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91.
We use quantitative microstructural analysis including misorientation analysis based on electron backscatter diffraction (EBSD) data to investigate deformation mechanisms of naturally deformed plagioclase in an amphibolite gabbro mylonite. The sample is from lower oceanic crust exposed near the Southwest Indian Ridge, and it has a high ratio of recrystallized matrix grains to porphyroclasts. Microstructures preserved in porphyroclasts suggest that early deformation was achieved principally by dislocation creep with subgrain rotation recrystallization; recrystallized grain (average diameter ∼8 μm) microstructures indicate that subsequent grain boundary sliding (GBS) was active in the continued deformation of the recrystallized matrix. The recrystallized matrix shows four-grain junctions, randomized misorientation axes, and a shift towards higher angles for neighbor-pair misorientations, all indicative of GBS. The matrix grains also exhibit a shape preferred orientation, a weak lattice preferred orientation consistent with slip on multiple slip systems, and intragrain microstructures indicative of dislocation movement. The combination of these microstructures suggest deformation by dislocation-accommodated GBS (DisGBS). Strain localization within the recrystallized matrix was promoted by a transition from grain size insensitive dislocation creep to grain size sensitive GBS, and sustained by the maintenance of a small grain size during superplasticity.  相似文献   
92.
利用基于TEC的电子密度廓线反演方法,对2014年12月31日的COSMIC和FY-3C掩星任务的电离层掩星相位数据进行处理,将反演的电子密度廓线及电离层峰值参数分别与两个掩星任务的官方产品进行比较,发现两个掩星任务的反演结果与官方产品均具有较好的一致性.其中COSMIC反演结果与CDAAC官方产品的一致性略好于FY-3C反演结果与NSMC官方产品的一致性,且两个任务的NmF2的反演质量均优于hmF2的反演质量.但与COSMIC不同,FY-3C掩星电离层相位数据进行反演处理之前有必要进行滤波平滑预处理,且由于FY-3C非掩星时段的相位数据量太少,反演过程中不建议对TEC进行改正.  相似文献   
93.
Five Plio-Pleistocene to Holocene aeolian quartz samples from the coastal dune deposits of the Wilderness-Knysna area (South Africa) previously dated by OSL were selected for ESR dating. Samples were processed following the Multiple Centre approach and using the Multiple Aliquot Additive dose method. Aluminium (Al) and Titanium (Ti) signals were systematically measured in all samples.Our study shows that ESR results obtained for Middle Pleistocene to Holocene samples may be strongly impacted by (i) the presence of a significant high frequency noise in the ESR spectra acquired for the Ti signals and (ii) the choice of the fitting function employed. In particular, if not taken into account, very noisy spectra can lead to a significant overestimation of the true ESR intensity measured for the Ti–H signal. These sources of uncertainty are however not sufficient to remove the ESR age overestimations. Consequently, our results indicate that the Al and Ti ESR signals of these quartz samples have not been fully reset during their aeolian transport.While this work contributes to improve our understanding of the ESR method applied to quartz grains, and especially of the potential and limitations of the Ti signals, it also provides additional baseline data to illustrate the existing variability among quartz samples of different origins or sedimentary context. Our results are consistent with previous studies by confirming that the Ti–H signal shows the best potential for the evaluation of low dose values (<100 Gy for these samples), whereas it becomes inappropriate for the higher dose range, and the Ti–Li–H (option D sensu Duval and Guilarte, 2015) should be used instead.Beyond the methodological outcome, this ESR dating study also provides a useful addition to the existing chronology of the aeolian deposits in this region. In particular, new (and possibly) finite numerical age results were obtained for the two oldest samples, constraining the aeolianite landward barrier dune and the coversand formations to the MIS 10-8 and Pliocene, respectively.  相似文献   
94.
