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井水位前驱波普遍性问题的探讨 总被引:3,自引:1,他引:2
以山西、河北、内蒙等地5口映震能力较强的地下水位观测井为研究对象,对井水位前驱波普遍性问题进行了探讨.结果表明,强震井水位前驱波现象较为普遍,其比例可达65.1%(41/63);相同地震不同观测井前驱波特征各不相同,同一观测井在不同地震前的特征也各异,这可能与不同观测井具有不同的井-含水层结构以及不同地震前有着不同的震源参数有关;与单井水震波相比,震前有前驱波记录的次数略低于水震波,其比例在39.7%~50.7%之间;震前有前驱波记录的观测井占研究区观测井总数的比例可达66.7%. 相似文献
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统计了银川台GS15-215型定点重力仪记录的数字化观测资料,分析了不同震级和不同震中距范围内的地震发生后前驱波的出现规律,发现银川台重力观测记录曲线中出现震前前驱波的比例比较小,尤其是震级较小的地震几乎无震前前驱波出现,对大地震前出现前驱波的比例、出现的时间及特征进行了归纳总结,以期为相关研究提供参考。 相似文献
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地下水动态的超远强震异常问题 总被引:5,自引:0,他引:5
自20世纪80年代以来,在我国地震地下水动态观测网中陆续发现井水位在超远距离强震前的异常现象。这种异常表现为井水位的振荡与阶变,多出现在震前几小时至几天内,有一定的重现性。对这种异常的形成机制有多种不同观点,其中具有代表性的有强震的前驱波作用观点与强震孕育的林构造牵动观点等。 相似文献
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分析华北地区 2 0余年地下水动态与强地震活动的关系 ,发现部分井水位动态在几次强地震前短期阶段出现形态相似的下降变化 .其特征表现为水位以突变下降或加速下降开始 ,转折后变为速率较缓慢的上升 ,其幅度比下降幅度小得多 ;地震发生在水位缓慢上升过程 ,震时或震前水位大幅度上升 .这种下降形态的异常在华北地区上百口观测井中记录虽然不多 ,但是在几次强地震前不同的井记录了形态相同的水位变化过程 .表明地下水的地震前兆异常具有一定的重现性 ,在不同的强地震前可重复出现 .因此 ,有必要研究这类异常的成因及其与强地震活动的关系 . 相似文献
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分析华北地区20余年地下水动态与强地震活动的关系,发现部分井水位动态在几次强地震前短期阶段出现形态相似的下降变化. 其特征表现为水位以突变下降或加速下降开始,转折后变为速率较缓慢的上升,其幅度比下降幅度小得多;地震发生在水位缓慢上升过程,震时或震前水位大幅度上升. 这种下降形态的异常在华北地区上百口观测井中记录虽然不多,但是在几次强地震前不同的井记录了形态相同的水位变化过程. 表明地下水的地震前兆异常具有一定的重现性,在不同的强地震前可重复出现. 因此, 有必要研究这类异常的成因及其与强地震活动的关系. 相似文献
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对山西、河北、北京和江苏地区14口观测井的前驱波记录次数进行了统计分析,并给出了前驱波记录次数占统计年份地震总次数的百分比;利用Cooper等人推导的井-含水层系统放大因子表达式,分析了井-含水层系统的特征参数与前驱波响应能力之间的关系. 研究结果表明,井-含水层系统对前驱波的响应能力大小与含水层的固有周期存在一定关系,即固有周期越大,记录前驱波的能力越强; 井-含水层系统对前驱波的响应能力大小还与导水系数和井孔半径平方的比值大小有关,该比值越大,响应能力越强. 相似文献
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The determination of the coefficient of viscosity of eruptive products gives useful elements to the knowledge of possible variations of composition and physical conditions of the magmas. 相似文献
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As is known, the secular deceleration of the Earth's diurnal rotation is explained mainly by the tidal friction in the ocean. Below we consider this mechanism in some detail, taking into account also elastic deformations of the mantle under the action of ocean loading and the interaction between the tide-generating body, ocean tidal wave, liquid outer core, and solid inner core. It is shown that elastic displacements of the core-mantle boundary under the action of ocean loading are of about the same amplitude and phase as the elastic loading displacements of the Earth's outer surface. As a result, side by side with the mechanism of secular deceleration of diurnal rotation of the mantle, there are also (1) the opposite mechanism of secular acceleration of diurnal rotation of the outer liquid core and of the solid inner core and (2) the mechanism of excitation of differential rotation in the liquid core. Taking these effects into account, we compare theoretical and modern observed data on the eastward drift of the solid inner core. It is shown that the best agreement may be obtained if the turbulent viscosity of the liquid core is about 2 × 10
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Poise 相似文献
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Geomagnetism and Aeronomy - The magnetic evolution of the active region of the Sun at the level of the photosphere has been studied. Magnetic synoptic maps of the 2007 Kitt Peak Observatory were... 相似文献
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The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth. 相似文献
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Studia Geophysica et Geodaetica - 相似文献
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地震激励下处于深水中的桥墩和周围水体的相互作用将对桥梁结构的动力响应产生较大影响。首先对地震作用下水-桥墩的相互作用理论做了概括,给出了动水压力对桥墩的作用效应及各自的适用范围;对主要的三种考虑流固耦合效应的分析方法做了对比,探讨了地震作用下影响水-结构相互作用的主要因素,并对今后的研究提出了建议。 相似文献
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V. E. Pavlov T. Yu. Tolmacheva R. V. Veselovskiy A. V. Latyshev A. M. Fetisova I. V. Bigun 《Izvestiya Physics of the Solid Earth》2017,53(5):702-713
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary. 相似文献
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Summary A simple model is proposed suitable for studying the effect of the ground layer of the atmosphere, polluted by aerosol, on the albedo. This model is founded on solving the equation of transfer of radiative energy. The numerical results are discussed, particular attention being paid to the analysis of errors due to neglecting the multiple reflection of solar radiation on the aerosol particles. A method which would also include the multiple reflection is proposed, and the conditions under which the presence of the aerosol is responsible for an increase or decrease of the solar radiation balance on the Earth's surface, are analysed. 相似文献