东海陆架南部邻近陆域晚三叠世—早侏罗世沉积古环境分析

东海陆架盆地南部邻近陆域主要包括福建东南部以及广东东北部的广大地区。结合野外地质考察、岩石薄片镜鉴及样品地球化学测试结果等资料,研究了该地区晚三叠世—早侏罗世沉积古环境。研究区晚三叠世—早侏罗世时期,属于温湿气候环境,南部的粤东地区沉积水体深度较大,因此,大部分样品指示厌氧环境。晚三叠世时,整个东海陆架南部邻近陆域自南向北水体逐渐变浅,南部主要为滨海—浅海陆棚—深水陆棚环境,北部主要表现为受海侵作用影响的海陆过渡相环境;早侏罗世时,南部主要表现为水体较深的深水陆棚环境,北部主要表现为海陆过渡相—陆相沉积环境。通过对具有相同大地构造背景的邻近陆域沉积古环境的研究,从而可以推断缺乏钻井资料的东海陆架盆地南部沉积古环境自北向南由陆及海,为后续开展海域中生界油气地质条件研究提供依据。     

A Kinematical Calibration of the Galactocentric Distance

1 INTRODUCTION The distance to the Galactic center R0 is a fundamental constant for astronomy and astrophysics. Most determinations of astronomical quantities are directly connected with the Galactic distance scale, e.g., the rotational speed of our Galax…     

Excitation of Annual Polar Motion by the Pacific,Atlantic and Indian Oceans

The global oceans play important roles in exciting the annual polar motion besides the atmosphere. However,it is still unclear about how large the regional oceans contribute to the annual polar motion. We investigate systemically the contributions of the Pacific,Atlantic and Indian Oceans to the excitation of the annual polar motion,based on the output data of ocean current velocity field and ocean bottom pressure field from "Estimating the Circulation and Climate of the Ocean (ECCO)" ocean circulation model over the period 1993-2005. The result shows that due to its particular location and shape,the Atlantic Ocean makes a less significant contribution to the x-component of the annual polar motion excitation than the Pacific and Indian Oceans,while all these three oceans contribute to the y-component of the annual polar motion excitation to some extent.     

An Infrared Photometric Study of Galaxies with Extragalactic H2O Maser Sources

All galaxies with extragalactic H_2O maser sources observed so far are collected. With the 2MASS and the IRAS photometric data an infrared study is performed on those galaxies.By a comparison between the H_2O maser detected sources and non-detected sources in the infrared it is indicated that infrared properties in the IRAS 12-25μm and 60-100μm are important for producing H_2O masers in galaxies.It is also found that the H_2O maser galaxies with different nuclear activity types have rather different infrared properties mainly in the IRAS 12-60μm region.     

Shallow Decay of X-ray Afterglows in Short GRBs： Energy Injection from a Millisecond Magnetar？

With the successful launch of Swift satellite,more and more data of early X-ray afterglows from short gamma-ray bursts have been collected.Some interesting features such as unusual afterglow light curves and unexpected X-ray flares are revealed.Especially,in some cases,there is a fiat segment in the X-ray afterglow light curve.Here we present a simplified model in which we believe that the flattening part is due to energy injection from the central engine.We assume that this energy injection arises from the magnetic dipole radiation of a millisecond pulsar formed after the merger of two neutron stars.We check this model with the short GRB 060313.Our numerical results suggest that energy injection from a millisecond magnetar could make part of the X-ray afterglow light curve flat.     

Rotation Periods of Nine ROSAT Selected Solar-Type Stars

We monitored 16 X-ray selected young solar-type stars for light variation and found appreciable periodic light variability with amplitudes of a few hundredths of a magni-tude in nine of the objects. Using the method of Phase Dispersion Minimization (PDM) and Fourier analysis (software PERIOD04), the rotation periods of these stars were determined from the photometric data. The rotation periods of all nine stars are shorter than about 3days. It is suggested that, as with the Pleiades cluster, small amplitude light variations are quite common among young solar-type stars with rotation periods around 3 days or less. This gives further evidence for the spin up of solar-type stars predicted by models of angular momentum evolution of pre-main sequence stars.     

