SE - Recent

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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; } #templateSearchLoadingModal .co_LoadingDotsContainer .text { text-align: center; font-weight: bold; padding-bottom: 1rem; } #templateSearchLoadingModal .co_LoadingDotsContainer .dot { background-color: #0072BC; border: 2px solid white; border-radius: 50%; float: left; height: 2rem; width: 2rem; margin: 0 5px; -webkit-transform: scale(0); transform: scale(0); -webkit-animation: animation_dots_breath 1000ms ease infinite 0ms; animation: animation_dots_breath 1000ms ease infinite 0ms; } #templateSearchLoadingModal .co_LoadingDotsContainer .dot:nth-child(2) { -webkit-animation: animation_dots_breath 1000ms ease infinite 300ms; animation: animation_dots_breath 1000ms ease infinite 300ms; } #templateSearchLoadingModal .co_LoadingDotsContainer .dot:nth-child(3) { -webkit-animation: animation_dots_breath 1000ms ease infinite 600ms; animation: animation_dots_breath 1000ms ease infinite 600ms; } #templateSearchResultModal [class*="grid-"] { padding-left: 10px !important; padding-right: 10px !important; } #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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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="漏 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="漏 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="漏 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="漏 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="漏 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, T眉rkiye</a> <div class="authors">Berkan 脰zkan, 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="漏 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="漏 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="漏 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="漏 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="漏 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, J眉rgen Adam, Elham Jonade, Silvia Negr茫o, 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-M眉ller, Adam W艂odek, Simon J. Cuthbert, and Jaros艂aw 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/15/1241/2024/se-15-1241-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1241/2024/se-15-1241-2024-avatar-thumb80.png" data-caption="漏 Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-web="https://se.copernicus.org/articles/15/1241/2024/se-15-1241-2024-avatar-web.png" data-width="600" data-height="350" width="80" height="80"> </a> </div> <div class="grid-85 tablet-grid-85"> <div class="published-date"> 07 Oct 2024</div> <a class="article-title" target="_parent" href="https://se.copernicus.org/articles/15/1241/2024/">ECOMAN: an open-source package for geodynamic and seismological modelling of mechanical anisotropy</a> <div class="authors">Manuele Faccenda, Brandon P. VanderBeek, Albert de Montserrat, Jianfeng Yang, Francesco Rappisi, and Neil Ribe</div> <div class="citation">Solid Earth, 15, 1241–1264, <nobr class="hide-on-mobile hide-on-tablet">https://doi.org/10.5194/se-15-1241-2024,</nobr><span class="hide-on-desktop">https://doi.org/10.5194/se-15-1241-2024,</span> 2024</div> <span class="show-hide journal-contentLinkColor triangle short_summary_button_117884" data-show=".short_summary_117884" data-hide=".short_summary_button_117884" >Short summary</span> <div class="j-widget__max short_summary short_summary_117884" style="display: none"> <div class="widget dark-border"> <div class="legend journal-contentLinkColor">Short summary</div> <div class="content"> The Earth's internal dynamics and structure can be well understood by combining seismological and geodynamic modelling with mineral physics, an approach that has been poorly adopted in the past. To this end we have developed ECOMAN, an open-source software package that is intended to overcome the computationally intensive nature of this multidisciplinary methodology and the lack of a dedicated and comprehensive computational framework. </div> <div><a href="#" class="show-hide triangle" data-hide=".short_summary_117884" data-show=".short_summary_button_117884">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/15/1241/2024/se-15-1241-2024-avatar-web.png"> <img class="img-responsive" src="https://se.copernicus.org/articles/15/1241/2024/se-15-1241-2024-avatar-thumb80.png" data-web="https://se.copernicus.org/articles/15/1241/2024/se-15-1241-2024-avatar-web.png" data-width="600" data-caption="漏 Author(s). Distributed under the Creative Commons Attribution 4.0 License." data-height="350" 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/15/1233/2024/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="漏 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="漏 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="漏 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="漏 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="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> </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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