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为了清晰认识发生于青藏高原西北部2008年与2014年的两次于田MS7.3地震发震构造环境与构造地貌特征,本文利用DEM(数字高程模型)数据分析"喀喇昆仑—西昆仑—康西瓦地区"的地形地貌特征,结合区域活动断裂研究资料、相对于塔里木盆地的两期GPS速度场资料和区域运动学特征等讨论两次MS7.3地震所处的青藏高原西北部区域构造环境和地壳运动学特征,分析喀喇昆仑断裂、阿尔金断裂康西瓦段、龙木错-邦达错断裂及贡嘎错断裂所围限的西昆仑地块的地质构造背景、阿尔金断裂西南端发震断裂活动性及孕震环境等发震构造基本条件;进而利用"地形剖面"方法及断裂分布特征分析震源区的地形地貌特征,给出晚第四纪以来的地貌形态与发震构造的关系,从区域构造地貌学和GPS地壳运动学的角度探讨中上地壳变形特征及孕震过程;最后讨论区域孕震构造、克尔牙张性裂谷演化过程和地球动力学背景等。通过地形剖面及区域地貌综合分析新疆于田2008年MS7.3拉张型发震构造和2014年MS7.3走滑拉张型地震的发震构造特点的区别,认为2014年发生的地震可能与2008年MS7.3地震同震库伦应力变化、触发过程及震后变形过程密切相关,并且青藏高原西北部地区存在明显的东西向拉张性构造单元,可能与青藏高原10~15 Ma以来的地壳减薄过程有关。 相似文献
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青藏高原北部地区弱震空间图像特征与中短期地震预测方法 总被引：3，自引：1，他引：2
通过对青藏高原北部地区31次地震的研究,确定了震前地震活动图像的中短期预测指标以及中期向短期过渡的异常判据及预测方法。研究结果表明,中强地震前普遍存在地震空区、弱震条带、前兆地震或震群、地震活动增强和平静等异常图像,所表现出的异常时间存在很大的差异。具有中短期特征的弱震空区(段)和条带一般出现在震前1～3a,平均持续时间1a,在空区解体后1～6个月发生地震。大多数前兆地震或震群活动属于短临异常,一般出现在震前几天至6个月,震级差为1．0～2．3,距离震中5～60km,空间上主要集中在祁连山地震带。地震活动增强以应力集中为主,属于短期异常特征。异常图像在时间上表现为中期阶段以孕震空区、弱震条带、地震活动增强和平静等异常,异常比较显著且不同步;短临阶段出现前兆地震和地震空区停止活动而形成的临震前的相对平静。异常图像在空间上具有较明显的分区性,与区域活动构造有一定的关系。 相似文献
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大量观测事实表明 ,赋存于地壳深部的流体 (水、气、油 )作为弹性介质 ,对深层地壳应力的分布、变化、转移过程及地震孕育、发生等有着较为灵敏的反映。地震的形成与区域构造应力活动强度密切相关 ,这种大范围的区域应力作用会形成多个应力集中点 ,在众多应力集中点上可产生地下流体前兆异常变化。在对新疆地下流体数十年的监测中 ,发现强震前出现大量与地震有关的由区域构造应力活动引起的前兆异常 ,异常范围广且种类繁多 ,它们在成因、特征上与震源应力活动的前兆异常明显不同 ;这种地下水位地震前兆异常场 ,不能完全孤立地与单个地震事件相对应 ,应充分考虑到它与一组或系列地震有关 ,而这些地震往往与块体挤压、断裂活动等区域性的应力活动有关。因此 ,正确区分并掌握其不同的特性 ,对地震预报具有一定的意义 相似文献
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地震前兆场物理模式与前兆时空分布机制研究(二)
——强震孕育时应力、应变场的演化与地震活动、地震前兆的关系x,auto,auto,415px);}style> hf=httprztl.com >business 总被引：10，自引：4，他引：10 
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下载免费PDF全文 分别研究构造块体内有多个震源体和单个震源体孕育时，应力集中过程、时空分布规律及其与地震活动、地震前兆的关系．结果表明:① 当区域应力场增强到相当水平时，破裂开始在某个或某些块体内发生，区域应力场将随着时间而变化，强震的成组性是这个动态应力场演变的结果．在此过程中，多个高应力集中区的存在与发展，有可能导致震前异常与地震关系的多样性；② 孕震块体的应力变化过程一般显示出非线性，在经历了长期弹性变形后，从进入非弹性变形阶段到主破裂前，可能经历不止一次的非弹性变形与断层软化过程；与此相应，孕震块体中的应力、应变场要表现出复杂的时空演化图象；受应力、应变控制的地震前兆场必然表现出多方面的复杂性. 相似文献
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分别研究构造块体内有多个震源体和单个震源体孕育时．应力集中过程、时空分布规律及其与地震活动、地震前兆的关系．结果表明：①当区域应力场增强到相当水平时，破裂开始在某个或某些块体内发生，区域应力场将随着时间而变化，强震的成组性是这个动态应力场演变的结果．在此过程中，多个高应力集中区的存在与发展，有可能导致震前异常与地震关系的多样性；②孕震块体的应力变化过程一般显示出非线性，在经历了长期弹性变形后，从进入非弹性变形阶段到主破裂前，可能经历不止一次的非弹性变形与断层软化过程；与此相应，孕震块体中的应力、应变场要表现出复杂的时空演化图象；受应力、应变控制的地震前兆场必然表现出多方面的复杂性． 相似文献
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通过对1986年门源6．4级地震以来青藏高原东北部发生的一系列6级强震时空分布特征的研究，提出了这些地震为成组孕震的观点，并从背景空区、诱发地震、地震活动增强及前兆异常的突变等方面论证了成组孕震的可能性。 相似文献
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D. M. Pechersky A. A. Lyubushin Z. V. Sharonova 《Izvestiya Physics of the Solid Earth》2010,46(7):613-623
The data on geomagnetic reversals are compared with the changes in the organic world and with the lower-mantle plumes. The
times of the formation of plumes and the times of their appearance on the Earth’s surface relate to the intervals characterized
by the different frequencies of geomagnetic reversals, i.e., there is no interrelation between the formation of plumes and
the frequency of the changes in the geomagnetic field polarity. At the same time, a certain synchronism is observed between
the frequency of the geomagnetic reversals and the boundaries of the biostratigraphic ages, i.e., the changes in the organic
world in the long-period range. A hypothesis is proposed, which explains the change in the sign of the geomagnetic field by
the combined effect of the irregular rotation of the internal core relative to the mantle and the changes in the slope angle
of the axis of the Earth’s rotation, which, in turn, results in synchronous events on the Earth’s surface: the rates of changes
