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51.
西太平洋海山磷酸盐的常量、微量和稀土元素地球化学研究 总被引:8,自引:0,他引:8
本文对主要取自于西太平洋我国调查区内不同海山、不同水深、不同产状的13个磷酸盐样品进行了常量、微量和稀土元素测定,以探讨与大洋富钴结壳密切伴生的磷酸盐的常、微量和稀土元素地球化学的特征。分析结果表明,调查区磷酸盐中主要氧化物的平均值与赤道太平洋的相近,暗示两者可能有相似的形成环境和形成机制。磷酸盐中微量元素Sr、Ba、Co、Cu、Ni及U丰度分别变化于862×10~(-6)~2181×10~(-6)、29×10~(-6)~3429×10~(-6)、6.3×10~(-6)~115×10~(-6)、23×10~(-6)~263×10~(-6)、12×10~(-6)~825×10~(-6)及4×10~(-6)~11×10~(-6),丰度多数低于泥质岩平均值,其CaO/P_2O_5、F/CO_2、Sr/P_2O_5值及常量、微量元素间的相关关系,清晰地显示了磷酸盐的种类、成分与结构、形成的地质背景和元素的主要组合特征。磷酸盐的稀土丰度为136.50×10~(-6)~853.70×10~(-6);Ce~*变化于0.01~0.18之间;(Ce/Yb)_N值变化于0.01~0.21之间。研究证实,不同产状磷酸盐的稀土元素配分模式基本一致,曲线相互平行,基本不呈现交叉现象,均呈Ce强烈亏损,轻、重稀土分馏程度大及重稀土富集的型式。调查区、赤道太平洋、中太平洋磷酸盐的稀土元素丰度、Ce~*、Ce/Yb值以及它们与海水稀土元素配分模式相似的特征,也进一步显 相似文献
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Russian Federation/ United States Calibration Working Group 《Pure and Applied Geophysics》2001,158(1-2):59-77
—?Joint Research Program of Seismic Calibration of the International Monitoring System (IMS) in Northern Eurasia and North America has been signed by the Nuclear Treaty Programs Office (NTPO), Department of Defense USA, and the Special Monitoring Service (SMS) of the Ministry of Defense, Russian Federation (RF). Under the Program historical data from nuclear and large chemical explosions of known location and shot time, together with appropriate geological and geophysical data, has been used to derive regional Pn/P travel-time tables for seismic event location within the lower 48 States of the USA and the European part of the RF. These travel-time tables are up to 5?seconds faster in shields than the IASPEI91 tables, and up to 5?seconds slower in the Western USA. Relocation experiments using the regional Pn travel-time curves and surrogate networks for the IMS network generally improved locations for regional seismic events. The distance between true and estimated location (mislocation) was decreased from an average of 18.8?km for the IASPEI91 tables to 10.1?km for the regional Pn travel-time tables. However, the regional travel-time table approach has limitations caused by travel-time variations inside major tectonic provinces and paths crossing several tectonic provinces with substantially different crustal and upper mantle velocity structure.¶The RF members of the Calibration Working Group (WG): Colonel Vyacheslav Gordon (chairman); Dr. Prof. Marat Mamsurov, and Dr. Nikolai Vasiliev. The US members of the WG: Dr. Anton Dainty (chairman), Dr. Douglas Baumgardt, Mr. John Murphy, Dr. Robert North, and Dr. Vladislav Ryaboy. 相似文献
54.
中国地震学会地震学专业委员会 《国际地震动态》2001,(1):17-18
中国地震学会第五届地震学专业委员会自1999年1月成立以来,在常务理事会和学会理事长的指导下,充分发挥委员在基础研究和战略研究方面的整体优势,围绕我国地震科学发展和防震减灾事业的一些重要问题,开展了多方面的工作。其中,将专业委员会活动的视野进一步扩大,与国内的有关机构和团体开展多方面的合作,并积极关注和参与国际性的学术活动,是本届专业委员会活动的一个特色。英国《自然》杂志(Nature)于1999年2月25日~4月8日在因特网上组织了主题为“Isthereliablepredictionofindividualearth-quakesarealisticscientificgoal?”的争论,引… 相似文献
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叙述了1989大同—阳高地震的基本情况,回顾了此次地震现场的分析预报工作。按照《地震现场工作大纲和震情分析指南》所确定的原则,采用国内常用的一些方法,对此次地震的类型、震前活动、地震趋势、余震活动等做了分析。并对几次强余震的预报过程进行了讨论。 相似文献
57.
