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1.
ITRF2000的无整体旋转约束及最新全球板块运动模型NNR-ITRF2000VEL 总被引：11，自引：0，他引：11
由IERS最新公布的ITRF2000地球协议参考架中, 用54个台站维持参考架的定向. 它有两个不足, (ⅰ) 54个台站只分布在全球14个大板块中的9个, 其中有3个板块只有1个台站, 因此这些台站不能很好地维持全球地壳无整体旋转的条件; (ⅱ) 虽然ITRF2000公报中称ITRF2000相对于NNR-NUVEL1A 地质模型为无整体旋转约束, 但计算结果表明ITRF2000不满足地球协议参考架相对于地壳无整体旋转的条件. 结合实测速度场与地质板块模型, 导出产生ITRF地球协议参考架的无整体旋转的条件, 给出选择维持地球协议参考架无整体旋转条件的核心站条件. 同时在建立ITRF地球协议参考架过程中获得新的地球板块运动模型, 可作为ITRF的产品. 相似文献
2.
关于ITRF96参考架整体旋转性的探讨 总被引：11，自引：3，他引：8
利用国际地球自转服务IERS发布的国际地球参考架ITRF96的速度场 ,建立了一个基于现代空间大地测量实测结果的全球板块运动模型ITRF96VEL ,该模型与NNR -NUVEL1A模型有着较好的一致性 .利用该模型 ,本文对ITRF96参考架相对无整体旋转参考架是否存在一个整体旋转的问题进行了初步的探讨 ,结果表明ITRF96参考架相对无整体旋转参考架有一个整体旋转 ,旋转角速度为 0 1 61°/Ma ,旋转极指向南纬 50 5° ,东经 65 5°,这与要求ITRF96无整体旋转的定义不相符 ,这个整体旋转将会对国际地球参考架的高精度应用和长期维持 ,特别是对地球自转参数长期变化的研究产生一定的影响 相似文献
3.
研究全球板块的运动对于地球动力学、地幔流动等具有非常重要的意义.目前常用来推断板块绝对运动模型的方法主要分为基于地质和地球物理的地学方法和空间大地测量方法.地学方法主要包括热点参考系框架,岩石圈无整体旋转、剪切波分裂法、古地磁及古气候资料推断古纬度变化法、海岭海沟法等;空间大地测量方法主要是包括采用VLBI、SLR、GPS以及DORIS等技术手段得到的观测数据进行计算推到全球板块的运动.随着观测技术的不断提高,数据的来源、数量、精度的到了不断的改善和优化,板块的划分也更加精细,不论是反应时间尺度在百万年量级的板块运动地学方法,还是能够反应现今板块运动的空间大地测量方法,给出的模型都随着数据的改善进行了不断的更新,本文综述了迄今为止这些板块绝对运动研究方法的发展历史以及最新进展,分析不同参考基准的特点,认为结合地学方法和空间测量两种方法对全球岩石圈板块的绝对运动研究具有重要意义. 相似文献
4.
利用最新的国际地球自转服务(IERS)发表的国际地球参考框架ITRF2005的速度场,建立了一个完全基于现代空间大地测量实测结果的现今全球板块运动模型ITRF2005VEL,并与地质模型NNR-NUVELlA及以往利用ITRF序列所建立的模型进行了比较.结果表明,从整体上看ITRF2005VEL与NNR-NUVELlA模型有较好的一致性,且较以往的ITRF序列的模型精度更高,但同时也存在着一定的差异性,这与观测台站、板块本身等相关因素都有关.本文还由ITRF2005VEL模型计算了构造板块的总角动量,结果不为零,说明ITRF2005框架有可能不满足无整体旋转的要求. 相似文献
5.
基于ITRF2000的全球板块运动模型和中国的地壳形变 总被引：10，自引：0，他引：10
基于最新的国际地球参考架ITRF2000的速度场构建了一个新的现时板块运动模型ITRF2000VEL,比以往用空间测量技术或地质、地球物理资料建立的板块运动模型,更精确和更全面地反映现时全球板块运动的特点.同时发现了ITRF2000存在整体旋转,旋转角动量矢量为(0.12°/m@a,40.2°S,154.4°E),不符合协议地球参考架的定义.以ITRF2000VEL的欧亚板块运动为背景,计算了近10年来建立的中国地壳运动GPS监测网(全国网和部分区域网)和亚太网的300多个GPS测站在ITRF2000框架内的运动速度.给出和研究了中国大陆及周边地区相对于欧亚板块地壳形变的特点,中国大陆地壳形变具有南强北弱,西强东弱的特点.西部具有一致性的北向运动,而东部具有一致性的南向运动. 相似文献
6.
7.
