole and Rasheed Ajala</div> <div class="citation">Solid Earth, 15, 747–762, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-747-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-747-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115862" data-show=".short_summary_115862" data-hide=".short_summary_button_115862" >Short summary</span> <div class="j-widget__max short_summary short_summary_115862" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We investigate the upper-crustal structure of the Rukwa–Tanganyika rift zone in East Africa, where the Tanganyika rift interacts with the Rukwa and Mweru-Wantipa rifts, coinciding with abundant seismicity at the rift tips. Seismic velocity structure and patterns of seismicity clustering reveal zones around 10 km deep with anomalously high <em>V</em><sub>p</sub> / <em>V</em><sub>s</sub> ratios at the rift tips, indicative of a localized mechanically weakened crust caused by mantle volatiles and damage associated with bending strain. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115862" data-show=".short_summary_button_115862">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://se.copernicus.org/articles/15/747/2024/se-15-747-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/747/2024/se-15-747-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/747/2024/se-15-747-2024-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 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"> 04 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1841/">Earthquake swarms frozen in an exhumed hydrothermal system (Bolfin Fault Zone, Chile)</a> <div class="authors">Simone Masoch, Giorgio Pennacchioni, Michele Fondriest, Rodrigo Gomila, Piero Poli, José Cembrano, and Giulio Di Toro</div> <div class="citation">External preprint server, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.22541/essoar.171995191.13613873/v1,</nobr><span class="hide-on-desktop">https://doi.org/10.22541/essoar.171995191.13613873/v1,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121184" data-show=".short_summary_121184" data-hide=".short_summary_button_121184" >Short summary</span> <div class="j-widget__max short_summary short_summary_121184" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We investigate an exhumed hydrothermal system in the Atacama Desert (Chile) to understand how earthquake swarms form. Wall-rocks near fault-veins experienced high-stress pulses, and fault-veins underwent cyclic crack opening and shearing. These findings suggest ancient earthquake swarm activity, from dynamic crack propagation to repeated crack opening and shearing. This system represents a unique geological record of earthquake swarms, providing insight into their initiation and evolution. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121184" data-show=".short_summary_button_121184">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"> 03 Jul 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1906/">Understanding the stress field at the lateral termination of a thrust fold using generic geomechanical models and clustering methods</a> <div class="authors">Anthony Adwan, Bertrand Maillot, Pauline Souloumiac, Christophe Barnes, Christophe Nussbaum, Meinert Rahn, and Thomas Van Stiphout</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1906,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1906,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript accepted for SE</span> <nobr>(discussion: final response, 5 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_121311" data-show=".short_summary_121311" data-hide=".short_summary_button_121311" >Short summary</span> <div class="j-widget__max short_summary short_summary_121311" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> <div class="flex-shrink-0 flex flex-col relative items-end"> <div> <div class="pt-0.5 juice:pt-0"> <div class="gizmo-bot-avatar flex h-6 w-6 items-center justify-center overflow-hidden rounded-full juice:h-8 juice:w-8"> <div class="relative p-1 rounded-sm flex items-center justify-center bg-token-main-surface-primary text-token-text-primary h-8 w-8">We use computer simulations to study how stress is distributed in large-scale geological models, focusing on how fault lines behave under pressure. By running many 2D and 3D simulations with varying conditions, we discover patterns in how faults form and interact. Our findings reveal that even small changes in conditions can lead to different stress outcomes. This research helps us better understand earthquake mechanics and could improve predictions of fault behavior in real-world scenarios.</div> </div> </div> </div> </div> </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_121311" data-show=".short_summary_button_121311">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://se.copernicus.org/articles/15/731/2024/se-15-731-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/731/2024/se-15-731-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/731/2024/se-15-731-2024-avatar-web.png" data-width="600" data-height="338" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 28 Jun 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/731/2024/">Mapping geochemical anomalies by accounting for the uncertainty of mineralization-related elemental associations</a> <div class="authors">Jian Wang, Renguang Zuo, and Qinghai Liu</div> <div class="citation">Solid Earth, 15, 731–746, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-731-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-731-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_116440" data-show=".short_summary_116440" data-hide=".short_summary_button_116440" >Short summary</span> <div class="j-widget__max short_summary short_summary_116440" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> This study improves geochemical mapping by addressing the uncertainty in defining element associations. It clusters the study area by element similarity, recognizes elemental associations for each cluster, and then detects anomalies indicating underlying geological processes. This method is applied to a region in China, confirming its effectiveness and consistency with the geology. This study can enhance geochemical mapping for mineral exploration and improve geological-process understanding. