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本文利用地震资料并结合地质资料,讨论了印度板块与欧亚板块在中国周边的相互作用及其对中国应力场的影响,指出两板块在喜马拉雅山前断裂地区碰撞,碰撞边界向西延续到35°N,74°E附近,其主要挤压方向为NNE,并形成SE方向的物质流动.帕米尔地区有强烈的构造运动,并存在俯冲带形态的构造.在26.5°N,97°E附近,板块边界的走向发生突变,并形成东倾的缅甸山弧俯冲带,但印度板块挤压造成的主压应力方向为NNE向.在安达曼-尼科巴-苏门答腊-爪哇岛弧,印度板块俯冲于欧亚板块之下,在中国南海一带形成NNW向或近Ns向的主压应力. 相似文献
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本文利用地震资料并结合地质资料,讨论了印度板块与欧亚板块在中国周边的相互作用及其对中国应力场的影响,指出两板块在喜马拉雅山前断裂地区碰撞,碰撞边界向西延续到35°N,74°E附近,其主要挤压方向为NNE,并形成SE方向的物质流动.帕米尔地区有强烈的构造运动,并存在俯冲带形态的构造.在26.5°N,97°E附近,板块边界的走向发生突变,并形成东倾的缅甸山弧俯冲带,但印度板块挤压造成的主压应力方向为NNE向.在安达曼—尼科巴—苏门答腊—爪哇岛弧,印度板块俯冲于欧亚板块之下,在中国南海一带形成NNW向或近Ns向的主压应力. 相似文献
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通过对位于印度板块与欧亚板块碰撞带缅甸弧附近三塔断裂带活动性的野外考察研究，探讨了位于缅甸弧东侧的滇缅泰板缘地区现代构造与地震活动动力来源和空间不均匀性。指出印度板块与欧亚板块沿兴都库什弧的正面碰撞和青藏高原隆起导致的侧向挤出作用对滇缅泰板缘地区现代构造与地震活动的影响可能大于印度板块与欧亚板块沿缅甸弧的碰撞对上述地区的影响。 相似文献
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基于地震参数的缅甸弧俯冲带处板块间几何接触方式的研究 总被引：2，自引：0，他引：2
从全球板块系统来看,中国大陆周边板块活动是其地壳运动的主要外部力源,明确周边板块与中国大陆间较精细的三维几何接触方式对中国大陆动力学研究具有实际意义.本文首先基于研究区域地震活动参数,引用Hayes等在2009和2010年提出的Slab1.0模型,对其进行改造以适用于研究缅甸弧俯冲带处欧亚大陆与印度板块接触的几何产状.其次,沿缅甸弧俯冲边界带截取了166个剖面,依次考察各剖面的震源深度分布情况,对其进行线性平面与非线性曲面拟合,定量地给出了缅甸弧俯冲带东向俯冲的三维几何产状及俯冲范围.最后,针对缅甸弧俯冲带上6个典型剖面的震源深度分布情况,并联合震源机制解和地质构造背景讨论并初步给出了该俯冲带可能的动力作用模式.本文企望为研究中国大陆与周边板块边界几何接触方式提供一个初步方案,并为板块间的动力作用及相关地球动力学研究提供基础研究资料. 相似文献
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利用2993个浅源地震的地震矩张量解、404个Ｐ波初动方向震源机制解和47个深井孔的孔壁崩落资料，编制了东亚地区现今地壳构造应力场主应力方向和应力类型分布图．按200km的等距格点，算出有资料地区各格点半径为200km范围内的平均应力方向，绘制了平均主应力方向分布图，并绘制了东亚地区的震源机制解分布图．主应力方向分布特征表明，东亚地区的现今构造应力场除受印度 欧亚板块碰撞的强烈影响外，俯冲带的弧后扩张亦有重要影响．喜马拉雅山弧处的大陆碰撞和缅甸山弧处的弧后扩张之联合作用可能形成了青藏高原东南部主应力方向的显著转动．菲律宾海板块与欧亚板块在台湾的碰撞与琉球岛弧弧后扩张的联合作用影响了中国东部的应力场．爪哇海沟俯冲带的弧后大片地区现今没有强震活动，这里的弧后扩张可能是造成东南亚地区物质容易向南运动的因素．青藏高原内部大致以昆仑山为界，北部和东北部是大陆内部的宽阔挤压带，南部和西南部地壳上部主要处于正断层型应力状态中． 相似文献
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《中国科学:地球科学》2015,(9)
<正>当地时间2015年4月25日14点11分(UTC2015-04-25 06:11:26),喜马拉雅南侧尼泊尔境内发生了Mw7.9级地震,美国地质调查局提供的震中位置为(28.147°N,84.708°E),震源深度为15.0 km.这次地震以及伴随的次生灾害滑坡、雪崩等对包括首都加德满都在内的尼泊尔以及中国西藏的喜马拉雅北部地区造成严重破坏,带来了重大的人员伤亡和财产损失.这次地震发生在印度板块和欧亚板块碰撞汇聚带之喜马拉雅弧型活动构造区.该地区印度板块以~40 mm/a的速率北向俯冲于欧亚大陆板块之下,喜马拉雅和印度板块汇聚率达~18 mm/a(Bilham等, 相似文献
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西太平洋地壳年龄较老,因而岩石层较冷和比重较大,俯冲带的角度也较大,活动和成熟的弧后盆地则较多;条件与之相反的东太平洋弧后盆地则较少.本文探讨这种相关关系的力学成因,计算了俯冲板块诱生的弧后上涌地幔流动.计算表明,俯冲角度大及存在后撤俯冲时,有利于在弧后地区产生明显的上涌地幔流,这种深部热物质的上涌会导致弧后扩张.反之,年龄较轻的海洋地块较热和较轻,俯冲角度一般也较小,不易诱生上涌地幔物质流动和弧后扩张.大陆地壳密度小于地幔物质,大陆碰撞区就更不具备弧后扩张的条件. 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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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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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 depth to the top of magnetic dykes can be estimated from total field aeromagnetic data using the relation between the depth to magnetic sources and the autocorrelation function of magnetic data. By using synthetic anomalies we show that in the ideal case, depth can be determined to an accuracy of 10% or better, when the anomaly sources are two-dimensional dykes. However, the estimated depths depend on the width of the dykes. The estimated depth is about 0.6 times the actual depth to the top of thin dykes, and around the true depth for thick dykes having width-to-depth ratio around 3. The depth is considerably overestimated for very thick dykes (e.g., contacts, which is a special case of the thick dyke). Thus, the autocorrelation method requires that the width-to-depth ratio of the dyke is estimated independently to correctly estimate the depths. Alternatively, it must be assumed that the width-to-depth ratio for the two-dimensional source body is between 1.5 and 4. 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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On data of bottom sampling, carried out by means of grab, trawl and underwater photography in August–September of 1993 in the area of the Pechora Sea, quantitative regularities of macrobenthos distribution are described for the ecological monitoring purposes. Maps of -biodiversity and biomass indices, bottom communities and trophic zones, singled out by dominant method, are presented. Assessment of structure changes of the investigated area bottom communities during the last 60–70 years is fulfilled. It is shown that the described communities on the whole are of natural undisturbed character and that the revealed changes are within the natural fluctuations in the abundance of benthic populations or may be interpreted in terms of methodical differences in the data analysis and generalization by different authors. 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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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