格尔木—额济纳旗地学断面地球动力学模型初探 总被引：33，自引：9，他引：33
概述格尔木－额济纳旗地学断面研究的地学环境，调查研究内容和初步建立的地球动力学模型，印度板块向北运动为主，西伯利亚板块向南楔入为辅的双向挤压环境是大陆岩石圈最新变形的背景，下地壳的挤压和上地壳的逆冲走滑以及滞后伸展构造组成了岩石圈变形的力学系统。 相似文献
8.
关于全球板块运动模型ITRF2000VEL若干问题探讨 总被引：4，自引：0，他引：4
利用最新的国际地球自转服务（IERS）发布的国际地球参考架ITRF2000速度场，建立了一个独立于任何其它模型、安全基于现代空间大地测量实测结果的现今全球板块运动模型ITRF2000VEL，较百万年平均地质模型NNR－NUVELIA更能真正反映全球板块现今运动特征，相比ITRF96,晚接近于百万年地质模型NNR－NUVELIA，而且ITRF2000参考架在定向、原点和尺度的定义较ITRF96和ITRF97参考架有了改进，但ITRF200VEL模型存在诸多问题：总角动量|L|=0.127，即不为零，与协议参考架（CTRF）不符，存在整体旋转，并建立无旋转NNR－ITRF2000VEL模型，台站不均匀分布全球板块、部分板块界线不明确以及有的板块不满足刚性特征等，这些对ITRF2000的高精度应用和长期维持、地球自转参数的长期变化都将产生一定的影响。 相似文献
9.
板块绝对运动(即岩石圈板块相对于深部地幔的运动)导致软流圈深度存在较强的剪切作用,为软流圈呈现较强的地震波速各向异性提供了一种物理解释.相应地,软流圈地震各向异性的实测数据为反演板块绝对运动提供了一种定量的约束.本文利用前人发表的由474个剪切波分裂数据组成的全球软流圈地震各向异性方向数据集,结合板块相对运动模型MORVEL,通过加权最小二乘法反演板块绝对运动.计算结果表明,由实测数据约束的板块绝对运动模型不能将观测数据拟合到原始数据测量误差要求的统计水平上,反映出以地震各向异性方向指示板块绝对运动方向存在原始数据测量误差之外的系统性误差.该误差或可归因于板块绝对运动控制软流圈地震各向异性的物理机制复杂性以及小尺度地幔流动的区域复杂性.因此,地震各向异性方向只能从统计平均的意义上约束板块绝对运动方向,两者间的差别除了测量误差外还应包含复杂物理成因的模型误差.在原始数据测量误差的基础上增加20°的模型误差并且剔除一个离群数据后,本文得到了最优拟合剪切波分裂数据集的SKS473模型,并与由热点数据反演得到的板块绝对运动模型进行对比.由于约束板块绝对运动的地震各向异性数据和热点数据都存在误差较大、地理分布不均的局限性,结合两类数据的联合反演或可成为未来建立更高精度板块绝对运动模型的有效途径. 相似文献
10.
对我国西南地区思茅地体中部巍山和五印地区白垩纪地层进行了详细的岩石磁学和古地磁研究,获得了两个地区的高温剩磁分量并通过了褶皱检验.巍山剖面特征剩磁方向为Ds=64.3°,Is=48.5°,k=54.6,α95=4.7°;五印剖面特征剩磁方向为Ds=15.4°,Is=44.8°,k=212.0,α95=4.6°.通过思茅地体磁偏角变化与兰坪-思茅褶皱带构造线迹变化的相关性分析,确定思茅地体内部差异性旋转变形受控于思茅地体弧形构造带的形成和演化.通过青藏高原东南缘走滑断裂带活动年代分析,确定兰坪-思茅褶皱带蜂腰构造部位形成于两期构造事件,早期构造变形与东喜马拉雅构造结北北东向挤压缩进有关,后期构造变形与川滇微地块发生顺时针旋转时南向挤出运动有关.以华南板块稳定区白垩纪古地磁极为参考极,计算得出巍山和五印相对于华南板块分别发生了10.5°±6.0°和3.8°±4.9°的南向运移量.通过选取思茅地体内部构造形态较稳定的巍山和普洱地区白垩纪古地磁极为参考极,计算得出五印相对于巍山和普洱分别发生了3.4°±5.0°和3.1°±5.4°的北向纬向运移,表明五印和和巍山之间自印亚碰撞以来经历了较大规模的北向地壳缩短变形作用. 相似文献
11.