Monte Carlo Radiative Transfer Modeling of Lightning Observed in Galileo Images of Jupiter 总被引:1,自引:0,他引:1
We study lightning on Jupiter and the clouds illuminated by the lightning using images taken by the Galileo orbiter. The Galileo images have a resolution of ∼25 km/pixel and are able to resolve the shape of single lightning spots, which have half widths (radii) at half the maximum intensity in the range 45-80 km. We compare the shape and width of lightning flashes in the images with simulated flashes produced by our 3D Monte Carlo light-scattering model.The model calculates Monte Carlo scattering of photons in a 3D opacity distribution. During each scattering event, light is partially absorbed. The new direction of the photon after scattering is chosen according to a Henyey-Greenstein phase function. An image from each direction is produced by accumulating photons emerging from the cloud in a small range (bins) of emission angles. The light source is modeled either as a point or a vertical line.A plane-parallel cloud layer does not always fit the data. In some cases the cloud over the light source appears to resemble cumulus clouds on Earth. Lightning is estimated to occur at least as deep as the bottom of the expected water cloud. For the six flashes studied, we find that the clouds above the lightning are optically thick (τ>5). Jovian flashes are more regular and circular than the largest terrestrial flashes observed from space. On Jupiter there is nothing equivalent to the 30-40-km horizontal flashes that are seen on Earth. 相似文献
58.
东坪式金矿床产于华北地台北缘金矿成矿带的冀西北金矿集中区,构造上位于华北克拉通北缘深大断裂-尚义-赤城断裂的南侧。金矿床产于泥盆纪早期(386~410Ma)水泉沟正长岩杂岩体内及接触带附近,矿体分布受脆-韧性剪切断裂构造的制约。金矿成矿作用具有多期次的特点,成矿时代为燕山期(156~203Ma)。矿石类型主要为石英脉型、石英网脉 脉旁钾硅化蚀变岩型和钾硅化蚀变岩型,具有典型的碱性岩金矿的金-碲组合,(含)金矿物主要为自然金、碲金矿和碲金银矿。流体包裹体的 H、O 及 He 同位素研究表明,成矿流体为以大气降水主的混合热液流体并可能存在深源流体的参与。矿床的 S、Pb、Sr 和 Si 同位素组成表明,金矿成矿物质主要来源于正长岩杂岩体,部分源于太古宙桑干群变质岩和燕山期花岗岩。因此,东坪式金矿是由燕山期伸展构造环境下热液流体在上涌地幔及岩浆活动的热驱动下对泥盆纪早期形成的正长岩交代改造的产物。 相似文献
59.
One of the fundamental questions concerning the nature and prediction of the oceanic states in the equatorial eastern Pacific is how the turnabout from a cold water state (La Nina) to a warm water state (El Nino) takes place, and vice versa. Recent studies show that this turnabout is directly linked to the interannual thermocline variations in the tropical Pacific Ocean basin. An index, as an indicator and precursor to describe interannual thermocline variations and the turnabout of oceanic states in our previous paper (Qian and Hu, 2005), is also used in this study. The index, which shows the maximum subsurface temperature anomaly (MSTA), is derived from the monthly 21-year (1980-2000) expendable XBT dataset in the present study. Results show that the MSTA can be used as a precursor for the occurrences of El Nino (or La Nina) events. The subsequent analyses of the MSTA propagations in the tropical Pacific suggest a one-year potential predictability for El Nino and La Nina events by identifying ocean temperature anomalies in the thermocline of the western Pacific Ocean. It also suggests that a closed route cycle with the strongest signal propagation is identified only in the tropical North Pacific Ocean. A positive (or negative) MSTA signal may travel from the western equatorial Pacific to the eastern equatorial Pacific with the strongest signal along the equator. This signal turns northward along the tropical eastern boundary of the basin and then moves westward along the north side of off-equator around 16°N. Finally, the signal returns toward the equator along the western boundary of the basin. The turnabout time from an El Nino event to a La Nina event in the eastern equatorial Pacific depends critically on the speed of the signal traveling along the closed route, and it usually needs about 4 years. This finding may help to predict the occurrence of the El Nino or La Nina event at least one year in advance. 相似文献
60.
中国海相碳酸盐岩层系油气地质特点、战略选区思考及需要解决的主要地质问题 总被引:2,自引:0,他引:2
中国海相碳酸盐岩层系油气资源量大,但探明程度低,是油气资源战略接替的重要领域。中国海相碳酸盐岩层系具有形成时代老、改造强烈、沉积中心与生烃中心不吻合、储层具有多样性且非均质性强、多烃源层、多期生烃、多期成藏、多期调整与改造等显著特点,与陆相碎屑岩层系有明显差别,又有别于国外海相碳酸盐岩层系。在对不同地区海相碳酸盐岩层系油气地质条件进行分析解剖的基础上,分别对四川盆地、中下扬子及滇黔桂地区、塔里木盆地、鄂尔多斯盆地、渤海湾盆地和青藏地区的海相碳酸盐岩层系油气勘探战略选区急需解决的地质问题进行了讨论。 相似文献