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_116440" data-show=".short_summary_button_116440">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://se.copernicus.org/articles/15/731/2024/se-15-731-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/731/2024/se-15-731-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/731/2024/se-15-731-2024-avatar-web.png" data-width="600" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="338" width="80" height="80"> </a> </div> </div> <div class="grid-container paperlist-object type-0 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"> 26 Jun 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1145/">Petrogenesis of Early Paleozoic I-type granitoids in the Longshoushan and implications for the tectonic affinity and evolution of the southwestern Alxa Block</a> <div class="authors">Renyu Zeng, Hui Su, Mark B. Allen, Haiyan Shi, Houfa Dua, Chenguang Zhange, and Jie Yan</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1145,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1145,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: open, 3 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_119468" data-show=".short_summary_119468" data-hide=".short_summary_button_119468" >Short summary</span> <div class="j-widget__max short_summary short_summary_119468" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> There has long been debate regarding the tectonic affinity and tectonic evolution of the Longshoushan, Alxa Block, during the Paleozoic. In this study, we present new geochronological and geochemical data for early Paleozoic granitoids from the Longshoushan. The main conclusions are as follows: (1) the Longshoushan was primarily influenced by the North Qilian Orogenic Belt; (2) The transition in crustal thickness occurred at ~435 Ma; (3) A three-stage Early Paleozoic tectonic model is proposed. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_119468" data-show=".short_summary_button_119468">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://se.copernicus.org/articles/15/711/2024/se-15-711-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/711/2024/se-15-711-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/711/2024/se-15-711-2024-avatar-web.png" data-width="409" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 24 Jun 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/711/2024/">Magmatic underplating associated with Proterozoic basin formation: insights from gravity study over the southern margin of the Bundelkhand Craton, India</a> <div class="authors">Ananya Parthapradip Mukherjee and Animesh Mandal</div> <div class="citation">Solid Earth, 15, 711–729, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-711-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-711-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_112684" data-show=".short_summary_112684" data-hide=".short_summary_button_112684" >Short summary</span> <div class="j-widget__max short_summary short_summary_112684" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> Global gravity data are used to develop 2D models and a Moho depth map from 3D inversion, depicting the crustal structure below the region covered by Proterozoic sedimentary basins, south of the Bundelkhand Craton in central India. The observed thick mafic underplated layer above the Moho indicates Proterozoic plume activity. Thus, the study offers insights into the crustal configuration of this region, illustrating the geodynamic processes that led to the formation of the basins. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_112684" data-show=".short_summary_button_112684">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://se.copernicus.org/articles/15/711/2024/se-15-711-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/711/2024/se-15-711-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/711/2024/se-15-711-2024-avatar-web.png" data-width="409" 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://se.copernicus.org/articles/15/683/2024/se-15-683-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/683/2024/se-15-683-2024-avatar-thumb80.png" data-caption="© Amante and Eakins 2009" data-web="https://se.copernicus.org/articles/15/683/2024/se-15-683-2024-avatar-web.png" data-width="600" data-height="538" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 21 Jun 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/683/2024/">Magma-poor continent–ocean transition zones of the southern North Atlantic: a wide-angle seismic synthesis of a new frontier</a> <div class="authors">J. Kim Welford</div> <div class="citation">Solid Earth, 15, 683–710, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-683-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-683-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115906" data-show=".short_summary_115906" data-hide=".short_summary_button_115906" >Short summary</span> <div class="j-widget__max short_summary short_summary_115906" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> I present a synthesis of the continent–ocean boundaries of the southern North Atlantic Ocean, as probed using seismic methods for rock velocity estimation, to assess their deep structures from the crust to the upper mantle and to discuss how they were formed. With this knowledge, it is possible to start evaluating these regions of the Earth for their capacity to produce hydrogen and critical minerals and to store excess carbon dioxide, all with the goal of greening our economy. