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41.
Zedník J. Pospíšil J. Růžek B. Horálek J. Boušková A. Jedlička P. Skácelová Z. Nehybka V. Holub K. Rušajová J. 《Studia Geophysica et Geodaetica》2001,45(3):267-282
In the time span from January 1995 to December 1999 the Czech National Seismological Network (CNSN), consisting of ten permanent digital broadband stations, several local networks and two data centers, detected and recorded 9530 regional natural seismic events, 27 greater than magnitude 2. Most of these events were located by the Czech Seismological Service (CSS), and the most prominent of them were analyzed in detail. A large number of quarry blasts were recorded as well but were not included in the analysis. We provide basic information on the configuration of the CNSN and on the way of routine data processing employed by the CSS in this paper. The over-all regional seismicity monitored by the CNSN in 1995–1999 is briefly reviewed. The main results of observations and evaluation of the local (NW-Bohemia/Vogtland, South Bohemia, Sudeten) and induced (Kladno, Píbram, Upper Silesia, Lubin/Poland) seismic activity within this period are presented in a condensed form. Finally, a summary on macroseismic observations on the territory of the Czech Republic in 1995–1999 is also presented. 相似文献
42.
西南三江地区造山演化过程及成矿时空分布 总被引:8,自引:0,他引:8
三江地区单凭“一次造山”是难以圆满解释的。本文试以“多次造山”多期成矿”的思路作出合理说明。晚古生代-中生代早期多岛海造山阶段,羌塘弧、江达弧和临沧弧应为前锋弧,其后由一系列弧后盆地和岛弧或残余弧(或微大陆)组成。中生代中-晚期为陆内俯冲造山阶段,推测金沙江带、哀牢山带和龙门山-锦屏山带为俯冲主边界,从而形成本区燕山期重熔型花岗岩带,控制相应矿产的分布特征。新生代陆内转换造山阶段,造成特征的构造-岩浆-成矿带,具有生成大型或超大型矿床的潜力。 相似文献
43.
从"统计预测"、"经验预测"、"物理预测"的角度讨论了世纪之交地震预测预报研究的国际进展。"统计预测"包括地震预测预报方法的统计检验、"统计地震学",以及统计物理在地震预测预报中的应用;"经验预测"包括搜索可能的前兆异常的尝试、建立将可能的前兆异常现象与地震孕育过程联系起来的简单模型、发现对地震预测预报研究具有重要意义的新现象,以及地球介质变化的动态监测试验;"物理预测"包括地震孕育和发生的物理模型、地震断层带性质的观测和实验研究,以及对震源的直接探测和钻探。讨论了"统计预测"、"经验预测"、"物理预测"之间的关系,对"把经验预测或统计预测变成物理预测"的发展战略提出质疑。 相似文献
44.
45.
地震学中的"暗物质"—"静地震"与地震预测研究的未来 总被引:1,自引:0,他引:1
正如暗物质的研究是理论物理学和宇宙学中的一个关键性问题,静地震的研究也将为地震预测研究的发展提供一个历史性的机遇. 相似文献
46.
核测井曲线高分辨率处理技术及其应用 总被引:1,自引:0,他引:1
着重探讨了放射性测井曲线中自然伽马测井曲线、补偿中子测井曲线和补偿密度测井曲线的高分辨率处理方法及其应用效果。对于自然伽马及自然伽马能谱测井曲线,采用反褶积技术和有效的噪音压制技术;对于补偿中子测井曲线和补偿密度测井曲线采用了改进的α因子法。可以发现:高分辨率处理技术可明显地改善有关曲线的纵向分层能力;处理后的曲线与岩心柱状图及与微球、微电极等高分辨率曲线进行对比,其相关性有很大的改善;应用高分辨率处理后的曲线求薄层的泥质含量等参数,其相对误差明显下降。 相似文献
47.
用地层倾角测井资料解释复杂构造的方法 总被引:1,自引:0,他引:1
倾角测井矢量图可以标示出井眼范围内各深度点的地层产状,一定的地层构造形态在矢量图上有一定的倾角矢量组合模式。通过正演计算,总结出了19种褶曲和断层等构造组合模式的样板及在一口井内各构造模式间的“串”、“缺”、“嵌”连接规律。对照组合模式样板进行矢量组合模式识别,采用“倾角矢量逐点叠加法”,可把井眼范围纵向排列的倾角矢量转换成任意方位的地层视产状,绘制构造剖面图。用多个剖面的地层空间坐标数据可绘制倾角构造平面图,确定钻遇构造的形态。据此原理,编制了一套倾角测井构造解释软件系统。 相似文献
48.
Daily full-disk solar maps obtained at 37 GHz in the years 1979, 1980, 1981, 1982, 1987, 1988, 1989, 1990, and 1991 are analysed and compared with full-disk solar maps in H. A search for a difference in the measured angular rotation velocity for two classes of microwave low-brightness-temperature regions (LTRs), associated and not associated with H filaments, is performed. Procedures with and without statistical weights, assigned to angular rotation velocities according to the tracing time, are applied and the statistical significance of the results is discussed. A higher angular rotation velocity is measured for LTRs associated with H filaments than for the not-associated ones. This angular velocity difference is interpreted as a consequence of a height difference between these two types of LTR tracers. Changes of the solar differential rotation velocity during the activity cycle measured using LTRs as tracers are explained by the measured cycle-dependence of the association rate between LTRs and H filaments. Similarly, the north–south asymmetry in the solar rotation velocity measured tracing LTRs is explained by the measured north–south asymmetry in the association rate between LTRs and H filaments. The rotation velocity of LTRs and H filaments is on the average more rigid in comparison with sunspots. 相似文献
49.
Adam Ružčka 《Astrophysics and Space Science》2003,284(2):519-522
A simple sticky-particle numerical model has been developed in order to check whether extended structures of gas created due
to the dynamical evolution of the Galaxy and the Magellanic Clouds system can be explained as remnants of a tidal interaction.
Influence of dissipative nature of gaseous medium has been taken into account. The most remarkable features are: the Magellanic
Stream, the common HI envelope surrounding both the LMC and SMC and the bridge extended between the Clouds. In contrast to
previous works of Murai and Fujimoto (1980), Gardiner et al. (1994) and H and Rohlfs (1994) no presumptions were done on the
actual galactocentric velocities of the Magellanic Clouds. The mean values of the LMC and SMC velocity vectors obtained from
the Hipparcos proper motion measurements (Kroupa and Bastian, 1997) were used in order to verify whether they allow to reproduce
the observed HI distribution. Numerical simulations showed that tidal forces are really significant for the evolution of extended
structures such as the Magellanic Stream but this approach becomes unsufficient for the internal regions of galaxies where
self-gravity and dissipative properties of the gas cannot be neglected. More precise proper motion measurements are urgently
needed.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
50.