闽东南大陆边缘构造特征及泉州海外大震构造环境分析          下载免费PDF全文

吕浩江  雷土成  陈辉琼  杨志辉 《地震工程学报》1995,17(2):76-81

闽东南大陆边缘构造活动，自晚更新世以来，断裂活动以继承性差异升降作为主要特点，本文分析了１６０４年１２月２９日泉州海外８级大震与该区断裂活动的关系，并对该次大震震源断层面错动方式进行了讨论。  相似文献   

天水地区大地电磁测量及深部电性结构   总被引：3，自引：0，他引：3       下载免费PDF全文

刘宝勤  朱佐全  贾政  郭万武  李柱国  张文仁  屈健鹏 《地震工程学报》1995,17(4):70-78

天水地区的大地电磁测量结果表明，在４３ｋｍ左右的深度上普遍存在高导层，这可能是壳幔过渡带的反映。岩石圈厚度大约９５－１１０ｋｍ。在天水太京附近可能存在一条大型近东西向地壳－岩石圈构造带，在秦安以北的叶堡和陇城附近可能也存在一条近南北向的大型地壳－岩石圈构造带，它们都是不同构造单元的分界线。１６５４年天水８级大震可能与深部热异常引起的热应力有关。  相似文献   

沂沭断裂带内构造体系特征及其复合现象     

王林祥 《吉林大学学报(地球科学版)》1987,(1)

沂沭断裂带是山东境内一条从北向南展布的巨大断裂带,主要由鄌郚—葛沟、沂水—汤头、安丘—莒县和昌邑—大店断裂组成。该带内构造体系的复合现象很发育,可概括为:褶皱构造的迭加;断层力学性质的迭加;断裂间的穿切;结构面的方位改变和岩脉或矿脉的穿切等。 根据构造形迹力学性质和构造体系的特征,确定上述构造形迹归属于东西构造带和新华夏系。  相似文献   

新的太阳系起源假说——再论巨星依次分离说     

牛广林 《吉林大学学报(地球科学版)》1987,(3)

本文以太阳系星球的物质状态、形态面貌、体积、物质密度、运动速度、运动方向和角动量等作为根据,研究它们在宇宙空间上的分布特点、相互关系、内在联系以及规律的基础上,提出太阳系(乃至宇宙星球)是在46亿年前,宇宙中一个巨大灼热的星球,在高速度左旋旋转(公转和自转)运动的过程中,从尾部分离出来的物质,经过……恒星、行星和卫星依次波状旋转分离运动产生的。  相似文献   

北京西山水平分层剪切流变构造初探   总被引：7，自引：2，他引：7  

单文琅  傅昭仁 《地球科学》1987,(2)

对比国内外关于变质岩区构造变形序列的实例,可知第一世代的构造变形几乎都以发育不同尺度的强烈扁平化平卧褶皱和有关的轴面流劈理或片理,以及近水平的韧性剪切带等构造组合为特征。北京西山的情况也不例外。这可能代表变质岩区早期构造变形的一种普遍模式,可能是地壳较深构造层次发生大规模透入性水平剪切流变的反映  相似文献   

Seasonal and diurnal variability of thermal structure in the coastal waters off Visakhapatnam     

B. Prabhakara Rao  V. Ramesh Babu  P. Chandramohan 《Journal of Earth System Science》1987,96(1):69-79

Seasonal and diurnal variability of thermal structure in the coastal waters off Visakhapatnam has been examined in relation to the flow field and surface winds utilizing the hourly data of temperature and currents taken at a fixed location over a tidal cycle at monthly intervals. The coastal currents in the pre-monsoon period and strong near-surface winter cooling processes affect the thermal structure of the coastal sea. Upwelling which is predominant during March to May with an intermittent relaxing event helps in the development of a strong layered thermal structure while convective mixing due to winter inversions during November to February causes weak thermal gradients in the water column.  相似文献   