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115906" data-show=".short_summary_button_115906">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://se.copernicus.org/articles/15/683/2024/se-15-683-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/683/2024/se-15-683-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/683/2024/se-15-683-2024-avatar-web.png" data-width="600" data-caption="© Amante and Eakins 2009" data-height="538" 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://se.copernicus.org/articles/15/671/2024/se-15-671-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/671/2024/se-15-671-2024-avatar-thumb80.png" data-caption="© Sandwell et al. 2014 for the left map. All rights reserved. © Authors for the right maps. Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/671/2024/se-15-671-2024-avatar-web.png" data-width="600" data-height="571" 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://se.copernicus.org/articles/15/671/2024/">Cretaceous–Paleocene extension at the southwestern continental margin of India and opening of the Laccadive basin: constraints from geophysical data</a> <div class="authors">Mathews George Gilbert, Parakkal Unnikrishnan, and Munukutla Radhakrishna</div> <div class="citation">Solid Earth, 15, 671–682, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-671-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-671-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_113625" data-show=".short_summary_113625" data-hide=".short_summary_button_113625" >Short summary</span> <div class="j-widget__max short_summary short_summary_113625" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The study identifies evidence for extension south of Tellicherry Arch along the southwestern continental margin of India through the integrated analysis of multichannel seismic and gravity data. The sediment deposition pattern indicates that this extension occurred after the Eocene. We further propose that the anticlockwise rotation of India and the passage of the Réunion plume have facilitated the opening of the Laccadive basin. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_113625" data-show=".short_summary_button_113625">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://se.copernicus.org/articles/15/671/2024/se-15-671-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/671/2024/se-15-671-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/671/2024/se-15-671-2024-avatar-web.png" data-width="600" data-caption="© Sandwell et al. 2014 for the left map. All rights reserved. © Authors for the right maps. Distributed under the Creative Commons Attribution 4.0 License." data-height="571" 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://se.copernicus.org/articles/15/657/2024/se-15-657-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/657/2024/se-15-657-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/657/2024/se-15-657-2024-avatar-web.png" data-width="513" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 14 Jun 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/657/2024/">Frequency-dependent shear wave attenuation across the Central Anatolia region, Türkiye</a> <div class="authors">Gizem Izgi, Tuna Eken, Peter Gaebler, Tülay Kaya-Eken, and Tuncay Taymaz</div> <div class="citation">Solid Earth, 15, 657–669, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-657-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-657-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_115789" data-show=".short_summary_115789" data-hide=".short_summary_button_115789" >Short summary</span> <div class="j-widget__max short_summary short_summary_115789" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> <p class="western" lang="en-US" align="justify">In this manuscript, we investigate the complexity of the upper-crustal block of the Central Anatolia region, Türkiye. We present the results of seismic attenuation by examining 1509 local earthquakes recorded at 72 broadband stations and deployed within the framework of a passive seismic experiment. We emphasize the detailed 2D maps of intrinsic and scattering attenuation within the area where two devastating earthquakes (<em>M</em><sub>1</sub><em> </em>7.8 and <em>M</em><sub>1</sub><em> </em>7.5 Kahramanmaraş Earthquake Sequence) happened in 2023. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_115789" data-show=".short_summary_button_115789">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://se.copernicus.org/articles/15/657/2024/se-15-657-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/657/2024/se-15-657-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/657/2024/se-15-657-2024-avatar-web.png" data-width="513" 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://se.copernicus.org/articles/15/639/2024/se-15-639-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/639/2024/se-15-639-2024-avatar-thumb80.png" data-caption="© Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/639/2024/se-15-639-2024-avatar-web.png" data-width="532" data-height="600" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 14 Jun 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/639/2024/">Rare Earth element distribution on the Fuerteventura Basal Complex (Canary Islands, Spain): a geochemical and mineralogical approach</a> <div class="authors">Marc Campeny, Inmaculada Menéndez, Luis Quevedo, Jorge Yepes, Ramón Casillas, Agustina Ahijado, Jorge Méndez-Ramos, and José Mangas</div> <div class="citation">Solid Earth, 15, 639–656, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-639-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-639-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_117652" data-show=".short_summary_117652" data-hide=".short_summary_button_117652" >Short summary</span> <div class="j-widget__max short_summary short_summary_117652" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The Basal Complex unit on Fuerteventura island comprises magmatic rocks showing significant rare Earth element (REE) concentrations with values up to 10 300 ppm REY (REEs plus yttrium). We carried out mineralogical and geochemical analyses, but additional research is needed to fully understand their distribution due to structural complexities and environmental factors. