新疆伽师及邻区地震与控震构造分析

1996年3月-1997年4月间,新疆伽师西部相继发生6.9级强震与由7次6-6.6级子震所构成的强震群。历史上伽师及邻区曾发生多次强烈地震,导致伽师及邻区包括塔里木盆地周缘地震强烈活动的原因,是印度岩石圈块体快速北向运动造成的SN向强烈挤压与欧亚岩石圈块体缓慢向西运动所引起的左旋走滑的联合作用及其相关的现今不同方向、不同性质的断裂活动。区域性EW向盆缘活动断裂控制盆缘大型地震活动带的空间展布,盆缘EW向主干活动断裂与其他方向次级活动断裂的交叉复合部位是强烈地震发震的有利部位。伽师强震群子震震中分布受塔里木盆地西缘近SN-NNW向隐伏深断裂及其与EW向盆缘活动断裂的复合所控制。伽师强震群发生之后,在原强震群震中处发生7级以上更大地震的可能性很小;但由于塔里木盆地及其周缘,自1996年起已进入一个新的地震活跃期,在伽师附近及其南侧或东侧,近年内发生6-7级以上强烈地震的可能性较大。      

中生代东亚大陆边缘构造演化

摘　要　根据东亚陆缘增生带生物古地理、放射虫时代研究的进展并结合同位素年代及东亚 地区火山活动、构造演化探讨了中生代东亚大陆与古太平洋板块之间的运动学关系及俯冲带 后退特征。中、晚三叠世那丹哈达岭、美浓等地体还位于北纬１２°以内及赤道附近,晚侏罗世 到达中高纬度。东亚活动大陆边缘开始于中侏罗世末,在此之前属转换大陆边缘。洋壳板块 向大陆下俯冲之后,由于地体拼贴引起俯冲带快速、长距离后退。     

华北西缘太原组火山事件沉积的发现及太原组地层对比

摘要：作者主要依据镜下岩矿特征,辅以岩石的野外产状与分布特点,并参考ＲＥＥ配分模式特征,首次发现华北西缘太原组存在３个火山事件层。根据火山事件沉积并结合最大海侵事件层对华北西缘太原组进行了区域对比．     

Kinematics of quasars and AGN

The VLBA has been used over a period of four years to study the internal motions within a sample of quasars and AGN. In most sources, features appear to propagate away from the central engine along a well collimated radio jet with apparent transverse velocities between zero and 10c, with some evidence for apparent accelerations and decelerations. The distribution of apparent velocity is not consistent with any simple ballistic model and appears to require either a spread in intrinsic velocity or a difference between the bulk velocity and pattern velocity. The dependence of apparent angular velocity with redshift is consistent with standard Friedmann world models. Further observations of a larger source sample, especially at large redshift may lead to meaningful constraints on world models.     

Rifting and early evolution of ancient ocean basins: the record of the Mesozoic Tethys and of the Galicia-Newfoundland margins

Although of different age, the undeformed Cretaceous Iberia/Newfoundland margins and the relics of the Jurassic Briançonnais/Adriatic margins preserved in the Alps document a similar spatial and temporal evolution of rifting suggesting that the evolution of both pairs of margins was controlled by the same processes. Rifting appears to depend strongly on the thermal history of the lithosphere, which controls the rheology and consequently also the structural evolution of the margin. The tectonic evolution of non-volcanic margins appears to be distinctly different from that of volcanic ones.     

Deep crustal structure and rheology of the Gascoyne volcanic margin,western Australia

Interpretation of deep seismic reflection data across the Gascoyne Margin reveals six distinct seismic facies units related to the tectono-magmatic breakup history. On the outer Exmouth Plateau four large scale units are identified: (1) an extensively block-faulted upper crust; (2) a middle-crustal unit of discontinuous, undulatory reflectors; (3) a reflection-free deep crustal unit; and (4) a lower-crustal band of low-frequency, high-amplitude reflectors. Two additional units are found near the continent-ocean boundary (COB); (5) seaward-dipping reflectors (SDR); and (6) landward-dipping reflectors in the lower crust below the SDR. The lower-crustal high-reflectivity band, located near the top of a high-velocity unit (V_p > 7 kms^–1), is interpreted as magmatic underplating. There is a spatial correlation between the underplated area and the presence of extensive upper-crustal block-faulting and intrusive rocks in the shallow crust. The undulatory middle-crustal reflector unit is also only identified in the outer plateau area, and is interpreted as a zone in which the upper-crustal faults terminate. The inner parts of the margin consist of a deep basin showing little upper-crustal faulting and no evidence of middle crustal deformation or underplating. Theoretical modeling of the effect of rifting and magmatic underplating on crustal strength profiles suggests that the brittle-ductile transition may migrate at least 5 km upwards during several million years after the underplating event. Based on the seismic interpretation and crustal strength modeling we propose that the seismic structure of the outer Exmouth Plateau is severely modified by a transient change in the crustal rheological structure associated with magmatic underplating.     

天山北麓活动背斜区河流阶地与古地震事件

利用航空遥感照片和Google earth卫星影像,对天山北麓独山子活动背斜区奎屯河两侧的河流地貌进行解释,结合野外调查发现,奎屯河流经独山子背斜段发育7级基座阶地,阶地基座为上新统独山子组泥岩,其上部为2.5 ～ 15m厚的砂砾石层和砂质黏土.在开挖或剥离的各级阶地堆积物剖面中采集细粒堆积物样品,实验室中采用细粒石英...     

被动陆缘盆地陆隆斜坡对盐构造形成的影响 ——来自物理模拟实验的启示

被动陆缘盆地盐构造形成的影响因素及时空演化分析受到了国内外学者的高度重视.丰富的油气资源促进了被动陆缘盆地地震资料品质的不断提升,高精度地震数据的解译结果表明,被动陆缘盆地盐层下的地形往往具有大型的起伏特征,而前人在基底构造形态对盐构造形成影响方面的研究并未取得共识,仍需要深入研究和探讨.为此,本文基于前人的研究认识,...     

Magnetic and velocity fields of active regions

We have observed about 15 active regions on the Sun, with the Advanced Stokes Polarimeter and Dick Dunn Telescope at NSO/SP to map the Stokes parameters in the photospheric Fe 6302.5 Å and chromospheric Mg I 5173 Å lines, during 1999‐2002. The observations are corrected for dark current, gain, instrumental polarization and cross‐talk using ASP pipeline. The wavelength calibration is carried out using the O₂ telluric line 6302 Å which is also present in the observations. The photospheric and chromospheric longitudinal magnetograms are made from the Stokes V profiles, which were intercalibrated with the Kitt Peak magnetograms. The plasma motions are inferred from the line bisector measurements at different positions of the spectral line. In this paper we present the height dependence of Doppler velocity scatter plots of a sunspot in the photospheric Fe I 6302 Å line.     

华北克拉通北缘柴胡栏子金矿富甲烷流体包裹体的发现及地质意义

柴胡栏子金矿位于华北克拉通北缘赤峰-朝阳金矿集区西段,是区内典型的石英脉型为主的金矿床,也是赤峰-朝阳地区首次发现的含大量单相甲烷包裹体群的金矿床.矿体呈脉状产于太古宙建平群大营子组下岩段含石墨绢云母片岩切层断裂中,金主要产出在蚀变含石墨绢云母片岩和石英脉中.根据野外观察和包裹体测温结果,将柴胡栏子金矿流体成矿过程划分...