本文在最新一代板块相对运动模型(MORVEL模型)的基础上,通过最小二乘反演观测热点方向数据建立板块绝对运动模型.经过对前人用于约束板块绝对运动模型的所有热点数据与MORVEL模型的一致性作系统的统计学检验,发现存在离群数据.相应地,提出两种系统剔除离群数据的新方法:逐一剔除法和全局搜索法.结合对总残差的卡方检验和对残差频率分布的正态检验,逐步筛选最优模型,最终得到一个基于热点参考系的板块绝对运动新模型(T87模型).该模型能够合理拟合全球分布的87个热点方向数据,而模型预测的板块绝对运动速率比观测热点火山的迁移速率系统偏小,最大偏差达到4 cm·a~(-1).这样的偏差可由观测热点速率的系统误差或地幔返回流造成的热点间运动解释.不论是哪种解释成立,本文结果表明热点方向数据能够独立、有效地定义全球热点参考系.这样定义的热点参考系可方便地应用于板块绝对运动、地幔对流及真极移的研究. 相似文献
12.
Fiona Simpson 《Earth and Planetary Science Letters》2002,203(1):535-547
It has been hypothesised that seismic and electrical anisotropy at the base of the lithosphere are caused by strain-induced lattice-preferred orientation (LPO) of olivine [100] axes parallel to present-day plate motion. This would imply that seismic and electrical anisotropy observations can provide geodynamicists with fundamental information for characterising mantle flow. The qualitative agreement between the fast direction of SV-waves and direction of maximum electrical conductance modelled deeper than 150 km below the North Central craton of Australia appear to support a common alignment mechanism, and the observed, anisotropic electrical conductances can be generated by hydrogen diffusivity in a water-poor (<1000 ppm H/Si) olivine mantle. A quantitative test is proposed for the hypothesis that electrical anisotropy is generated by anisotropic hydrogen diffusion rates (D) in olivine. Electrical anisotropy factors are computed using random resistor network models assuming that D[100]≈20×D[010]≈40×D[001]. Electrical and seismic anisotropies calculated from olivine LPO angular distribution functions modelled for a range of shear strains under a simple shear deformation demonstrate that the intensity of olivine [100] alignments (and associated shear strains) that would be required to explain the electrical anisotropy in the mantle below central Australia are significantly greater than predicted by Rayleigh wave anisotropies. The poor agreement between the observed electrical anisotropies and the electrical anisotropies that would be predicted from the Rayleigh wave anisotropies indicates that either (i) electrical anisotropy in the upper mantle below central Australia is not generated by hydrogen diffusivity alone or (ii) the seismic anisotropy is underestimated. The orientation of the olivine [100] axes maxima is inferred to be ∼30° rotated relative to the direction of present-day absolute plate motion (APM) that is determined relative to the hotspot reference frame (HS2-NUVEL1). Both the APM direction that is determined relative to a reference frame defined by requiring no-net rotation of the lithosphere (NNR-NUVEL1) and GPS-derived plate motion vectors fit the geophysical observations of upper mantle anisotropy better. This may support the contention that hotspots are not stationary relative to the deep mantle. 相似文献
13.
Pacific plate equatorial sediment facies provide estimates of the northward motion of the Pacific plate that are independent of paleomagnetic data and hotspot tracks. Analyses of equatorial sediment facies consistently indicate less northward motion than analyses of the dated volcanic edifices of the Hawaiian-Emperor chain. The discrepancy is largest 60–70 Ma B.P.; the 60- to 70-Ma equatorial sediment facies data agree with recent paleomagnetic results from deep-sea drilling on Suiko seamount [1] and from a northern Pacific piston core [2]. Equatorial sediment facies data and paleomagnetic data, combined with K-Ar age dates along the Emperor chain [3], indicate a position of the spin axis at 65 Ma B.P. of 82°N, 205°E in the reference frame in which the Pacific Ocean hotspots are fixed. This pole agrees well with the position of the spin axis in the reference frame in which the Atlantic Ocean hotspots and the Indian Ocean hotspots are fixed [4,5], supporting the joint hypotheses that (1) the Pacific Ocean hotspots are fixed with respect to the hotspots in other oceans, (2) the hotspots have shifted coherently with respect to the spin axis, and (3) the time average of the earth's magnetic field 65 Ma B.P. was an axial geocentric dipole. Global Neogene paleomagnetic data suggest that a shift of the mantle relative to the spin axis has been occurring during the Neogene in the same direction as the shift between 65 Ma B.P. and the present. All data are consistent with a model in which the hotspots (and by inference the mantle) have shifted with respect to the spin axis about a fixed Euler pole at a constant rate of rotation for the last 65 Ma. 相似文献
14.
