关中盆地浅层地热能赋存规律及资源量估算     

周阳  洪增林  张卉  曹晓凡  穆根胥 《中国地质调查》2020,7(2):21-29

通过野外地质调查及室内综合研究,分析了关中盆地浅层地热能的开发利用情况、赋存特征和形成模式,并对资源量进行了估算,总结了盆地不同地貌单元、不同岩性的岩土体热物性参数特征,计算了区域恒温带深度和浅层大地热流值。关中盆地地热能的形成模式主要为热传导型和热对流型: 热传导型地热资源主要分布于西安凹陷、固市凹陷等完整地质块体内; 热对流型地热资源主要分布于深大断裂直接沟通地表的区域以及断裂带周边区域。采用层次分析法对关中盆地浅层地热能进行适宜性分区,认为关中盆地整体属于地埋管地源热泵系统适宜区或较适宜区,地下水地源热泵系统适宜区和较适宜区主要分布在盆地中部漫滩区和阶地区。利用热储法,计算关中盆地浅层地热能热容量为1.38×10¹⁶ kJ/℃,浅层地热能储量巨大,开发利用前景优良。  相似文献   

Solar System Collisions with Dense Interstellar Gas Clouds and Radiocarbon Traces of Periods with “Abnormally Low” Solar Modulation of Cosmic Rays     

Vasil’ev  G. I.  Konstantinov  A. N.  Kudryavtsev  I. V.  Ogurtsov  M. G.  Ostryakov  V. M.  Pavlov  A. K.  Frolov  D. A. 《Geomagnetism and Aeronomy》2019,59(8):1075-1080

Geomagnetism and Aeronomy - The causes of a sharp increase in the radiocarbon content in the Earth’s atmosphere for periods with abnormally low solar modulation of galactic cosmic rays (GCRs)...  相似文献   

Classification of Harmonic Functions in the Exterior of a Unit Sphere and Its Application to the Description of the External Magnetic Field of the Earth     

Akhmet’ev  P. M.  Petrov  A. V. 《Geomagnetism and Aeronomy》2019,59(6):752-760

Geomagnetism and Aeronomy - The magnetic fields of a subterranean source observed on the Earth’s surface or from the orbit of a satellite are studied. We analyze the space of all harmonic...  相似文献   

On the Question of Calculating the Parameters of Vortices in the Near-Surface Atmosphere of Mars     

Izvekova  Yu. N.  Popel’  S. I.  Izvekov  O. Ya. 《Solar System Research》2019,53(6):423-430

Solar System Research - The paper is dedicated to the study of dust vortices on the Earth and Mars. The hydrodynamic similarity of convective vortices is considered, and the similarity criteria are...  相似文献   

大数据驱动下的数字古地理重建：现状与展望     

张蕾  钟瀚霆  陈安清  赵应权  黄可可  李凤杰  黄虎  刘宇  曹海洋  祝圣贤  穆财能  侯明才  JAMES G. Ogg 《高校地质学报》2020,26(1):73

古地理学是一门强数据依赖性学科,古地理重建作为古地理学的核心任务之一,着眼于研究地质历史时期地球表面的地理、生物、气候面貌及其演化规律。随着大数据时代的来临,海量古地理数据的不断积累和计算机技术的高速发展使得标准化、智能化的数字古地理重建成为可能。文章通过介绍国内外与古地理相关的代表数据库及团队,总结其优缺点,提出大数据驱动下的数字古地理重建核心思路:(1)建立标准化的古地理学知识体系;(2)建立开放互动、动态更新的古地理数据库,并利用机器阅读技术等拓展数据来源;(3)建立标准化的古地理学数据质量控制体系;(4)利用机器学习技术建立各类型古地理重建模型,深度挖掘数据;(5)以可实时更新的智能数字地图集或多维动画形式输出成果。  相似文献   

Optical archival spectra of blazar candidates of uncertain type in the 3rd Fermi Large Area Telescope Catalog     

N. Álvarez Crespo  F. Massaro  R. D’Abrusco  M. Landoni  N. Masetti  V. Chavushyan  E. Jiménez-Bailón  F. La Franca  D. Milisavljevic  A. Paggi  V. Patiño-Álvarez  F. Ricci  Howard A. Smith 《Astrophysics and Space Science》2016,361(9):316

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Tilt Angles of Solar Filaments over the Period of 1919 – 2014     

Andrey G. Tlatov  Kirill M. Kuzanyan  Valeria V. Vasil’yeva 《Solar physics》2016,291(4):1115-1127

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Analytical Model of an Asymmetric Sunspot with a Steady Plasma Flow in its Penumbra     

A. A. Solov’ev  E. A. Kirichek 《Solar physics》2016,291(6):1647-1663

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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   

Effects of seismic force and pore water pressure on stability of 3D unsaturated hillslopes     

Wang  Long  Liu  Wenhua  Hu  Wei  Li  Wugang  Sun  De’an 《Natural Hazards》2021,105(2):2093-2116

Natural Hazards - Three-dimensional (3D) kinematic limit analysis of unsaturated hillslopes is presented in this paper. Different from the traditional two-dimensional (2D) mechanism based on the...  相似文献