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_117652" data-show=".short_summary_button_117652">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://se.copernicus.org/articles/15/639/2024/se-15-639-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/639/2024/se-15-639-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/639/2024/se-15-639-2024-avatar-web.png" data-width="532" 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-1 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"> 13 Jun 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1668/">On the choice of finite element for applications in geodynamics. Part II: A comparison of simplex and hypercube elements</a> <div class="authors">Cedric Thieulot and Wolfgang Bangerth</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1668,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1668,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 3 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120794" data-show=".short_summary_120794" data-hide=".short_summary_button_120794" >Short summary</span> <div class="j-widget__max short_summary short_summary_120794" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> One of the main numerical methods in geodynamics is the finite-element method. Many types of elements have been used in the past decades in hundreds of publications. They usually fall under two categories: quadrilaterals and triangles. For the first time we compare results obtained with the most used elements of each type on a series of geodynamical benchmarks and draw conclusions as to which are the best ones and which are to be preferably avoided. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120794" data-show=".short_summary_button_120794">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-2 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"> 10 Jun 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1670/">Alternating Extensional and Contractional Tectonics in the West Kunlun Mountains during Jurassic: Responses to the Neo-Tethyan Geodynamics along the Eurasian Margin</a> <div class="authors">Hong-Xiang Wu, Han-Lin Chen, Andrew V. Zuza, Yildirim Dilek, Du-Wei Qiu, Qi-Ye Lu, Feng-Qi Zhang, Xiao-Gan Cheng, and Xiu-Bin Lin</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1670,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1670,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript under review for SE</span> <nobr>(discussion: final response, 6 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120796" data-show=".short_summary_120796" data-hide=".short_summary_button_120796" >Short summary</span> <div class="j-widget__max short_summary short_summary_120796" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The Tethyan Orogenic Belt documents an extensive history of subduction along the southern margin of Eurasia. This study examines the stratigraphy and provenance of Jurassic strata in the West Kunlun Mountains, highlighting the alternating extensional and contractional tectonic episodes in this region. We interpret that this complex evolution was related to the northward subduction of the Neo-Tethys Ocean, transitioning from southward retreat to northward flat-slab advancement. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120796" data-show=".short_summary_button_120796">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-2 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"> 06 Jun 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1602/">The structural anatomy of the Pyrenees examined through EMAG2v2 magnetic data</a> <div class="authors">África Gamisel-Muzás, Ruth Soto, Conxi Ayala, Tania Mochales, Félix Manuel Rubio, Pilar Clariana, Carmen Rey-Moral, and Juliana Martín-León</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1602,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1602,</span> 2024</div> <div class="statusMessage"><span>Revised manuscript under review for SE</span> <nobr>(discussion: final response, 5 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120576" data-show=".short_summary_120576" data-hide=".short_summary_button_120576" >Short summary</span> <div class="j-widget__max short_summary short_summary_120576" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> In this work we compare magnetic maps obtained from the EMAG2v2 (Earth Magnetic Anomaly Grid 2-arc-minute resolution) magnetic intensity data with the main geological structures and units of the Pyrenees and adjacent areas. The magnetic response arrangement for the different domains mimic the main structural lineaments and highlight the occurrence of major magnetic anomalies linked to specific geological bodies. