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地震和火山都反映了地球表层的构造活动,因而地震活动区往往也是火山活动区。根据全球大震、火山活动目录,分析研究了全球地震、火山分布的特征。描述了各区的地震、火山活动分布,总结了地震、火山活动强度的时、空分布特征。全球地震、火山活动可以分为碰撞带、大陆区和大洋区。大陆地震以其片状的分散分布而不同于板块边缘的带状分布,大陆火山活动比大洋火山更受应力场的影响。大洋区地震活动相对较弱,岩浆活动主要是平静的岩浆溢出与洋中脊的扩张,往往没有形成火山喷发。有记录的火山喷发主要来自深部地幔的热柱。俯冲-碰撞活动区地震活动与火山喷发最强烈,大角度俯冲的弧后火山活动最强,当板块运动方向与板块边缘走向成小角度相交时,缺少正面俯冲的动力,火山活动相对平静。>500km深震的地段,火山活动较弱。火山与地震强烈活动的大多在大地水准面(Geoid)异常高的区域。地震与火山平均纬度随时间表现出同步的变化外,火山和大震活动也显示了大致同步的变化 相似文献
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J. L. Rubinstein J. E. Vidale J. Gomberg P. Bodin K. C. Creager S. D. Malone 王小琼 《世界地震译丛》2007,(5):30-35
在火山附近观测到非脉冲的地震辐射或“颤动”已有很长时间了(McNutt,2005),最近在消减带附近也观测到了类似现象(Obara,2002)。尽管非火山颤动观测资料的数量一直持续增加,然而人们对其发生机理依然知之甚少。有人将非火山颤动归结为流体的运动(Obara,2002;Kaoet al,2005;McCauslandet al,2005;Katsumataand Kamaya,2003;Seno and Yamasaki,2003),然而大地测量学观测发现非火山颤动与有规则间隔的慢滑动事件具有很好的一致性(Rogers and Dragert,2003;),这让另外一些人将非火山颤动发生的原因解释为板块边界的滑动(Rogers and Drager… 相似文献
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板块俯冲时海沟位置存在不变、前进和后撤 3种情况 ,后撤俯冲可能造成弧后扩张 .层析成像等资料显示 :太平洋板块低角度俯冲到欧亚板块之下后没有穿透 670km相变界面 ,而是平卧于该界面之上 .这种平卧过程可能始于 2 8Ma前 .地球动力学计算表明 :俯冲板片前缘触及上下地幔相变界面而受阻平卧时 ,有利于形成后撤俯冲和弧后扩张 .中国东北火山形成很可能属于这种后撤俯冲、远离海沟陆内弧后引张、地幔热物质上涌、减压熔融的情况 . 相似文献
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腾冲火山活动构造动力学研究 总被引：7，自引：1，他引：6
利用腾冲火山区域 (10°～ 35°N ,90°～ 10 6°E) 1990～ 1998年 6 6 0个地震基本参数和震源机制资料 ,以及原先已作过 370多个强震震源参数资料[1 ] ,并结合本区域的地质资料 ,对本区的火山作用的构造动力学以及腾冲火山与印度、欧亚两大板块的关系作了探讨。研究表明 ,腾冲火山区西侧的印度板块对缅甸板块和包括腾冲在内的滇缅泰板块作用 ,大致在 0～ 10 0km作用机制表现为斜俯冲 ,10 0km以下表现为碰撞挤压作用。分析还表明 ,腾冲火山的形成与活动 ,与印度板块和亚欧板块两个大陆板块俯冲、碰撞 ,及在缅甸那加山、阿拉干山板块缝合线产生的斜俯冲和侧面挤压剪切作用密切相关 ,它应该属于两个大陆板块碰撞型板缘火山。 相似文献
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长白山火山的历史与演化 总被引：3，自引：0，他引：3
长白山火山跨越中朝两国,在我国境内包括天池火山、望天鹅火山、图们江火山和龙岗火山,火山活动从上新世持续到近代,是我国最大的第四纪火山分布区。长白山火山的母岩浆是钾质粗面玄武岩,将长白山火山岩区称钾质粗面玄武岩省,岩浆结晶分异作用和混合作用主导了岩浆演化过程。天池火山之下地壳岩浆房和地幔岩浆房具双动式喷发特点,一方面来自地幔的钾质粗厨玄武岩浆直接喷出地表;另一方面钾质粗面玄武岩浆持续补给地壳岩浆房,发生岩浆分离结晶作用和混合作用,导致双峰式火山岩分布特征和触发千年大喷发。西太平洋板块俯冲-东北亚大陆弧后引张是长白山火山活动的动力学机制。 相似文献
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扬子板块东北缘中元古代的大地构造划分 总被引：1，自引：0，他引：1
扬子板块东北缘存在四条主要的中元古代变质带,自南向北依次为江南变质带、沿江变质带、云台一张八岭变质带和连云港一泗阳变质带。它们分别为中元古代的古弧后盆地、火山岛弧、裂谷及弧前盆地,扬子板块东北缘中元古代为活动大陆边缘构造体系。苏（北）胶（南）变质造山带应解体,其中一部分属扬子大陆边缘体系。 相似文献
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流体/水分在地球演化过程中具有重要作用,它的存在可以提高地质体的扩散及蠕变,降低岩石/地幔的固液相限,对地质体的地球物理性质、地质灾害诱发、地质构造演化等都有着重要的作用.在板块俯冲区,流体/水分的影响贯穿了整个动力学过程,但板块深部脱水还存在着争议,且目前系统地研究水分在整个俯冲中的迁移过程及其地球物理意义的工作还较少.本次研究以我国东北地区为例,借助于地球动力学数值模拟,利用二维岩石化学-热-力学耦合的数值计算程序,建立西太平洋板块向欧亚大陆岩石圈俯冲的数值模拟模型,模拟了板块俯冲整个连续动力学过程中流体/水分的迁移过程.模拟与分析结果表明,板块俯冲过程中水分的迁移过程可分为三个阶段:洋壳水化、板块浅(中)部脱水、板块深部脱水.进一步揭示了洋壳水化过程中水分渗流通道形成、水分渗流以及板块及地幔物质水化反应的机制;解释了板块浅(中)部脱水过程对火山岛弧、弧后盆地及低速异常带形成的作用,以及对~410 km不连续带的影响;模型演化过程中观察到的板块深部脱水现象说明了存在板块深部脱水的可能性,而且板块深部脱水可以较好地解释部分内陆火山以及部分地区地幔柱(岩浆羽)和深源地震的成因.研究展示了板块俯冲过程中水分运移的地球物理意义. 相似文献
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2004年的苏门答腊—安达曼M9级地震将俯冲的印度—澳大利亚板块和仰冲的缅甸板块分裂开。这次地震的形变属于三维问题,为此我们构建了有限元模型进行模拟,以说明俯冲板块、弧前、火山弧及弧后的物性分布。同震形变的模拟使用一种基于协议的方法。该方法考虑俯冲带的地质复杂性,使用有限元模型反演估计断层滑动分布。结果表明不考虑俯冲带中物性差异的形变预测的灵敏度比近场GPS的测量误差可大一个数量级还多。本文介绍的基于有限元模型的技术可用于地质上相符的形变模型,提高同震与震后形变、应力耦合及海啸发生的基于模拟技术的评估可靠性。 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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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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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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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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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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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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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