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1.
将大陆岩石层视为由幂指数律控制的一薄层,它上伏在粘滞性较低的软流层之上蠕变流动,其运动限制在与东亚大陆构造形态较相似的梯形边界模型框架之中．设印度板块以一恒定的速度向北推进,其被视为青藏高原挤压隆升的主要动力．用数值模拟的方法研究了青藏高原的挤压隆升和中国大陆形变的演化过程．模拟结果表明,计算得到的现代水平形变与现代空间大地测量技术（GPS）观测的水平形变格局较好吻合,说明印度板块与欧亚板块的碰撞、挤压是构成中国大陆内部岩石层水平形变的主要驱动力．模型计算还表明,大陆水平形变受多种因素,如岩石层的力学参数,特别是边界条件的制约． 相似文献
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东亚大陆形变应力场格局演化的数值模拟 总被引：4，自引：0，他引：4
用数值模拟方法研究了印度板和欧亚板块碰撞后４０Ｍａ以来青藏高原的挤压隆升、东亚大陆形变及应力场的演化过程。模型将东亚大陆限定在一梯形边界框架之中,大陆岩石层被视为由幂指数律控制的薄层,它上伏在粘滞性较低的软流层之上蠕变流动。模型设定印度板块以５ｃｍ／ａ的恒定速度向北推进,并视其为青藏高原挤压隆升的主要驱动力,除此可活动边界之外,其余均被设为固定边界,数值模拟结果表明,模型预测的现代水平形变速度和Ｇ 相似文献
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以GPS观测资料和地震学研究成果为约束，针对不同流变参数的中国大陆岩石圈模型，数值模拟了岩石粘度与中国大陆板块边界作用强度的关系，探讨了陆-陆碰撞对中国大陆分层岩石圈运动的驱动机制．给出了陆-陆碰撞驱动力、附加地形与山根浮力及热浮力对中国大陆构造运动的驱动特点．印度板块、太平洋板块和菲律宾板块对中国大陆驱动的边界作用强度之比约是4：1．25：1，所引起的水平主压应力主要集中在坚硬岩石层；而附加地形等垂直方向作用力在水平方向产生的最大主压应力则主要集中在软弱岩石层．这种垂直方向上的作用力在高原南部地区阻碍陆-陆碰撞向北的推挤运动，在高原东北部增加对其它块体的推挤作用。 相似文献
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采用较为符合实际岩石层变形的非线性幂指数本构关系,基于ANSYS有限元平台, 模拟了近20万年来中国大陆地区地表运动及演化过程,探讨了印度板块挤压作用和地幔对流拖曳力各自对于中国大陆地区地表形变运动格局的影响.模拟结果与观测数据的比较表明：在印度板块的挤压和地幔拖曳力联合作用下,中国及东亚大陆岩石层运动形变模式能够和现代GPS观测有较好的吻合; 印度大陆和欧亚大陆的碰撞以及印度大陆的持续向北推进、挤压所产生的应力环境,一直主导了以青藏高原为核心的我国西部地域岩石圈构造、运动和演化,但其影响随着远离青藏高原地区而逐渐变小;地幔对流产生的作用于岩石层底部的拖曳力是中国大陆（特别是远离碰撞带）岩石层运动构造变形的重要驱动力.然而在构造复杂和东部靠近太平洋板块的区域,模型预测结果和GPS观测还存在一定的差距,这说明在未来的中国大陆岩石层变形运动的数值模拟中,应当采用更为复杂的构造模型和驱动力因素. 相似文献
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利用全球重力大地水准面异常、板块绝对运动及全球地震层析成像数据,计算了青藏高原-天山地区岩石层下部地幔大尺度对流格局以及此种尺度对流驱动下岩石层内应力场分布;同时,利用区域均衡重力异常数据反演青藏高原中、北部到天山地区上地幔小尺度对流模型．结果表明,大尺度的地幔物质运移过程可能驱动着中国大陆岩石层整体从西部以南北方向为主的运动转向东部地区以北东和南东方向的运动;而该区域上地幔小尺度上升流动支持了现代青藏高原和天山地区的抬升运动．提出和讨论了青藏高原隆升的“断离隆升-挤压隆升-对流隆升”三阶段模式,并探讨了大陆岩石层构造运动的地幔深部动力学背景． 相似文献