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120576" data-show=".short_summary_button_120576">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="6"> <div class="grid-100 hide-on-desktop hide-on-tablet"> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 29 May 2024</div> <a class="article-title" target="_parent" href="https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1507/">Dislocation creep near the frictional-viscous transition in blueschist: experimental constraints</a> <div class="authors">Lonnie Justin Hufford, Leif Tokle, Whitney Maria Behr, Luiz Grafula Morales, and Claudio Madonna</div> <div class="citation">EGUsphere, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/egusphere-2024-1507,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/egusphere-2024-1507,</span> 2024</div> <div class="statusMessage"><span>Preprint under review for SE</span> <nobr>(discussion: final response, 4 comments)</nobr></div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_120386" data-show=".short_summary_120386" data-hide=".short_summary_button_120386" >Short summary</span> <div class="j-widget__max short_summary short_summary_120386" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> We constrained the rheology of glaucophane aggregates deforming near its brittle-ductile transition with general shear deformation experiments. In the experiments, glaucophane first underwent work hardening and strain weakening associated with brittle grain size reduction and incipient dislocation processes, then evolved to steady-state dislocation creep. We developed a flow law that can be used to approximate the rheological behavior of mafic oceanic crust at blueschist facies conditions. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_120386" data-show=".short_summary_button_120386">Hide</a></div> </div> </div> </div> <div class="grid-15 tablet-grid-15 text-right hide-on-mobile"> </div> </div>  <div class="pswp" tabindex="-1" role="dialog" aria-hidden="true" >  <div class="pswp__bg"></div>  <div class="pswp__scroll-wrap">  <div class="pswp__container"> <div class="pswp__item"></div> <div class="pswp__item"></div> <div class="pswp__item"></div> </div>  <div class="pswp__ui pswp__ui--hidden"> <div class="pswp__top-bar">  <div class="pswp__counter"></div> <button class="pswp__button pswp__button--close" title="Close (Esc)"></button> <button class="pswp__button pswp__button--fs" title="Toggle fullscreen"></button>   <div class="pswp__preloader"> <div class="pswp__preloader__icn"> <div class="pswp__preloader__cut"> <div class="pswp__preloader__donut"></div> </div> </div> </div> </div> <div class="pswp__share-modal pswp__share-modal--hidden pswp__single-tap"> <div class="pswp__share-tooltip"></div> </div> <button class="pswp__button pswp__button--arrow--left" title="Previous (arrow left)"> </button> <button class="pswp__button pswp__button--arrow--right" title="Next (arrow right)"> </button> <div class="pswp__caption "> <div class="pswp__caption__center"></div> </div> </div> </div> </div> <script> $(function (){ $('.recent-selection-wrapper button').click((event) => { event.preventDefault(); event.stopPropagation(); event.stopImmediatePropagation(); let currentElement = event.currentTarget; $("html, body").animate({ scrollTop: $('.breadcrumb').offset().top }, "slow"); return false; }); }); </script>  <a rel="license" style="display: none" href="https://creativecommons.org/licenses/by/4.0/">CC BY 4.0</a> <div> <a href="https://se.copernicus.org/by_ms_types.html?ms-type-id=58&selection=none" class="btn btn-primary">Check for further papers</a> </div> </div> </div>  </div> </div> </main>  <footer class="d-print-none version-2023"> <div class="footer"> <div class="container"> <div class="row align-items-center mb-3"> <div class="col-12 col-lg-auto text-center text-md-left title-wrapper"> <div id="j-header-footer" class="text-center text-md-left"> <div class="h1 text-center text-md-left"> Solid Earth </div> <p>An interactive open-access journal of the European Geosciences Union</p> </div> </div> <div class="col-12 col-lg-auto text-center text-md-left pt-lg-2"> <div class="row align-items-center"> <div class="col-12 col-sm col-md-auto text-center text-md-left mb-3 mb-sm-0"> <span class="egu-logo"><a href="http://www.egu.eu/" target="_blank"><img src="https://contentmanager.copernicus.org/319373/431/ssl" alt="" style="width: 410px; height: 325px;" /></a></span> </div> <div class="col-12 col-sm text-center text-md-left"> <span class="copernicus-logo"><a href="https://publications.copernicus.org/" target="_blank"><img src="https://contentmanager.copernicus.org/319376/431/ssl" alt="" style="width: 1784px; height: 330px;" /></a></span> </div> </div> </div> </div> </div> </div> <div class="links pb-4 pt-4"> <div class="container"> <div class="row align-items-center"> <div class="col-12 col-xl-auto mt-3"> <div class="row align-items-start align-items-lg-center"> <div class="col-12 mb-3 mb-md-0 pl-md-0 text-center text-md-left"><a href="https://creativecommons.org/licenses/by/4.0/" target="_blank"><i class="fab fa-creative-commons fa-lg mr-1"></i><i class="fab fa-creative-commons-by fa-lg"></i></a> All site content, except where otherwise noted, is licensed under the <a href="https://creativecommons.org/licenses/by/4.0/" target="_blank">Creative Commons Attribution 4.0 License</a>.</div> </div> </div> <div class="col-12 text-center text-md-left col-lg-auto mt-3"> <div class="row align-items-center"> <div class="col d-md-none px-0"></div> <div class="col-auto pr-1"><a href="https://www.solid-earth.net/about/contact.html">Contact</a></div> <div class="col-auto px-1">|</div> <div class="col-auto px-1"><a href="https://www.solid-earth.net/imprint.html">Imprint</a></div> <div class="col-auto px-1">|</div> <div class="col-auto px-1"><a href="https://www.copernicus.org/data_protection.html" target="_blank">Data protection</a></div> <div class="col-auto pl-2"><a class="twitter-follow-button" target="_blank" href="https://twitter.com/EGU_SEarth"><i class="fab fa-square-x-twitter fa-2x"></i></a></div> <div class="col d-md-none px-0"></div> </div> </div> </div> </div> </div> </footer> </body> </html>

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