首页> 外文期刊>Journal of geophysical research. Solid earth: JGR >Shock Compression and Melting of an Fe‐Ni‐Si Alloy: Implications for the Temperature Profile of the Earth's Core and the Heat Flux Across the Core‐Mantle Boundary
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Shock Compression and Melting of an Fe‐Ni‐Si Alloy: Implications for the Temperature Profile of the Earth's Core and the Heat Flux Across the Core‐Mantle Boundary

机译:Fe-Ni-Si合金的冲击压缩和熔化:对地球核心温度曲线的影响以及核心地幔边界的热量

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Abstract > Understanding the melting behavior and the thermal equation of state of Fe‐Ni alloyed with candidate light elements at conditions of the Earth's core is critical for our knowledge of the region's thermal structure and chemical composition and the heat flow across the liquid outer core into the lowermost mantle. Here we studied the shock equation of state and melting curve of an Fe‐8?wt% Ni‐10?wt% Si alloy up to ~250?GPa by hypervelocity impacts with direct velocity and reliable temperature measurements. Our results show that the addition of 10?wt% Si to Fe‐8?wt% Ni alloy slightly depresses the melting temperature of iron by ~200–300?(±200)?K at the core‐mantle boundary (~136?GPa) and by ~600–800?(±500)?K at the inner core‐outer core boundary (~330?GPa), respectively. Our results indicate that Si has a relatively mild effect on the melting temperature of iron compared with S and O. Our thermodynamic modeling shows that Fe‐5?wt% Ni alloyed with 6?wt% Si and 2?wt% S (which has a density‐velocity profile that matches the outer core's seismic profile well) exhibits an adiabatic profile with temperatures of ~3900?K and ~5300?K at the top and bottom of the outer core, respectively. If Si is a major light element in the core, a geotherm modeled for the outer core indicates a thermal gradient of ~5.8–6.8?(±1.6)?K/km in the <fi>D</fi> ″ region and a high heat flow of ~13–19?TW across the core‐mantle boundary. </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”> <标题类型=“main”>抽象</ title> >了解熔化行为和使用候选光元素的Fe-Ni状态的热方程在地球的核心条件下,对于我们对该地区的热结构和化学成分以及液体外芯的热流进入最低地幔,这是至关重要的。在这里,我们研究了Fe-8的状态和熔化曲线的冲击方程,其Fe-8?WT%的Si合金高达〜250〜250〜250°GPA,通过直接速度和可靠的温度测量。我们的结果表明,加入10〜Wt%Si至Fe-8吗?wt%Ni合金略微按压铁的熔化温度〜200-300?(±200)?核心 - 地幔边界(〜136? GPA)分别在内核 - 外部核心边界(〜330〜GPA)处〜600-800?(±500)?k。我们的结果表明,与S和O的热力学建模相比,Si对铁的熔化温度效果相对轻微。我们的热力学建模表明Fe-5?WT%Ni用6〜wt%Si和2?wt%s(其中与外芯的地震型材匹配良好的密度 - 速度曲线分别与外核的顶部和底部的温度呈绝热曲线。如果Si是核心中的主要光元件,则为外部核心建模的地热梯度表示<fi> d </ fi>“区域和a中的〜5.8-6.8?(±1.6)?k / km高热流动〜13-19?TW贯穿芯边界。 </ p> </ abstract> </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-34677/'>《Journal of geophysical research. Solid earth: JGR》</a> <b style="margin: 0 2px;">|</b><span>2018年第2期</span><b style="margin: 0 2px;">|</b><span>共14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=Zhang Youjun&option=202" target="_blank" rel="nofollow">Zhang Youjun;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Sekine Toshimori&option=202" target="_blank" rel="nofollow">Sekine Toshimori;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Lin Jung‐Fu&option=202" target="_blank" rel="nofollow">Lin Jung‐Fu;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=He Hongliang&option=202" target="_blank" rel="nofollow">He Hongliang;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Liu Fusheng&option=202" target="_blank" rel="nofollow">Liu Fusheng;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Zhang Mingjian&option=202" target="_blank" rel="nofollow">Zhang Mingjian;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Sato Tomoko&option=202" target="_blank" rel="nofollow">Sato Tomoko;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Zhu Wenjun&option=202" target="_blank" rel="nofollow">Zhu Wenjun;</a> <a href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=Yu Yin&option=202" target="_blank" rel="nofollow">Yu Yin;</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>Center for High Pressure Science and Technology Advanced Research (HPSTAR)Shanghai China;</p> <p>Center for High Pressure Science and Technology Advanced Research (HPSTAR)Shanghai China;</p> <p>Center for High Pressure Science and Technology Advanced Research (HPSTAR)Shanghai China;</p> <p>National Key Laboratory of Shock Wave and Detonation PhysicsChina Academy of Engineering PhysicsMianyang China;</p> <p>College of Physical Science and TechnologySouthwest Jiaotong UniversityChengdu China;</p> <p>College of Physical Science and TechnologySouthwest Jiaotong UniversityChengdu China;</p> <p>Department of Earth and Planetary Systems ScienceHiroshima UniversityHigashihiroshima Japan;</p> <p>National Key Laboratory of Shock Wave and Detonation PhysicsChina Academy of Engineering PhysicsMianyang China;</p> <p>National Key Laboratory of Shock Wave and Detonation PhysicsChina Academy of Engineering PhysicsMianyang China;</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=Earth's core&option=203" rel="nofollow">Earth's core;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=light elements&option=203" rel="nofollow">light elements;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=core‐mantle boundary&option=203" rel="nofollow">core‐mantle boundary;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=heat flow&option=203" rel="nofollow">heat flow;</a> <a style="color: #3E7FEB;" href="/search.html?doctypes=4_5_6_1-0_4-0_1_2_3_7_9&sertext=geotherm&option=203" rel="nofollow">geotherm;</a> </p> <div class="translation"> 机译:地球的核心;光元素;核心地幔边界;热流;地热; 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