Petrology and geochemistry of feldspathic impact‐melt breccia Abar al' Uj 012, the first lunar meteorite from Saudi Arabia          下载免费PDF全文

Marianna Mészáros  Beda A. Hofmann  Pierre Lanari  Randy L. Korotev  Edwin Gnos  Nicolas D. Greber  Ingo Leya  Richard C. Greenwood  A. J. Timothy Jull  Khalid Al‐Wagdani  Ayman Mahjoub  Abdulaziz A. Al‐Solami  Siddiq N. Habibullah 《Meteoritics & planetary science》2016,51(10):1830-1848

Abar al' Uj (AaU) 012 is a clast‐rich, vesicular impact‐melt (IM) breccia, composed of lithic and mineral clasts set in a very fine‐grained and well‐crystallized matrix. It is a typical feldspathic lunar meteorite, most likely originating from the lunar farside. Bulk composition (31.0 wt% Al₂O₃, 3.85 wt% FeO) is close to the mean of feldspathic lunar meteorites and Apollo FAN‐suite rocks. The low concentration of incompatible trace elements (0.39 ppm Th, 0.13 ppm U) reflects the absence of a significant KREEP component. Plagioclase is highly anorthitic with a mean of An_96.9Ab_3.0Or_0.1. Bulk rock Mg# is 63 and molar FeO/MnO is 76. The terrestrial age of the meteorite is 33.4 ± 5.2 kyr. AaU 012 contains a ~1.4 × 1.5 mm² exotic clast different from the lithic clast population which is dominated by clasts of anorthosite breccias. Bulk composition and presence of relatively large vesicles indicate that the clast was most probably formed by an impact into a precursor having nonmare igneous origin most likely related to the rare alkali‐suite rocks. The IM clast is mainly composed of clinopyroxenes, contains a significant amount of cristobalite (9.0 vol%), and has a microcrystalline mesostasis. Although the clast shows similarities in texture and modal mineral abundances with some Apollo pigeonite basalts, it has lower FeO and higher SiO₂ than any mare basalt. It also has higher FeO and lower Al₂O₃ than rocks from the FAN‐ or Mg‐suite. Its lower Mg# (59) compared to Mg‐suite rocks also excludes a relationship with these types of lunar material.  相似文献   

Geoeffective Disturbances in the Solar Wind near the Solar Activity Minimum according to the Data of a Two-year Series of Observations of Interplanetary Scintillations with the BSA LPI Radio Telescope     

Chashei  I. V.  Lebedeva  T. O.  Tyul’bashev  S. A.  Subaev  I. A. 《Astronomy Reports》2021,65(11):1150-1169

Astronomy Reports - A joint analysis of the monitoring data of interplanetary scintillations with solar and geophysical data showed that at the descending phase of the 24 solar activity cycle, the...  相似文献   

Coexisting Tetrahedrite–(Zn) and Sphalerite at the Teremki Gold-Ore Deposit (East Transbaikalia): Chemical Composition and Formation Conditions     

Lyubimtseva  N. G.  Prokof’ev  V. Yu.  Bortnikov  N. S. 《Geology of Ore Deposits》2021,63(5):454-464

Geology of Ore Deposits - Paragenetic associations of tetrahedrite-(Zn) and sphalerite are distinguished in the Teremki gold-ore deposit. The chemical composition of coexisting minerals of this...  相似文献   

Convergence acceleration of iterative sequences for equilibrium chemistry computations     

Nazer  Safaa Al  Jazar  Mustapha  Rosier  Carole 《Computational Geosciences》2021,25(5):1509-1538

Computational Geosciences - The modeling of thermodynamic equilibria leads to complex nonlinear chemical systems which are often solved with the Newton-Raphson method. But this resolution can lead...  相似文献   

Search for Periodic Emission from Five Gamma-Ray Pulsars at the Frequency of 111 MHz     

Tyul’bashev  S. A.  Kitaeva  M. A.  Tyulbasheva  G. E. 《Astronomy Reports》2021,65(9):819-825

Astronomy Reports - The search for pulsar (periodic) radiation of five gamma-ray pulsars was carried out using the summed power spectra and summed periodograms. No harmonics corresponding to the...  相似文献   

Causes and consequences of long-term groundwater overabstraction in Jordan     

Brückner  Florian  Bahls  Rebecca  Alqadi  Mohammad  Lindenmaier  Falk  Hamdan  Ibraheem  Alhiyari  Mohammad  Atieh  Ala’a 《Hydrogeology Journal》2021,29(8):2789-2802

