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61.
Yun Jiang Piers Koefoed Olga Pravdivtseva Heng Chen Chun‐Hui Li Fang Huang Li‐Ping Qin Jia Liu Kun Wang 《Meteoritics & planetary science》2021,56(1):61-76
The alkali element K is moderately volatile and fluid mobile; thus, it can be influenced by both primary processes (evaporation and recondensation) in the solar nebula and secondary processes (thermal and aqueous alteration) in the parent body. Since these primary and secondary processes would induce different isotopic fractionations, K isotopes could become a potential tracer to distinguish them. Using recently developed methods with improved precision (0.05‰, 95% confidence interval), we systematically measured the K isotopic compositions and major/trace elemental compositions of chondritic components (18 chondrules, 3 CAIs, 2 matrices, and 5 bulks) in the carbonaceous chondrite fall Allende. Among all the components analyzed in this study, CAIs, which formed initially under high‐temperature conditions in the solar nebula and were dominated by nominally K‐free refractory minerals, have the highest K2O content (average 0.53 wt%) and have K isotope compositions most enriched in heavy isotopes (δ41K: ?0.30 to ?0.25‰). Such an observation is consistent with previous petrologic studies that show CAIs in Allende have undergone alkali enrichment during metasomatism. In contrast, chondrules contain lower K2O content (0.003–0.17 wt%) and generally lighter K isotope compositions (δ41K: ?0.87‰ to ?0.24‰). The matrix and bulks are nearly identical in K2O content and K isotope compositions (0.02–0.05 wt%; δ41K: ?0.62 to ? 0.46‰), which are, as expected, right in the middle of CAIs and chondrules. This strongly indicates that most of the chondritic components of Allende suffered aqueous alteration and their K isotopic compositions are the ramification of Allende parent‐body processing instead of primary nebular signatures. Nevertheless, we propose the small K isotope fractionations observed (< 1‰) among Allende components are likely similar to the overall range of K isotopic fractionation that occurred in nebular environment. Furthermore, the K isotope compositions seen in the components of Allende in this study are consistent with MC‐ICP‐MS analyses of the components in ordinary chondrites, which also show an absence of large (10‰) isotope fractionations. This is not expected as evaporation experiments in nebular conditions suggest there should be large K isotopic fractionations. Nevertheless, possible nebular processes such as chondrules back exchanging with ambient gas when they formed could explain this lack of large K isotopic variation. 相似文献
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Shengming Hu Zhijian Chen Chenghui Wan Chun Tang Wen Xiong 《Marine Georesources & Geotechnology》2020,38(4):385-392
AbstractCompared with traditional methods, the three-dimensional laser-scanning (3D-LS) technique can efficiently acquire many high-quality geometric properties of rock discontinuities. In practice, engineers usually prefer to simplify the processing by using single-station point data and roughly orienting owing to the complexity of registration/georeferencing multi-station point data. However, prior published studies have paid little attention to the accuracy and reliability when determining discontinuity orientations using 3D-LS. We propose a reliable and accurate method with robust on-site applicability. As part of an ongoing effort, we are evaluating the precision of the commonly used coarse registration method and the fine registration method, and promoted the optimized coarse- and fine-registration methods and evaluated their precision. It is found that: (1) the common and the optimized registration method can meet our project’s engineering requirements, and the optimized registration method improved accuracy in the dip direction by approximately 1°; (2) fine registration using an iterative closest point (ICP) algorithm can correct both dip direction and dip angle; and (3) the orientation is of high precision with commonly used coarse and fine registration, whereas the optimization effect to correct the orientation is slightly limited. 相似文献
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针对北斗卫星类型间偏差(ISTB)导致载波相位差分高精度定位(RTK)的整周模糊度无法固定问题,本文提出了改进ISTB快速改正方法,在观测量层面仅利用1组不同卫星类型的载波相位差分观测量即可实现ISTB估计与改正,实际应用中较传统方法更具普适性与简易性。该方法的测试结果表明,ISTB值由NH码调制不同引起,不同频点的ISTB值具有不一致性;此外,有无改正ISTB的北斗RTK性能对比反映了ISTB会严重降低整周模糊度固定与RTK定位性能。由此可知,本文方法能够保障现阶段北斗接收机更新换代过程中北斗RTK的高精度与高可靠性能。 相似文献
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Hedgehog信号通路参与动物神经系统发育、分节等诸多发育过程,研究该信号通路对理解动物的发育与演化机制有重要意义。对软体动物而言,目前Hedgehog信号通路的研究较少。本文克隆了腹足纲软体动物笠贝的hedgehog基因,利用整装原位杂交技术研究了其在胚胎发育过程中的时空表达规律;并与重要发育基因brachyury及soxb的表达模式进行了比较。结果表明,笠贝hedgehog基因与神经外胚层及中/内胚层相关,可能调控了幼虫神经、肌肉及消化道的分化。通过比较原肠胚及担轮幼虫不同阶段的基因表达模式,研究了hedgehog基因相关的组织和细胞随个体发育进程的动态变化。这些结果为理解软体动物形态发生和重要器官的分化机制提供了基础。 相似文献
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Sky surveys represent one of the most important efforts to improve developments in astrophysics,especially when using new photometric bands. We are performing the Stellar Abundance and Galactic Evolution(SAGE) survey with a self-designed SAGE photometric system, which is composed of eight photometric bands. The project mainly aims to study the stellar atmospheric parameters of ~0.5 billion stars in ~12 000 deg2 of the northern sky, which mainly focuses on Galactic astronomy, as well as some aspects of extragalactic astronomy. This work introduces the detailed data reduction process of the test field NGC 6791, including the data reduction of single-exposure images and stacked multi-exposure images, and properties of the final catalog. 相似文献
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足是软体动物最重要的器官之一,目前对其发育机制尚不了解。软体动物的足由神经和肌肉两部分构成,研究足部神经和肌肉系统在发育早期的的动态变化,对于了解足的形态建成机制具有重要意义。本文利用电镜研究了笠贝(Lottiagoshimai)足的早期发育过程。克隆了lgo-soxb和lgo-mox基因,整装原位杂交表明这两个基因分别表达在早期笠贝幼虫的神经外胚层和中胚层,可作为足发育过程的分子标记。不同发育阶段幼虫的原位杂交结果表明,神经外胚层和中胚层细胞在足发育的起始阶段尚未重叠,而在后续发育阶段,二者相向运动并重叠在一起。结果提示组成贝类足部的神经和肌肉细胞起源于早期胚胎不同的部位,在发育过程中逐渐互相接近并重叠,至担轮幼虫晚期共同作用形成足原基。本研究展示了足原基的早期形成过程,为深入研究软体动物足的发育机制提供了基础信息。 相似文献