石榴石是最重要的造岩矿物之一,通常能够保留早期的矿物结构和物质并记录较为晚期的变形和变质反应。石榴石钇(Y)元素环带特征丰富、复杂,不同的环带特征通常暗示不同的形成环境或经历了不同的变质事件,是变质演化历史研究的重要媒介之一。以往的研究中,多以LA-ICP-MS作为石榴石Y元素的主要分析手段,EPMA主要用于主量元素的分析。但是,LA-ICP-MS的束斑尺寸(44μm)和基底效应较EPMA(0~5μm)大,当石榴石颗粒小、包体和裂隙发育或成分环带以微区尺寸内存在较大变化时,大束斑更容易覆盖某些特殊信息。通过对石榴石Y元素测试参数的调试和标样验证,最终确定峰位测试时长和背景测试时长分别为140s和70s,并进行了PHA谱峰干扰剥离,降低检测限至54×10^(-6)。本文将通过对比佛子岭石榴云母片岩(LD025)4颗石榴石的EPMA主、微量原位分析(Ca、Mg、Mn、Fe、Y、Al、Si、Cr、Ti、Na)和LA-ICP-MS石榴石Y元素分析结果,论证EPMA分析Y元素的可行性。石榴石X-ray Mapping和主量成分剖面揭示该4颗石榴石均为生长环带,Mn呈钟形分带,Y与X Sps呈强烈正相关性,与X Grs、X Alm、X Prp相关性不清晰。EPMA和LA-ICP-MS分析结果显示Y含量曲线在核部和幔部具有良好的一致性,Grt1~Grt3中Y均表现出自核部(500×10^(-6)~1200×10^(-6))向幔部(200×10^(-6)~500×10^(-6))逐渐降低,极边部Y含量低(20×10^(-6)~200×10^(-6))且变化复杂;Grt4中Y含量差异相对较小(180×10^(-6)~450×10^(-6)),仅在边部出现不同程度的升降。因EPMA对于Y元素含量较低(<200×10^(-6))时灵敏度不够或者LA-ICP-MS束斑尺寸大容易掩盖边部窄带成分真实变化等原因,二者在边部Y元素差异较大。分别对EPMA和LA-ICP-MS的分析结果应用Grt-Xtm温度计和Grt单矿物压力计获得的变质PT结果显示Grt1~Grt3(核-幔-边)和Grt4(核-边)均记录较为完整、统一的温压演化过程。M1→M2→M3的变质温压变化分别为T=530~544℃、P=0.78~0.82GPa→T=577~616℃、P=0.89~0.98GPa→T=631~661℃、P=1.01~1.07GPa,表现为顺时针演化型式,M1至M3反映的是一个“暖俯冲”过程。根据温度评价结果,Grt1~Grt3(1.2~1.4mm,自形程度高)形成时间应早于Grt4(0.8mm,自形程度低)。由此可知,大颗粒的石榴石Y元素含量及变化特征通常更容易揭示相对完整的变质演化历史。本次研究为变泥质岩演化历史、变质温压评价等研究提供了不同视角和思路,结合EPMA主量(矿物成分、X-ray mapping、BSE分析)和微量元素(Y等)分析能够更加精准、全面地解读地质信息。  相似文献   
95.
96.
对含碲金矿中碲化物物相组成和元素赋存特征开展系统的研究,有助于对此类金矿矿床成因的理解和找矿勘查工作。山东金青顶金矿床伴生的碲化物由于碲化物颗粒较小,不易被发现,以往的研究缺乏对碲化物元素分布的精细刻画。本文通过电子探针背散射图像、波谱分析、能谱分析结合面扫描技术对金青顶金矿床碲化物进行了分析,研究碲化物的种类、共生关系、化学成分以及元素分布特征等。结果表明:碲金银矿与碲银矿密切共生,常形成连生体,Au、Ag在连生体中不均匀分布,面扫描图局部可见碲金矿亮斑;Te总是优先和Ag结合,生成碲银矿,随着Ag的消耗碲金银矿开始出现,Ag被耗尽后Te与Au生成碲金矿,成矿后期热液中多余的金与碲金银矿或碲银矿反应生成非常规碲化物(如本文发现的Ag2.95Au1.83Te),当Te消耗完后生成自然金;金银矿物的生长顺序是碲银矿—碲金银矿—碲金矿—自然金。本研究为含碲金矿的综合利用提供了技术支持。  相似文献   
97.