in the organic world. 相似文献
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Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan. 相似文献
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Prof. Dr. W. A. Heiskanen 《Pure and Applied Geophysics》1958,41(1):1-18
Summary The author mentions the aims of the World-wide gravity project he established in the Ohio State University in Columbus, in 1950. He outlines the practical procedure of the gravimetric computations of the undulationsN and the vertical deflection components and and emphasizes that only by the global international cooperation and additional gravity observations at sea carried out during the last decade it has been possible to gather to Columbus the needed gravity material. Since there exist still large gravimetrically unsurveyed areas it is of vital significance to study what gravity anomalies are best to be used for these regions. The given figures concerning the accuracy of theN, and , estimated theoretically and obtained in practice, indicate that in the gravimetrically well surveyed parts of the world like in Europe and the United States we can get gravimetrically on basis of existing gravity material theN-values with accuracy of about 5–10 meters, and and with the accuracy of about 1. The geoid undulationsN are already computed in Columbus for more than 6000 points of the northern hemisphere. The sample maps show the interesting geoid of Europe and vicinity between the latitudes 60° and 30° and longitude 5° W and 30° E, drafted on basis of more than 1000N-values computed at the corners of 1°×1° squares. It is interesting to realize that the geoid undulations in all this area are positive, the extreme values being between 40 and 50 meters. The geophysical significance of the geoid maps of this kind is pointed out. 相似文献
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综合APIA、HONOLULU、PAMATAI 3个地磁台三分量的11年周期变化的形态后,可定性地提出该变化源于内场。如内源为核幔边界的电涡流,则其中心点应位于3台之间。 相似文献
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The global database on the paleointensity, containing determinations of the virtual dipole moment (VDM) for a stable (normal) regime of the geomagnetic field in a time interval of up to 3.5 Ga, is supplemented by new VDM determinations and analyzed. The field generation process started no later than 3–3.5 Ga (earlier data are absent) at the stage of the Earth’s core formation. Since that time, the dipole value has differed from its present value by no more than an order of magnitude, and the deviations that have already been detected tend toward smaller values. The distribution of VDM values in the time interval 0–400 Ma is bimodal, which apparently reflects the presence of two different generation levels of the geomagnetic field distinguished by a relatively large value (close to the present field value) and a relatively small value (approximately half as large as the present value). The total duration of decreased VDM values appreciably exceeds that of increased VDM values (179.1 and 28.6 Myr, respectively). On the whole, data on the paleointensity do not contradict the hypothesis about the dipole nature of the field over the last 400 Myr; however, the number of determinations at high paleolatitudes is too small to draw decisive conclusions on the validity (or invalidity) of the dipole field approximation based solely on paleointensity data. 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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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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Geomagnetism and Aeronomy - The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the... 相似文献