Travel-time residuals and three-dimensional velocity structure of Italy     

Roberto Scarpa 《Pure and Applied Geophysics》1982,120(3):583-606

Jeffreys-Bullen P and PKP travel-time residuals observed at more than 50 seismic stations distributed along Italy and surrounding areas in the time interval 1962–1979, indicate the complex velocity pattern of this region. Strong lateral velocity inhomogeneities and low velocity zones are required to explain the observed pattern of residuals. In particular, late arrivals of about 1 sec are observed in the Apenninic mountain range, requiring both greater crustal thickness and low velocity layers, coherent with seismic refraction data and surface wave dispersion measurements. The seismic stations located in the Western and Eastern Alps indicate the presence of high velocities. In the Western Alps the strong azimuthal variation of residuals and the high values of early arrivals have a close relationship to the Ivrea body, an intrusive crustal complex characterized by a velocity as high as 7–7.2 km/sec.A travel-time inversion performed with theAki et al. (1977) block model, confirms the peculiar characteristics and the sharp variations in the lithosphere of the whole Italian region, with values of velocity perturbations between many adjacent blocks, ranging in size from 50 to 100 km, and independent from the earth parametrization chosen, reaching values up to 10% in the lithospheric part and 5% in the asthenosphere. 3-D inversion requires also high velocity along the Tyrrhenian coastal margin, equivalent to an uprise of major crustal and lithospheric discontinuities along this part of the Italian peninsula. Moreover low velocity material must be present in the northern part of the Adriatic foreland, in the lithosphere-asthenosphere system, closely related to the stress and seismicity pattern, and the lateral bending of the lithosphere in the same region.  相似文献   

Statistics on the sizes and internal structures of rainshowers     

R. R. Rogers  K. J. Keen  A. P. Schwartz 《Pure and Applied Geophysics》1983,121(1):133-166

A large sample of radar reflectivity data from essentially a full summer of operation was analyzed to determine the horizontal extents and internal structure of rain areas observed at altitude levels from 2 to 10 km. Results are given on the size distributions of individual cells or patches defined by reflectivity thresholds approximately 4 dBz apart, on the dependence of mean size on altitude and reflectivity threshold, and on the interior structure of the patches as characterized by the number and sizes of higher-threshold patches contained in each echo. In a more detailed analysis of internal structure, the data were restricted to convective echoes in which certain prescribed reflectivities, ranging from about 30 to 50 dBz, were exceeded. It was found that the dependence of mean quantities, such as patch area, on reflectivity and altitude could be approximately described by simple functions, but that the scatter of observations about the mean was usually large.  相似文献   

高表面活性矿物对Zn~(2+)的吸附机理及其环境意义     

吴平霄  廖宗文  毛小云 《矿物学报》2001,(3)

本文利用高表面活性矿物蒙脱石、蛭石、沸石在一定的介质条件下对Zn2 +进行吸附实验研究。蒙脱石和蛭石对Zn2 +的等温吸附线呈双“S”型 ,而沸石对Zn2 +的等温吸附线则呈“Langmuir”型。三种矿物对Zn2 +的吸附容量大小顺序为 :蒙脱石 >蛭石 >沸石。运用粉晶X射线衍射、红外光谱、差热及热重分析等技术对矿物及矿物吸附Zn2 +后的结构特征进行了研究。结果表明 ,蒙脱石吸附锌后其层间域中吸附锌大量水解形成新的物相 ,而蛭石与沸石吸附锌后水解很少。这为利用高表面活性矿物控制和治理环境污染及其可循环利用提供了理论依据。  相似文献   

Hydrogen recombination lines near 327 MHz−II: A Galactic plane survey with a 2°×6′ beam     

D. Anish Roshi  K. R. Anantharamaiah 《Journal of Astrophysics and Astronomy》2001,22(1):81-119

In a previous paper we presented a low-resolution (2°×2°) survey of radio recombination lines (RRLs) at 327 MHz in the longitude rangel=330° to 0° to 89°. In this paper, we present the results of a higher resolution (2°×6′) survey of RRLs from seven 2°-wide fields and two 6°-wide fields in the same longitude range. Observations were made using the Ooty Radio Telescope (ORT). A total of 252 spectra that were obtained are presented. RRLs were detected in almost all the individual positions within the fields withl<35° and at several individual positions within the fields in the longitude rangel=35° to 85°. Detailed analysis of the data towards the field centered at G45.5+0.0, shows that the line emission consists of discrete zones of ionized gas. The angular extent of these zones are likely to be one degree or more corresponding to a linear size of >110 pc at the kinematic distance.  相似文献