共查询到18条相似文献，搜索用时 187 毫秒
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在小尺度地幔对流模型的基础上,建立了顾及岩石层与地幔耦合的地幔对流模型,考虑到岩石层对上地幔小尺度对流的弹性响应,将上地幔视为一均匀的等粘滞系数的牛顿粘滞流体,其对注能量来源于下地幔,用热流体动力学基本方程得到地上地幔对流在壳幔边界处的垂向应力作为弹性板弯曲方程的垂直加载,来耦合弹性岩石层和可流动地幔,推导了两者耦合下区域重力异常和上地幔小尺度对流的相关方程,用以反演上地幔小尺度对流场模式和岩石层底部拖力场格局,对比了有,无弹性岩石层影响的模型之间的差异,并对模型应用范围,特别要板块边界水平均造力可能产生的影响,作了进一步探讨。 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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利用最新的地球重力场模型,计算了新疆及邻近地区的自由空气重力异常、大地水准面扰动异常、地壳和上地幔平均密度异常以及地幔对流引起的岩石层底界面粘滞应力场分布．根据计算结果,对新疆天山地区的构造动力学特征进行了分析和推断,认为天山处于地幔对流形成的挤压沉降环境中,在南北不对称的挤压应力作用下快速隆升,挤压应力场中心在天山以南．这种应力场特征有利于塔里木板块向天山之下俯冲的观点．天山南北两侧的准噶尔盆地南缘和塔里木盆地北缘,是地壳内质量缺失区,是由于南北两侧地壳向天山下挤压而弯曲造成的．中国天山东段的深部密度分布特征与中段和西段的不同,可能是地幔对流分布的东西向差异造成的． 相似文献
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上地幔小尺度对流是控制区域地球动力学过程的主要机制之一,蒙古-贝加尔地区的一些区域动力学过程被认为与上地幔小尺度对流相关.本文目的在于利用重力资料研究蒙古-贝加尔地区的上地幔小尺度对流,并探讨其与构造动力学的关系.基于区域均衡重力异常与上地幔小尺度对流的相关方程,本文利用区域均衡重力异常资料反演了蒙古-贝加尔地区上地幔小尺度对流流场及作用于岩石层底部的应力场.结果显示,蒙古-贝加尔地区地幔流场及对流应力场呈现非常复杂的图像,流场及应力场分布与地表构造具有很好的相关性.西伯利亚地台和蒙古褶皱带下地幔流场和对流应力场均较弱,这与这些地区现今较弱的构造活动性是一致的.贝加尔裂谷区下存在地幔上升流,对流应力场呈拉张状态,但应力场的幅值较小(约8 MPa),表明地幔对流不是贝加尔裂谷开裂的主要控制因素.Hangay高原、阿尔泰和戈壁-阿尔泰下存在地幔上升流,对流应力场为拉张状态,这一方面可能构成Hangay高原隆升的深部动力机制,另一方面,也为Amurian板块西边界划分提供了动力背景. 相似文献
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详细讨论了我国西北区域(80～95E，35～45N)均衡重力异常以及与之相应的地幔动力学问题．假定其区域均衡重力异常主要源于该区域岩石层变形和上地幔之中物质流动的结果．利用傅容珊等(1994 a，b)用区域均衡重力异常反演上地幔小尺度热对流的模型，计算了西北地区上地幔对流格局．结果表明，天山和昆仑山——阿尔金山系强烈地上升，与之相应地幔中的上升流动以及塔里木盆地下部地幔物质的汇聚流动，控制了这一区域岩石层动力学的主要格局．西北地区的几个大型盆地，如塔里木盆地、准葛尔盆地和吐鲁番盆地等对应了均衡重力异常的负异常中心，同时也对应于地幔中物质流动的汇聚中心，物质流动结果加上其上部岩石层横向挤压向下凹陷而形成压性盆地．天山、昆仑山及阿尔金山等新构造运动活跃的山区对应了地幔中物质上升及发散流动，这一作用使得这些地区的岩石层向上隆起维持其山系不断抬升．以此为基础，本文构成了该区域岩石层动力学的基本框架模型，并对这一框架以及影响这一力学框架构成的其它动力学因素，诸如印度板块向北俯冲、挤压运动、全地幔范围内物质流动以及均衡力等问题作了初步探讨． 相似文献
