张北地震前地壳形变异常及力学分析   总被引：2，自引：2，他引：0  

陈绍绪  张跃刚  丁瑞同  吴晓岚 《大地测量与地球动力学》2003,23(4):5-8

1998年 1月河北省张北 6 .2级地震前 ,在震中区西部存在一个幅度为 2 0mm的隆起异常区 ,震后异常恢复。根据张北地区 1984～ 1991年的水准测量资料 ,反演地震孕育期间的力学参数 ,结果显示震源区受力增加了32× 10 14 N ;力系中心位置为 4 0 .99°N ,113.99°E ,力系的方位角α =2 8.6 5°,力系的倾角 β =- 17.19° ,与后来实际发生地震的震中及震源机制十分接近 ,与华北地区区域应力场也基本一致。理论形变图与实测图大体相似。  相似文献   

Mountains on Titan observed by Cassini Radar     

Jani Radebaugh  Ralph D. Lorenz  Randolph L. Kirk  Ellen R. Stofan  Stephen D. Wall  the Cassini Radar Team 《Icarus》2007,192(1):77-91

The Cassini Titan Radar mapper has observed elevated blocks and ridge-forming block chains on Saturn's moon Titan demonstrating high topography we term “mountains.” Summit flanks measured from the T3 (February 2005) and T8 (October 2005) flybys have a mean maximum slope of 37° and total elevations up to 1930 m as derived from a shape-from-shading model corrected for the probable effects of image resolution. Mountain peak morphologies and surrounding, diffuse blankets give evidence that erosion has acted upon these features, perhaps in the form of fluvial runoff. Possible formation mechanisms for these mountains include crustal compressional tectonism and upthrusting of blocks, extensional tectonism and formation of horst-and-graben, deposition as blocks of impact ejecta, or dissection and erosion of a preexisting layer of material. All above processes may be at work, given the diversity of geology evident across Titan's surface. Comparisons of mountain and blanket volumes and erosion rate estimates for Titan provide a typical mountain age as young as 20-100 million years.  相似文献   

Recently Ratified and Proposed Cambrian Global Standard Stratotype-section and Points     

PENG Shanchi  ZHU Xuejian  ZUO Jinxun  LIN Huanling  CHEN Yong’an  WANG Longwu 《《地质学报》英文版》2011,85(2):296-308

This paper briefly summarizes an officially ratified Global Standard Stratotype-section and Point (GSSP) and a proposed GSSP for global stages of the Cambrian System. The Luoyixi section near Luoyixi town, Guzhang, northwestern Hunan is ratified as the boundary stratotype for the base of the global Guzhangian Stage, which is the upmost stage of an unnamed series termed provisionally as Cambrian Series 3. The GSSP position lies 121.3 m above the base of the Huaqiao Formation in the section, coinciding with the first appearance of the cosmopolitan agnostoid trilobite Lejopyge leavigata. The Duibian B section at Duibian village, Jiangshan, western Zhejiang, is proposed as the boundary stratotype for the base of the proposed global Jiangshanian Stage that is the second stage of the Furongian Series. The proposed GSSP position lies 108.12 m above the base of the Huayansi Formation in the section, coinciding with the first appearance of the cosmopolitan agnostoid trilobite Agnostotes orientalius. This horizon is also with the first appearance of the cosmopolitan polymerid trilobite Irvingella angustilimbata.  相似文献   

Northern Eurasia earth science partnership initiative (NEESPI), science plan overview     

Pavel Ya. Groisman  Sergey A. Bartalev  The NEESPI Science Plan Development Team 《Global and Planetary Change》2007,56(3-4):215

Northern Eurasia Earth System Partnership Initiative, NEESPI, was established to address the global change processes associated with and/or originated within Northern Eurasia as well as to study the major socially-important processes within the region. NEESPI began as a US–Russian initiative but has quickly broadened into a fully international program. Scientists from 11 countries participated in preparing the NEESPI Science Plan. Current version of the Science Plan was released for public review on the World Wide Web in summer 2004 and finalized in December 2004. This paper provides an Overview of the Plan and is based, mainly, on its Executive Summary. The Overview describes the Plan's science themes and key science questions, provides a justification of the urgency studying Northern Eurasia from the global change prospective, and outlines research strategy and tools to address NEESPI science questions, as well as projected deliverables of the Initiative.  相似文献   

营口—宽甸地区重力场特征及地质解释     

曹恩久 《国土资源》1991,(4)

营口—宽甸地区重力场自北而南有逐渐增高的总趋势。中部区重力低与重力高呈带状相间出现。结合该区已知的地质构造特征综合分析,重力负值带是早元古宙拗拉槽边界深断裂和构造—岩浆岩带的反映。隐伏、半隐伏花岗岩体的解释和推断,为逃一步寻找金、硼、铅锌等矿产提供了信息。  相似文献   