—We examine the possibility of seismic anisotropy in the asthenosphere due to present plate motion using SKS splitting results. The fast directions of anisotropy correlate weakly with the directions of the absolute plate motion (APM) for all APM models. Weak correlation indicates the possibility of asthenospheric anisotropy as well as frozen anisotropy in the lithosphere. Detection of strain rate dependence of anisotropy is helpful to further conclusion of the problem. The selection of reference frame is important to describe shear deformation in the asthenosphere beneath continent due to plate motion. The behavior of hot spots to the mesosphere, fixed or drifted by mantle return flow, is a key of the selection of the reference frame. For the NNR-NUVEL1 model, APM correlated anisotropy appears only at plate velocity faster than 1.4 cm/yr. It suggests the new possibility of the formation of asthenospheric anisotropy in addition to frozen anisotropy in the lithosphere. A critical plate velocity for the formation of anisotropy can be caused by the dislocation-diffusion transition as a function of strain rate on a deformation mechanism map of the upper mantle olivine. 相似文献
15.
The Comores Islands together with the Tertiary volcanic province of northern Madagascar form a sublinear trend of alkali olivine basalt shield volcanoes across the northern entrance of the Mozambique Channel. Potassium-argon dating of shield-building lavas confirms an eastward increase in age of volcanism along the chain, consistent with a hotspot origin for the lineament. The velocity of the Somali plate over the mantle magma source is 50 mm/yr.
We use the distribution of ages along the Comores-Madagascar chain in conjunction with existing age data for the Reunion-Mascarene Plateau hotspot track to model the absolute motion of the Somali plate for the last 10 m.y. We calculate the relative motion across the East African Rift by subtracting the Somali plate absolute motion from African plate absolute motion during this period. The model predicts 320 km of total separation across the East African Rift during the past 10 m.y. which is greater than has been estimated from surface geological evidence
The geometry of older portions of the Comores and Reunion trends indicates that there was no significant relative motion between the African and Somali plates prior to about 10 m.y. ago. 相似文献
16.
T.H TorsvikAuthor Vitae R Van der VooAuthor VitaeT.F RedfieldAuthor Vitae 《Earth and Planetary Science Letters》2002,202(2):185-200
The fixity of hotspots and mantle plume locations has long been axiomatic. If the assumption of fixed hotspots is granted, ‘absolute’ plate motions and movements of the spin axis with respect to the hotspot framework, defined by some as True Polar Wander (TPW), can be determined. However, this assumption can be tested by paleomagnetic data, and such tests are gradually raising some doubts about the fixity of hotspots. The result is that discrepancies between Cretaceous and Tertiary hotspot and paleomagnetic reference frames are now beginning to be interpreted as the result of plume drift within a convective mantle. In the Indo-Atlantic, hotspots have remained relatively stationary with respect to the spin axis for the last 95 million yr. However, the Pacific hotspots, notably Hawaii, appear to have undergone large-scale southward drift with respect to the spin axis during the Early Tertiary. Global paleomagnetic data do not indicate that any TPW occurred during the Late Cretaceous or Tertiary. Although the Early Cretaceous paleomagnetic and hotspot frames for the Indo-Atlantic realm can be interpreted as slow TPW, direct estimates of paleolatitude and hotspot motion, in particular the Kerguelen hotspot, challenge TPW as a global phenomenon. At present, we consider that the large Early Cretaceous discrepancy between hotspot and paleomagnetic data is best explained by southward drift of the Atlantic hotspots prior to ∼95 Ma. 相似文献
17.
S. Thomas Crough W. Jason Morgan Robert B. Hargraves 《Earth and Planetary Science Letters》1980,50(1):260-274
Available age data support the hypothesis that kimberlite intrusions are formed by mantle hotspots. The hypothesis has been tested by inverting the volcanic traces formed by three hotspots to determine the post-Triassic motions of Africa, South America, and North America relative to these hotspots. Then, using these motions, the kimberlites intruded on these continents within the last 150 m.y. are relocated to their place of origin in the present hotspot reference frame. The result indicates that a majority of the kimberlites formed within 5° of a mantle hotspot. Statistical analysis shows that this kimberlite/hotspot correlation is significant at above the 90% level. 相似文献
18.
The effects of plate rheology (strong plate interiors and weak plate margins) and stiff subducted lithosphere (slabs) on the geoid and plate motions, considered jointly, are examined with three-dimensional spherical models of mantle flow. Buoyancy forces are based on the internal distribution of subducted lithosphere estimated from the last 160 Ma of subduction history. While the ratio of the lower mantle/upper mantle viscosity has a strong effect on the long-wavelength geoid, as has been shown before, we find that plate rheology is also significant and that its inclusion yields a better geoid model while simultaneously reproducing basic features of observed plate motion. Slab viscosity can strongly affect the geoid, depending on whether a slab is coupled to the surface. In particular, deep, high-viscosity slabs beneath the northern Pacific that are disconnected from the surface as a result of subduction history produce significant long-wavelength geoid highs that differ from the observation. This suggests that slabs in the lower mantle may be not as stiff as predicted from a simple thermally activated rheology, if the slab model is accurate. 相似文献