湖南元古宙林家湾组和横路冲组的对比研究   总被引：2，自引：2，他引：0  

潘传楚 《大地构造与成矿学》1999,23(4):381-385

简单介绍了湖南元古宙论水铺群林家湾组正层型剖面和板溪群横路冲组正副层型剖面;对比了二组剖面的地层岩性和成岩时代及层位等特征;论证了沧水铺群林家湾组层位是合乎客观地质实际的;阐述了对湖南益阳沧水铺地区磨拉石一火山建造的划分对比讨论的重要意义。  相似文献   

长庆气田奥陶系风化壳气藏、气源研究   总被引：22，自引：4，他引：18  

戴金星  夏新宇 《地学前缘》1999,6(Z1):195-203

对10年来长庆气田奥陶系风化充气藏气源问题存在的不同观点（上古生界煤成气和奥陶系海相碳酸盐岩气何者为主）及相应的证据进行了总结和讨论,认为“奥陶系自生自储为主”的观点对地质和地球化学现象的解释存在疑问,包括用次要组分来判别混源天然气的主要来源,用不确切的端员气地球化学特征来计算混源比,对本溪组底部岩石的封盖性和下奥陶统碳酸盐岩的原始生烃潜力评价偏高,忽略了石炭系存在能够生成油型气的海相源岩。因此,长庆气田不能作为海相贫有机质的碳酸盐岩生成的大、中型油气田的实例。根据天然气及气源岩的地球化学特征,提出长庆气田奥陶系风化壳气藏气是以上古生界煤成气为主、石炭系海相源岩生成的油型气为辅的混合气。  相似文献   

冕流与日冕物质抛射的关系     

堵锦生  童彝  杨静  伊塞列维奇 《紫金山天文台台刊》1999,18(2):135-138

本文研究了卡林顿自转周１５９１ － １５９２ 中冕流偏振亮度的变化。冕流带偏振亮度的分布是不均匀的,不均匀度为１０ ％ － ５０ ％ 。无日冕物质抛射影响存在时,沿冕流带冕流的分布可持续稳定存在近两个太阳自转周。当一个日冕物质抛射伴随冕流产生时,冕流的经向角大小若大于２７°,可导致冕流尖角区顶部上升速度大于２ｋｍ／ｓ。  相似文献   

滇黔桂卡林型金矿区水系沉积物和岩石金含量与时空分布     

赵东杰  王学求 《地球学报》2020,41(3):407-419

为研究滇黔桂卡林型金矿区水系沉积物和岩石中金的地球化学时空分布及其与金矿规模的对应关系,系统收集了该区1:20万区域化探全国扫面计划水系沉积物和全国地球化学基准计划岩石金的地球化学数据,绘制了水系沉积物和岩石金的地球化学分布图。滇黔桂卡林型金矿区以水系沉积物金地球化学异常面积大于1000 km^2为准,共圈定5处金的地球化学省,这些金的地球化学省同时也是矿床大规模产出的部位。区内右江盆地水系沉积物金背景值(1.94×10^–9)高于扬子克拉通(1.68×10^9),其内以泥岩、页岩、砂岩、灰岩为代表的容矿岩石金背景值(0.51×10^–9)也高于扬子克拉通(0.39×10^–9)。研究区不同构造单元及沉积相中水系沉积物金背景值受岩石金背景值的制约。金的地球化学省是地壳演化过程中不均匀分布的高金背景岩石、金矿化作用及金矿床次生风化作用相互叠加的结果。该研究有助于有效判断异常成因、识别成矿作用存在,对研究金的区域成矿规律和聚焦找矿靶区具有重要意义。  相似文献   

Estimation of PM_(2.5) Mass Concentration from Visibility     

Denghui JI  Zhaoze DENG  Xiaoyu SUN  Liang RAN  Xiangao XIA  Disong FU  Zijue SONG  Pucai WANG  Yunfei WU  Ping TIAN  Mengyu HUANG 《大气科学进展》2020,37(7):671-678

Aerosols in the atmosphere not only degrade visibility, but are also detrimental to human health and transportation. In order to develop a method to estimate PM_(2.5) mass concentration from the widely measured visibility, a field campaign was conducted in Southwest China in January 2019. Visibility, ambient relative humidity(RH), PM_(2.5) mass concentrations and scattering coefficients of dry particles were measured. During the campaign, two pollution episodes, i.e., from 4-9 January and from 10-16 January, were encountered. Each of the two episodes could be divided into two periods. High aerosol hygroscopicity was found during the first period, when RH was higher than 80% at most of the time, and sometimes even approached 100%. The second period experienced a relatively dry but more polluted condition and aerosol hygroscopicity was lower than that during the first period. An empirical relationship between PM_(2.5) mass concentration and visibility(ambient aerosol extinction) under different RH conditions could thus be established. Based on the empirical relationship,PM_(2.5) mass concentration could be well estimated from visibility and RH. This method will be useful for remote sensing of PM_(2.5) mass concentration.  相似文献   

