Field Response of Magnetic Vortices in Dusty Olivine From the Semarkona Chondrite

Nichols Claire I. O.; Einsle Joshua F.; Im Mi‐Young; Kasama Takeshi; Saghi Zineb; Midgley Paul A.; Harrison Richard J.

摘要

Abstract >Recent paleomagnetic studies have constrained the strength and longevity of the magnetic field generated by the solar nebula, which has broad implications for the early evolution of the solar system. Paleomagnetic evidence was recorded by nanoscale iron inclusions in olivine crystals in the Semarkona LL 3.0 chondrite. These dusty olivines have been shown to be credible carriers of ancient magnetic remanence. The small scale of the iron inclusions presents several challenges for defining their fundamental magnetic properties. Here we present the first correlative study of the response of these magnetic structures under applied laboratory fields. Results show that the majority of particles are in a single‐vortex state and exhibit stable magnetic behavior in applied fields up to 200?mT. Experimental observations using Lorentz microscopy and magnetic transmission X‐ray microscopy are shown to compare well with the results of finite‐element micromagnetic simulations derived from 3‐D models of the particles obtained using electron tomography. This correlative approach may be used to characterize the fundamental magnetic behavior of many terrestrial and extraterrestrial paleomagnetic carriers in the single‐vortex to multivortex size range, which represent the vast majority of stable magnetic carriers in rocks and meteorites. </abstract> </span> <span class="z_kbtn z_kbtnclass hoverxs" style="display: none;">展开▼</span> </div> <div class="translation abstracttxt"> <span class="zhankaihshouqi fivelineshidden" id="abstract"> <span>机译：</span><Abstract Type =“main”XML：Lang =“en”XML：ID =“GGGE21828-ABS-0001”> <标题类型=“main”>抽象</ title> <P>最近的古磁性研究已经限制了太阳星云产生的磁场的强度和寿命，这对太阳系的早期演变具有广泛的影响。古磁证据通过南斯科纳LL 3.0 Chondrite中的橄榄石晶体中的纳米级铁夹杂物记录。这些尘土飞扬的橄榄石已被证明是古代磁性遗弃的可信载体。铁夹杂物的小规模呈现了定义其基本磁性的几个挑战。在这里，我们介绍了应用实验室领域这些磁性结构响应的第一个相关研究。结果表明，大多数颗粒处于单涡流状态，并且在施加的场中表现出高达200μmt的稳定磁性。使用洛伦兹显微镜和磁传动X射线显微镜的实验观察结果与使用电子断层扫描获得的颗粒的3-D模型的有限元微磁模拟的结果相比很好。这种相关性方法可用于表征单涡流中许多陆地和外星古磁性磁携带者的基本磁力，以多想大小范围，这代表了岩石和陨石中绝大多数稳定的磁性载体。</ p> </摘要> </span> <span class="z_kbtn z_kbtnclass hoverxs" style="display: none;">展开▼</span> </div> </div> <div class="record"> <h2 class="all_title" id="enpatent33" >著录项</h2> <ul> <li> <span class="lefttit">来源</span> <div style="width: 86%;vertical-align: text-top;display: inline-block;"> <a href='/journal-foreign-23285/'>《Geochemistry, geophysics, geosystems》</a> <b style="margin: 0 2px;">|</b><span>2019年第3期</span><b style="margin: 0 2px;">|</b><span>共13页</span> </div> </li> <li> <div class="author"> <span class="lefttit">作者</span> <p id="fAuthorthree" class="threelineshidden zhankaihshouqi"> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Nichols Claire I. O.&option=202" target="_blank" rel="nofollow">Nichols Claire I. O.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Einsle Joshua F.&option=202" target="_blank" rel="nofollow">Einsle Joshua F.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Im Mi‐Young&option=202" target="_blank" rel="nofollow">Im Mi‐Young;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Kasama Takeshi&option=202" target="_blank" rel="nofollow">Kasama Takeshi;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Saghi Zineb&option=202" target="_blank" rel="nofollow">Saghi Zineb;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Midgley Paul A.&option=202" target="_blank" rel="nofollow">Midgley Paul A.;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Harrison Richard J.&option=202" target="_blank" rel="nofollow">Harrison Richard J.;</a> </p> <span class="z_kbtnclass z_kbtnclassall hoverxs" id="zkzz" style="display: none;">展开▼</span> </div> </li> <li> <div style="display: flex;"> <span class="lefttit">作者单位</span> <div style="position: relative;margin-left: 3px;max-width: 639px;"> <div class="threelineshidden zhankaihshouqi" id="fOrgthree"> <p>Department of Earth SciencesUniversity of CambridgeCambridge UK;</p> <p>Department of Earth SciencesUniversity of CambridgeCambridge UK;</p> <p>Center for X‐ray OpticsLawrence Berkeley National LaboratoryBerkeley CA USA;</p> <p>National Centre for Nano Fabrication and CharacterisationTechnical University of DenmarkKongens Lyngby Denmark;</p> <p>Department of Materials Science and MetallurgyUniversity of CambridgeCambridge UK;</p> <p>Department of Materials Science and MetallurgyUniversity of CambridgeCambridge UK;</p> <p>Department of Earth SciencesUniversity of CambridgeCambridge UK;</p> </div> <span class="z_kbtnclass z_kbtnclassall hoverxs" id="zhdw" style="display: none;">展开▼</span> </div> </div> </li> <li > <span class="lefttit">收录信息</span> <span style="width: 86%;vertical-align: text-top;display: inline-block;"></span> </li> <li> <span class="lefttit">原文格式</span> <span>PDF</span> </li> <li> <span class="lefttit">正文语种</span> <span>eng</span> </li> <li> <span class="lefttit">中图分类</span> <span><a href="https://www.zhangqiaokeyan.com/clc/163.html" title="地球物理学">地球物理学;</a></span> </li> <li class="antistop"> <span class="lefttit">关键词</span> <p style="width: 86%;vertical-align: text-top;"> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=rock magnetism&option=203" rel="nofollow">rock magnetism;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=microscopy&option=203" rel="nofollow">microscopy;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=dusty olivine&option=203" rel="nofollow">dusty olivine;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=solar nebula&option=203" rel="nofollow">solar nebula;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=meteorite&option=203" rel="nofollow">meteorite;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=correlative study&option=203" rel="nofollow">correlative study;</a> </p> <div class="translation"> 机译：岩石磁性;显微镜;尘土飞扬的橄榄石;太阳星云;陨石;相关研究; </div> </li> </ul> </div> </div> <div class="literature cardcommon"> <div class="similarity "> <h3 class="all_title" id="enpatent66">相似文献</h3> <div class="similaritytab clearfix"> <ul> <li class="active" >外文文献</li> <li >中文文献</li> <li >专利</li> </ul> </div> <div class="similarity_details"> <ul > <li> <div> <b>1. </b><a class="enjiyixqcontent" href="/journal-foreign-detail/0704023360291.html">Field Response of Magnetic Vortices in Dusty Olivine From the Semarkona Chondrite</a> <b>[J]</b> . <span> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Nichols Claire I. 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