Remote sensing of mesospheric winds with the high-resolution doppler imager     

Paul B. Hays  HRDI Science Team 《Planetary and Space Science》1992,40(12):1599-1606

Observations of the winds in the upper atmosphere obtained with the High-Resolution Doppler Imager (HRDI) on the Upper Atmosphere Research Satellite (UARS) are discussed. This instrument is a very stable high-resolution triple-etalon Fabry-Perot interferometer, which is used to observe the slight Doppler shifts of absorption and emission lines in the O₂ Atmospheric bands induced by atmospheric motions. Preliminary observations indicate that the winds in the mesosphere and lower thermosphere are a mixture of migrating and non-migrating tides, and planetary-scale waves. The mean meridional winds are dominated by the 1,1 diurnal tide which is easily extracted from the daily zonal means of the satellite observations. The daily mean zonal winds are a mixture of the diurnal tide and a zonal flow which is consistent with theoretical expectations.  相似文献   

青海德尔尼硫化物矿床成因的新认识   总被引：2，自引：0，他引：2  

阿延寿 《青海国土经略》2001,(1)

通过对青海德尔尼硫化物矿床的产出部位、成矿环境、矿石矿物的组合、主要化学元素的成份及同位素测试数据等分析研究,认为该矿床具有裂谷成矿机制的特征,成因类型应属裂谷型层控矿床。  相似文献   

滩间山金矿矿床成因初步探讨     

党兴彦  付宝侠 《青海国土经略》1996,(2)

本文通过对滩间山矿区地层、构造及岩浆岩与成矿关系的研究,认为中元古界万洞沟群是金的矿源层;成矿构造具有多期次、多阶段活动的特点,矿体受单一及复合型式的构造控制;华力西期侵入体对成矿作用仅体现于为矿床的形成与再造提供热源。矿质在弱酸—中偏碱性溶液中,主要呈硫络合物的形式搬运、并在还原条件下成矿。特别指出,含磷质物地层是区内重要的岩金找矿标志之一。  相似文献   

东秦岭金堆城花岗斑岩体的锆石U-Pb年龄、物质来源及成矿机制   总被引：10，自引：0，他引：10  

焦建刚  汤中立  钱壮志  袁海潮  闫海卿  孙涛  徐刚  李小东 《地球科学》2010,35(6):1011-1022

通过LA-ICP-MS方法测得金堆城和老牛山花岗岩体中锆石U-Pb年龄分别为143.7±3 Ma和144.5±4.4 Ma,与金堆城钼矿床中辉钼矿的Re-Os年龄139±3.0 Ma在误差范围内一致,界定了金堆城成岩成矿时代为侏罗纪末-白垩纪初,2个岩体为同期岩浆事件的产物,与燕山运动有关.金堆城岩体较老牛山岩体富SiO₂、K₂O,岩石地球化学数据显示2个岩体都具有一致的高硅、富碱、过铝质系列和钙碱性岩石系列特征;高的ε_Sr(t)、低的ε_Nd(t)及Pb同位素图解证明2个岩体主要来自下地壳物质部分熔融,可能有少量地幔物质加入.年代学与岩石地球化学数据证实老牛山岩体和金堆城岩体的岩浆源区与岩石成因相同,推测老牛山岩体在深部发生分异演化,为金堆城小岩体提供了大量的热液和矿物质,从而出现了金堆城小岩体成大矿现象.   相似文献   

Emplacement of the youngest flood lava on Mars: A short, turbulent story   总被引：1，自引：0，他引：1  

W.L. Jaeger  L.P. Keszthelyi  M.P. Milazzo  T.N. Titus  D.M. Galuszka  R.L. Kirk  the HiRISE Team 《Icarus》2010,205(1):230-243

Recently acquired data from the High Resolution Imaging Science Experiment (HiRISE), Context (CTX) imager, and Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) onboard the Mars Reconnaissance Orbiter (MRO) spacecraft were used to investigate the emplacement of the youngest flood-lava flow on Mars. Careful mapping finds that the Athabasca Valles flood lava is the product of a single eruption, and it covers 250,000 km² of western Elysium Planitia with an estimated 5000-7500 km³ of mafic or ultramafic lava. Calculations utilizing topographic data enhanced with MRO observations to refine the dimensions of the channel system show that this flood lava was emplaced turbulently over a period of only a few to several weeks. This is the first well-documented example of a turbulently emplaced flood lava anywhere in the Solar System. However, MRO data suggest that this same process may have operated in a number of martian channel systems. The magnitude and dynamics of these lava floods are similar to the aqueous floods that are generally believed to have eroded the channels, raising the intriguing possibility that mechanical erosion by lava could have played a role in their incision.  相似文献