The fraction of galaxies that contain active nuclei and their accretion rates     

M.J. Page 《Monthly notices of the Royal Astronomical Society》2001,328(3):925-930

We investigate the relationship between the present-day optical luminosity function of galaxies and the X-ray luminosity function of Seyfert 1s to determine the fraction of galaxies that host Seyfert 1 nuclei and their Eddington ratios. The local type 1 active galactic nuclei (AGN) X-ray luminosity function is well reproduced if ∼1 per cent of all galaxies are type 1 Seyferts which have Eddington ratios of ∼10⁻³. However, in such a model the X-ray luminosity function is completely dominated by AGN in E and S0 galaxies, contrary to the observed mix of Seyfert host galaxies. To obtain a plausible mix of AGN host galaxy morphologies requires that the most massive black holes in E and S0 galaxies accrete with lower Eddington ratios, or have a lower incidence of Seyfert activity, than the central black holes of later-type galaxies.  相似文献   

抚顺地区砬子山杂岩体地质特征及成因     

何建泽 《国土资源》1993,(4)

砬子山岩体出露于华北地台抚顺—清原古隆起带与吉黑地槽的相接部位。砬子山岩体是由石英闪长岩、似斑状石英二长岩、二长花岗岩和碱长花岗岩构成的杂岩体。4个岩性不同的侵入体构成连续的中-酸性钙碱岩石序列。岩体的地质特征、地球化学特征表明4个侵入体是同源岩浆不同演化阶段的产物。岩浆的演化机制为深部岩浆分异作用,岩浆则是来源于下部地壳。  相似文献   

鄂拉山东北段都龙超单元地质特征     

邢国忠  安勇胜 《青海国土经略》1996,(2)

都龙超单元是一个大型中酸性复式岩体,具成分和结构演化序列。根据同源岩浆演化的理论,结合岩石化学、地球化学、包体特征及各侵入体的接触关系等,将该岩体进行了系统的解体,圈定出23个大小不等的侵入体,进一步归并为5个单元和一个超单元,建立了区内的岩石谱系单位。并对超单元的成因类型和就位机制进行了探讨,认为该岩体是同一大地构造环境下同源岩浆多次脉(涌)动形成的超单元。  相似文献   

青藏高原物质东流的岩石层力学背景探讨   总被引：3，自引：0，他引：3  

熊熊  许厚泽  滕吉文 《大地测量与地球动力学》2001,21(2):1-6

利用地表大地热流观测资料、岩石生热率及热导率数据研究了三江和四川盆地 6个地区的岩石层平均温度结构及强度分布。结果表明 ,整个三江地区岩石层温度较高 ,而四川盆地温度较低 ;在岩石层强度分布上 ,四川盆地为高强度区 ,而三江地区则为低强度区 ;整个三江地区构成了一条青藏高原物质东流的低强度通道 ;由于四川盆地高强度块体的阻挡 ,青藏高原向东的物质流在此转向近南向 ,沿三江地区流逸 ;不同岩石层块体的强度差异可能是控制高原物质流动态势的重要力学背景之一。  相似文献   

Stable Eocene Magnetization Carried by Magnetite and Iron Sulphides in Marine Marls (Pamplona-Arguis Formation,Southern Pyrenees,Northern Spain)     

Larrasoaña  J.C.  Parés  J.M.  Pueyo  E.L. 《Studia Geophysica et Geodaetica》2003,47(2):237-254

In order to establish the magnetic carriers and assess the reliability of previous paleomagnetic results obtained for Eocene marine marls from the south Pyrenean basin, we carried out a combined paleo- and rock-magnetic study of the Pamplona-Arguis Formation, which crops out in the western sector of the southern Pyrenees (N Spain). The unblocking temperatures suggest that the characteristic remanent magnetization (ChRM) is carried by magnetite and iron sulphides. The ChRM has both normal and reversed polarities regardless of whether it resides in magnetite or iron sulphides, and represents a primary Eocene magnetization acquired before folding. Rock magnetic results confirm the presence of magnetite and smaller amounts of magnetic iron sulphides, most likely pyrrhotite, in all the studied samples. Framboidal pyrite is ubiquitous in the marls and suggests that iron sulphides formed during early diagenesis under sulphate-reducing conditions. ChRM directions carried by magnetic iron sulphides are consistent with those recorded by magnetite. These observations suggest that magnetic iron sulphides carry a chemical remanent magnetization that coexists with a remanence residing in detrital magnetite. We suggest that the south Pyrenean Eocene marls are suitable for magnetostratigraphic and tectonic purposes but not for studies of polarity transitions, secular variations and geomagnetic excursions, because it is difficult to test for short time differences in remanence lock-in time for the two minerals. The presence of iron sulphide minerals contributing to the primary magnetization in Eocene marine marls reinforces the idea that these minerals can persist over long periods of time in the geological record.  相似文献