Basic characteristics of active tectonics of China

Active tectonics is inferred to all the structures which have been active since the late Pleisto-cene, 100—120 ka B.P., are still active recently, and will be active in a certain time period in the future, such as active faults, active folds, active basi…     

X-ray emission from accretion disks in active galactic nuclei

We constructed a grid of relativistic models for standard high-relative-luminosity accretion α-disks around supermassive Kerr black holes (BHs) and computed X-ray spectra for their hot, effectively optically thin inner parts by taking into account general-relativity effects. They are known to be heated to high (～10⁶–10⁹ K) temperatures and to cool down through the Comptonization of intrinsic thermal radiation. Their spectra are power laws with an exponential cutoff at high energies; i.e., they have the same shape as those observed in active galactic nuclei (AGNs). Fitting the observed X-ray spectra of AGNs with computed spectra allowed us to estimate the fundamental parameters of BHs (their mass and Kerr parameter) and accretion disks (luminosity and inclination to the line of sight) in 28 AGNs. We show that the Kerr parameter for BHs in AGNs is close to unity and that the disk inclination correlates with the Seyfert type of AGN, in accordance with the unification model of activity. The estimated BH masses M_x are compared with the masses M_rev determined by the reverberation mapping technique. For AGNs with luminosities close to the Eddington limit, these masses agree and the model under consideration may be valid for them. For low-relative-luminosity AGNs, the differences in masses increase with decreasing relative luminosity and their X-ray emission cannot be explained by this model.     

Study on coupling between deep and shallow structures of Xingtai area and some significant questions

IntroductionIn order to gain a clear idea of the deep tectonic environment of Xingtai earthquake area,three wide-angle deep seismic renectionlrefraction profiles have been conducted through the are4they are Yuanshi--Ji'nan profile, Renxian--Wuqing profile and Tat' an--LongyaM inzhou profi I e.The Yuanshi--Ji'nan profile passes through the epicenter of the Ms=7.2 main shock andTat' ~ongyaO--X inzhou profi ie passes through the ep icenter of the Ms=6. 8 earthquake. Duringthe "Eighth Five-…     

阿勒泰复向斜的成矿环境及其矿产

在阿勒泰复向斜内,分布有众多矿产,是阿尔泰山南缘重要的铜、铅、锌及多金属成矿区之一。文章详细介绍了这些重要矿床即铁木尔特铜-锌矿床、大东沟铅-锌矿床、乌拉斯沟铜-铅-锌矿床、阿巴宫铁矿床、红墩铅-锌矿床的地质特征,并从现代成矿理论角度全面分析了这些矿床形成的区域成矿环境及其找矿前景。     

鄂尔多斯盆地东北部延安组铀异常与沉积体系的关系

在鄂尔多斯盆地东北部,延安组第V成因单元存在着多处铀异常,这对铀的后备战略基地建设有重要意义。从沉积学的角度重建了第V成因单元的沉积体系,识别出两种沉积体系,分别是位于研究区西北部的辫状河沉积体系和东南部的曲流河沉积体系。通过对铀异常信息的成功提取及平面编图,发现延安组中铀异常呈一个又一个具有自我中心的单元出现,且与曲流河沉积体系的关系密切:通常发育于河道分岔或转弯处;普遍发育于薄砂带(区),一般砂体厚度在30 m以下,含砂率小于40%;铀异常单元与厚煤层关系密切;主要赋存于粒度较细的岩性中,部分也富集于煤中,但铀异常最高值富集于中砂岩中。     

构造控制型天然气水合物矿藏及其特征

构造环境是天然气水合物富集成藏的重要控制因素,增生楔、断裂体系、褶皱、(泥)底辟、滑塌等特殊构造体是影响天然气水合物成藏的主要地质载体。通过对这些特殊构造体与天然气水合物成藏关系的研究,结合流体活动对水合物形成的影响,总结出陆缘地区有增生楔型、盆缘斜坡型、埋藏背斜型、断褶型、滑塌型及底辟型等六类构造控制型水合物矿藏。南海位于欧亚板块、太平洋板块及印澳板块的交汇处,早期为活动陆缘,晚期演化为被动陆缘,其构造活动具有早期张裂、后期挤压的特点,这既不同于被动陆缘,也有别于活动陆缘,可视为“复合型”大陆边缘,兼具了“被动陆缘沉积速率高、活动陆缘构造活跃”的优点,从而形成了“增生楔型、断褶型、底辟型、滑塌型、盆缘斜坡型”等多种构造控制型水合物矿藏,是“复合型”大陆边缘水合物成藏地质模式的典型代表。     

夏季青藏高原东部降水变化与副热带高压带活动的研究

用青藏高原上常规的台站资料和NCEP/NCAR的再分析资料,分析和研究了1993/1994年夏季5—8月青藏高原东部降水变化与西太平洋副热带高压南北移动的关系。结果表明:1993年夏季的副热带高压异常偏南,5—8月副高脊线北移过程中,还伴有准双周南北移动过程;而1994年夏季的副热带高压异常偏北,5—8月副高脊线北移过程中,则主要伴有30—60d的低频变化的南北移动过程。同时,在分析青藏高原上的天气变化特征时,发现这两年高原东部的降水变化特征也有明显的不同,夏季高原上降水的活跃和中断与副高脊线南北移动变化有类似的特征。因此,夏季西太平洋副热带高压南北移动可能与高原东部降水的中断/活跃有一定的关系。     

中国大陆及邻区、川滇成组强震活动特征初步研究

将中国大陆及其邻区1902年以来MS≥7地震的成组活动划分出7组,其首发大震分别为1902年阿图什8.2级,1911年阿拉木图8.2级,1920年海原8.5级,1931年富蕴8.0级,1946年缅甸7.8级,1966年邢台7.2级,1988年缅甸7.2级。川滇MS≥6.7地震成组活动划分出5组,其首发强震为1913年峨山7.0级,1933年茂县7.5级,1948年理塘7.3级,1966年东川6.5级、6.2级,1988年澜沧7.4级。其中,川滇MS≥7的首发大震滞后中国大陆首发大震几个月至4年不等。按成组大震的界定,目前中国大陆处于1998~2007年(估计)的大震少发时段。川滇未来1~2年的大震形势为川滇西部存在发生大震的可能性。中国大陆新一轮强震成组活动中的大地震将可能在2007~2009年前后发生,主体危险区可能为天山地震带中段及川滇东部。2007~2008年可能出现5~6级地震的增强过程。巧家—东川一带可能最先发生6级地震。     

A network communication and recording system for digital seismic observation

Introduction Digital seismic observation systems originated from 1970′s. It has developed greatly in the past 30 years up to now. Its performances were improved, dynamic range and resolution increased a lot, the power consumption decreased a lot, and so on (YOU et al, 2003a, b). In a word, the dream of broad frequency-band, big dynamic range, digitalization of seismic observation has come true already. But, the previous digital seismic observation systems only support communica-tion based o…