Hydrogeology Journal - In 2017, a comprehensive review of groundwater resources in Jordan was carried out for the first time since 1995. The change in groundwater levels between 1995 and 2017 was...  相似文献   

鄂尔多斯盆地南缘中寒武统张夏组鲕粒滩相储层特征及主控因素     

李维岭  周进高  吴兴宁  吴东旭  王少依  丁振纯  于洲 《海相油气地质》2021,(1)

鄂尔多斯盆地寒武系深层具有良好的勘探潜力,中寒武统张夏组为寒武系勘探的重要目的层系。通过野外剖面详测和岩心、薄片观察及实验分析,对张夏组储层的特征、成因及主控因素进行了分析和研究,并预测了有利储层发育区。研究表明:①张夏组主要发育台缘鲕粒白云岩和台内鲕粒白云岩2类储层。②台缘带鲕粒滩累计厚度集中在50~300 m之间,鲕粒粒径平均为1.25 mm,鲕粒白云岩储集空间以溶蚀孔洞、粒间溶孔和晶间(溶)孔为主,平均测井孔隙度和渗透率分别为2.0%和0.038×10^-3μm²。③台内鲕粒滩厚度在50~120 m之间,鲕粒粒径平均为0.85 mm,鲕粒白云岩储集空间以溶蚀孔洞、粒间溶孔为主,平均测井孔隙度和渗透率分别为3.3%和2.787×10^-3μm²。④张夏组储层受鲕粒滩相、白云石化以及三级/四级层序界面控制,台缘规模有利储层发育在四级海退层序中上部的鲕粒白云岩地层中,台内规模有利储层发育在寒武系顶部不整合面之下的鲕粒白云岩地层中。预测台缘岐山—旬邑一带和台内陇东地区为两大规模有利储层发育区。  相似文献   

闪电产生氮氧化物对青藏高原臭氧低谷形成的影响     

郭凤霞  穆奕君  李扬  王曼霏  黄兆楚  曾凡辉  廉纯皓 《大气科学》2019,43(2):266-276

为了进一步了解青藏高原闪电的产生氮氧化物（LNO_x）经由光化学反应对O₃浓度变化及夏季O₃低谷形成的可能影响,本文利用2005~2013年由OMI卫星得到的对流层NO₂垂直浓度柱（NO₂ VCD）、O₃总浓度柱（TOC）和O₃廓线以及星载光学瞬变探测器OTD和闪电成像仪LIS获取的总闪电数资料,对青藏高原和同纬度长江中下游地区的TOC和NO₂ VCD月均值时空分布特征、闪电与NO₂ VCD的相关性和O₃的垂直分布特征及其与LNO_x的关系进行了对比分析。结果表明,青藏高原的O₃低谷主要出现在夏季和秋季,其TOC值比同纬度长江中下游地区低约10~15 DU（Dobson unit）。青藏高原NO₂VCD总体较小,表现为夏高冬低的分布特征。青藏高原夏季O₃浓度受南亚高压的影响总体呈减小趋势,但因强雷暴天气导致对流层中上部LNO_x浓度升高,并随强上升气流向对流层顶输送,同时通过光化学反应使O₃浓度增加,缩小了青藏高原和同纬度地区的O₃浓度差,减缓了O₃总浓度的下降,抑制了夏季O₃低谷的进一步深化。  相似文献   

济阳坳陷沾化凹陷邵家走滑—伸展断层带构造特征及其石油地质意义     

杨林龙  刘惠民  贾光华  穆星  孟涛  张波  王迪 《地质论评》2023,69(Z1):305-306

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新太阳光压模型在GNSS定轨中的应用     

常春涛  慕仁海  程鹏飞  成英燕 《测绘科学》2021,46(2):78-84

太阳光压摄动是影响卫星定轨中重要的误差源,在GNSS导航卫星精密定轨过程中使用最为广泛的光压模型为ECOM模型。为了探究几种ECOM模型及其适用性,该文以超快速星历为起算轨道,分析对比经典ECOM-1模型与最新13参数ECOMC模型对GPS/BDS卫星轨道的影响。结果显示:相较于ECOM-1模型,ECOMC模型在GPS定轨中精度有所提升,特别体现在径向精度提升,单天与三天弧段在径向的解算精度分别提升了12.73%和24.74%;在BDS定轨中,采用ECOMC模型,部分GEO卫星在径向方向单天精度有12.38%的提升,而对于IGSO与MEO卫星二者精度差异不大;分析可得,由于星体结构不对称引起卫星在沿太阳-卫星方向作用的偶数阶短周期谐波扰动,引入卫星-太阳方向偶数阶项的参数估计可提升卫星径向精度。  相似文献