利用一维三分量完全电磁粒子模拟方法研究了由温度各向异性电子束流和电于环束流引起电磁辐射特征,结果表明它们都能激发高频宽带电磁不稳定性,其中环束流不稳定性(RBI)的非线性饱和水平比温度各向异性束流不稳定性(TABI)强,对RBI波在系统发展的线性增长阶段呈右旋极化,在非线性饱和阶段则主要呈左旋极化,而对TABI波在系统发展的整个阶段均享右旋极化.这些结果可应用于磁化星磁层射电暴的解释中.  相似文献   
98.
国内外寻找隐伏矿化探新方法研究进展   总被引:15,自引:2,他引:13       下载免费PDF全文
简要总结了根据超显微镜物质的迁移吸附机制和矿物结构与成矿物关系寻找隐伏矿的化探新方法的原理,技术及试验应用效果,预计这些方法技术近期内在寻找隐伏矿及解决环境,地震预报,地热工发等研究领域发挥重要作用。  相似文献   
99.
Examples of data from DE-2 satellite instruments are presented. These illustrate the behaviour of plasma parameters in the F-region and adjacent topside ionosphere during rapid sub-auroral ion drift (SAID) events. In particular, a variety of behaviours of the electron temperature (Te) is demonstrated, both within and equatorward of the SAID region. The Sheffield University plasmasphere-ionosphere model (SUPIM) is used to perform calculations in which a model SAID is applied to a plasma flux tube. The model results indicate that strongly elevated ion temperature (a recognised signature of SAID events) is on occasion sufficient to raise Te to observed values by ion-electron heat transfer. On other occasions, an additional heat source is required. It is suggested that such a source for the electron gas may be due to interaction between the ring current and the plasmasphere at high altitudes. The magnitude of the downward heat flux is consistent with that necessary to produce sub-auroral red arcs. The resulting strongly heated electron gas causes vibrational excitation of molecular nitrogen in the thermosphere.  相似文献   
100.
Shale gas is a resource of emerging importance in the energy field. Many countries in the world have been making big financial investments in this area. Carboniferous shale in the eastern Qaidam Basin shows good exploration prospects, but limited research and exploration work for shale oil and gas resources has been undertaken. Geochemical analyses were performed on shale derived from the Upper Carboniferous Hurleg Formation in the eastern Qaidam Basin, Qinghai Province, and secondary electron imaging capability of a Field Emission scanning electron microscope(FE-SEM) was used to characterize the microstructure of the shale. The reservoir and exploitation potential of the studied shale was assessed by comparison with research results obtained from the Barnett Formation shale in Fort Worth Basin, North America and the Basin shale of Sichuan province. The results indicate that the eastern Qaidam Basin Carboniferous shale is high-quality source rock. There are four major microstructural types in the study area: matrix intergranular pores, dissolution pores, intergranular pores, and micro-fractures. The size of the micropores varies from 6–633 nm, the majority of which is between 39–200 nm, with a relatively small number of micro-scale pores ranging from 0.13–1 μm. The pore characteristics of the studied shales are similar to the North American and Sichuanese shales, indicating that they have good reservoir potential. No micropores are present in the organic matter, which is induced by its composition; instead we found an important lamellar structure in the organic matter. These micropores and microfractures are abundant, and are connected to natural visible cracks that form the network pore system, which controls the storage and migration of shale gas. This connectivity is favorable for shale gas exploitation, providing great scientific potential and practical value.  相似文献   
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