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将大陆岩石层视为由幂指数律控制的一层薄层,它上伏在粘滞性较低的软流层之 上蠕变流动,其运动限制在与东亚大陆构造形态较相似的边界模型的梯形框架之中．设印度 板块以一恒定的速度向北推进,并被视为青藏高原挤压隆升的主要动力．用数值模拟的方法 研究了青藏高原的挤压隆升演化过程,并对数值模拟的隆升过程作了剥蚀修正．结果表明, 由挤压模型所产生的地形和现代青藏高原及其邻区的地形格局比较吻合．同时也表明,挤压 隆升过程受多种因素（如岩石层的力学特性、边界条件以及剥蚀作用）的制约,无论从空间还 是从时间上看,模拟所反映的高原隆升都是不均匀的演化过程． 相似文献
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中国大陆位于欧亚板块的东南部, 受到印度板块、太平洋板块和菲律宾海板块的碰撞挤压与俯冲作用, 其构造应力场形态和动力学机制相当复杂. 本文采用伪三维有限元方法, 以世界应力图2008年版本数据(WSM2008)的应力方向和应力型两类指标作为主要约束, 对中国大陆及邻区的动力驱动机制进行数值模拟, 给出了中国大陆周边地区板块边界力的大小和方向估计. 同时对3个典型情况的数值模型进行了分析. 结果显示, 软流层静压推力对该区域构造应力场影响相对较小, 板块边界力作用则起主导作用; 印度板块在喜马拉雅造山带对欧亚板块的碰撞控制了中国大陆地区应力场的基本形态, 是形成川滇地区走滑型地震为主的重要原因; 琉球海沟——南海海槽俯冲带边界力显示了挤压-张性的分段特性, 贝加尔裂谷表现为拉张作用. 进一步的分析表明, 中国大陆大部分区域内最大水平剪应力分布图像与该地区地震辐射能量密度的分布存在较好的空间正相关性． 相似文献
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采用有限元方法模拟了近20万年来青藏高原岩石圈形变演化过程，探讨了印度-欧亚大陆的碰撞对中国大陆岩石层形变和应力场的影响以及它们与强地震活动性的关系.结合现代GPS、地震和地质学观测的结果，对比分析了中国大陆在百万年、十万年和十年尺度上的形变和构造应力场的基本格局.研究表明：（1）印度-欧亚大陆的碰撞以及印度大陆的持续向北推进、挤压所产生的应力环境，一直主导了以青藏高原为核心的我国西部地域岩石圈构造、运动和演化，但其影响随着远离青藏高原地区而逐渐变小.（2）断层滑移和重力势作用对于青藏高原东西部以及塔里木盆地的影响相当大，它们导致青藏高原岩石层东西向形变速率增大，对青藏高原的中南部地区产生拉张效应，同时导致塔里木盆地出现整体的右旋趋势.（3）青藏高原区域水平方向形变速率和GPS观测结果吻合较好.但在垂直方向上，一些地区计算结果与观测数据相差较大，这说明单纯的挤压作用不是现代青藏高原隆升的惟一机制.现代青藏高原的隆升可能与其他驱动机制，如地幔对流、重力均衡以及剥蚀作用等有关.（4）印度板块的挤压作用基本上决定了中国大陆西部的主压应力场分布.（5）印度板块的碰撞对中国大陆的强地震活动性有重要影响，但华北地区是个例外，该地区的地震活动性很强而印度板块的挤压在该区域产生的影响却很小，说明其他的驱动力在一定程度上活化了华北地块. 相似文献
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综合分析了前人对青藏高原岩石层构造和动力学研究的成果,提出印度板块和欧亚板块会聚、大陆碰撞及大陆形变的基本特征为青藏高原地壳的加厚和地壳缩短,地壳物质的横向流动;青藏高原隆升过程呈现出阶段性、多样性和复杂性;组成青藏高原的各块体可能有不同的主导隆升机制．认识到在板块构造理论所揭示的全球构造格局中,青藏高原不仅仅是印度板块和欧亚板块会聚、碰撞以及大陆形变的结果,它也是青藏高原大陆岩石层和下伏地幔物质运动的相互耦合、相互作用的结果．从地幔动力学的角度出发讨论了青藏高原隆升的断离险升－挤压隆升－对流隆升三阶段模式（ＢＣＣＭ）,结合数值模拟的结果分析了与此模式相对应的该区域岩石层构造、运动的地幔深部物质运移和动力学背景． 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
18.
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