中国东部海域及相邻陆域综合地层分区及地层发育特征

中国东部海域地质历史上长期处于板块的结合部位,构造活动剧烈,地层发育特征复杂,一直是众多学者研究的焦点。海域和陆域地层研究程度不均衡,陆域资料多,研究程度高,而海域受各种条件限制,研究程度较低。此外,地层分区方案多针对陆域开展工作,迄今没有开展过统一的海域-陆域的地层分区,制约了对我国地层整体发育特征的深入认识。本文以近几年实施的1∶100万和更高比例尺的海洋区域调查成果资料为基础,开展了中国东部海域及邻域综合地层分区,系统研究了各地层分区中地层发育特征,重点研究了我国东部海域(台湾以北海域)中生代以来的地层特征和沉积演化历史。结果表明,我国东部海域及相邻陆域可以划分为1个地层大区(一级)、5个地层区(二级)和13个地层分区(三级);渤海海域主体位于华北平原分区,北黄海海域主要分布在辽东地层分区,南黄海海域主要属于下扬子地层分区,而东海和冲绳海槽主要位于东海陆架分区;中生代以来中国东部海域内各个盆地经历了复杂的构造-沉积演化过程,地层发育特征差异性明显。     

准噶尔盆地腹部下侏罗统三工河组储层物性—含油性特征及主控因素分析

为解决准噶尔盆地腹部沙窝地、莫西庄和征沙村三地区下侏罗统三工河组砂岩储层物性—含油性差异大及控制因素不清的问题,本文通过岩芯描述、铸体薄片和扫描电镜分析,依据物性数据及压汞资料,对研究区三工河组储集空间特征、孔渗特征及孔喉结构特征进行了详细的研究,通过隔夹层分析、岩屑成分及含量分析、成岩特征研究等方法探讨了制约研究区三工河组储层物性—含油性关系的主控因素,研究表明沙窝地和莫西庄小区三工河组储层埋深相对较浅,主要以中粗孔喉和较细孔喉的原生（残留）孔隙为主;征沙村小区埋藏较深,以细孔喉和微孔喉的次生孔隙及裂缝发育为特色。在此基础上探讨了三工河组储层物性的控制因素,研究认为埋藏深度为影响储层发育的主要因素;沉积微相和砂体成因类型为控制储层发育的基础;低地温梯度延迟了压实效应等,有效保存了原生孔隙;塑性岩屑含量、储层的隔层和夹层因素,即储层的非均质性在某种程度上影响砂体的储集性。     

郯庐断裂南段怀远—池河北西向断裂的第四纪活动性——来自韭山东北缘的地质证据

怀远—池河断裂与郯庐断裂带南段相交,处在郯庐断裂带活动性逐渐减弱的地段。为获取断裂活动的地质证据,选取安徽韭山东北缘进行地貌调查、探槽开挖、年龄样品测试等工作。研究表明,韭山东北缘的线性地貌受断裂活动控制,在调查揭示的多个剖面中,断层表现出一致的活动性质,走向NW,倾向NE,倾角70°左右,具有正断性质;断层垂直断距在第四系中由下往上逐渐变小,直至消失在第四纪覆盖层中,说明断裂具有多期活动,进入中更新世后活动性逐渐减弱。通过跨断层探槽剖面分析及测年结果可知,断层最新活动错断了中更新世地层,上覆的中更新世顶部地层及晚更新世地层未受影响,说明该断裂是一条中更新世断裂,晚更新世以来不活动。怀远—池河断裂的活动情况与其所在地区的新构造环境有关。郯庐断裂带是本区规模最大的控制性构造,它的活动性对区内其他断裂具有重要影响,断裂带明光以南段最新活动时代为中更新世,受其影响,与它相交的怀远—池河断裂最新活动时代也表现为中更新世。这或是蚌埠—凤阳地区以中小地震活动为主的一个构造背景。