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利用中国地震台网和ISC台站1980～2004年的地震数据，反演了南海东北部及其邻近地区的Pn波速度结构和各向异性.上地幔顶部的速度变化揭示出区域地质构造的深部特征：华南地区速度较高并且变化平缓，具有构造稳定地区的岩石层地幔特征；华南沿海尤其是滨海断裂带附近出现低速异常，表明该断裂可能穿过壳幔边界深达上地幔顶部.南海北部至台湾海峡较高的速度与华南地区类似，反映出大陆边缘和陆架地区的岩石层地幔性质；西沙海槽附近较高的速度不仅反映了华南大陆向南的延伸，而且与海槽裂谷拉张引起的地幔上拱有关，整个南海北部没有发现大规模地幔热流的活动痕迹.相比之下，南海东部次海盆的上地幔顶部存在明显的低速异常，对应于海底扩张中心的地幔上涌区，表明岩石层地幔强烈减薄甚至缺失；台湾东部－吕宋－菲律宾北部的低速异常与地震、火山活动以及岩浆作用紧密相关，揭示了西太平洋岛弧俯冲带的活动特征；南海东北部的洋－陆边界清晰，南海东部和菲律宾海西部较高的速度代表了海洋岩石层地幔的性质.Pn波各向异性反映出区域性构造应力状态及岩石层地幔的变形痕迹：华南地区的各向异性较小，说明这一构造稳定地区的岩石层地幔变形程度较弱；南海北部的快波方向与地壳浅表层构造的伸展方向一致，主要反映了中、新生代以来的大陆边缘张裂和剪切作用对岩石层地幔结构的影响；琉球－台湾－吕宋岛弧两侧各向异性十分强烈，平行于海沟的快波方向表明菲律宾海板块和欧亚大陆的相互作用导致俯冲板块前缘的岩石层地幔强烈变形；台湾东南海域快波方向的变化可能与欧亚大陆和菲律宾海板块俯冲机制的转换以及岩石层被撕裂有关. 相似文献
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利用中国及邻区地形、地震层析成像、沉积层底面、Moho面及岩石层底面资料,正演计算出中国及邻区岩石圈大地水准面异常;再从全阶大地水准面异常中扣除正演模拟得到的岩石圈大地水准面异常与不同阶次波段的大地水准面进行比较,寻求表示中国及邻区地幔物质不均匀的大地水准面异常的最佳阶次为2-60阶. 结果表明,对应于岩石圈的大地水准面异常的重力位球谐函数阶数为61-20阶;下地幔重力位球谐函数阶数为2-6阶;而-60阶重力位球谐函数则表示中国及邻近区域上地幔大地水准面异常. 相似文献
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本文利用数值法求解瞬时地幔对流问题以模拟大地水准面异常.利用两个较新的S波速度异常层析模型SEMUCB_WM1和TX2019slab,将其转换为密度异常作为控制方程的浮力驱动项;采取的黏度结构模型中,上下地幔的黏度比为1∶50.为了研究地幔不同结构对罗斯海海域大地水准面异常的影响,分别提取上、下地幔的密度异常正/负值,作为对流控制方程的输入项,计算相应的模拟大地水准面异常.将模拟大地水准面异常与观测值进行对比,发现罗斯海海域的大地水准面异常主要来自下地幔及上地幔的负密度(波速)异常,下地幔正密度异常对该区域大地水准面负异常也有一定的贡献.本文认为,地幔密度负异常在罗斯海海域大地水准面异常的形成中占据主导作用,地幔对流的动力学效应对该区域大地水准面异常的形成影响较弱. 相似文献
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以湖南地区为例,利用超高阶地球重力位模型EGM2008计算了研究区的重力大地水准面,并采用棱柱体公式和球体公式相结合的方法分别进行了完全地形改正和Airy-Heiskanen局部均衡改正,得到布格大地水准面和均衡大地水准面.对三种大地水准面进行不同波长分量的分离处理,得到包含不同深度异常信息的剩余大地水准面,并结合其他地球物理资料对研究区进行了详细的地球物理解释.结果表明,剩余重力大地水准面可以有效地反映出研究区内的深部构造特征,如深大断裂带分布、构造块体位置、上地幔密度横向分布等,但对地壳内异常结构反映不明显;研究区岩石圈密度变化相对平缓,厚度由东向西增加;根据剩余均衡大地水准面及研究区Airy局部均衡莫霍面,可以大致推测出研究区的莫霍面起伏形态以及均衡状态,可作为一种有用的参考信息. 相似文献
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由于卫星观测技术的发展，现在已能利用测高大地水准面简捷可靠地研究海底构造与动力问题. 根据Geosat T2/ERM、Topex/Poseidon 和ERS 1/2测高数据给定的0°N ～45°N、100°E～150°E范围内4′×4′大地水准面，采用全球地形/均衡的重力位效应改正，计算布格、格莱尼和均衡大地水准面. 由格莱尼大地水准面反演Moho面埋深，再从均衡大地水准面起伏推算小尺度地幔流应力场. 结果表明，菲律宾海和南海显示了与磁条带、扩张脊对应或斜交的高频成分大地水准面起伏条带. 各边缘海盆的Moho面埋深有往南变浅的趋势，与菲律宾海各海盆的Moho面埋深大致相当，说明琉球—台湾—菲律宾岛弧两侧的构造动力强度基本相近. 从各种构造特征和大、中、小尺度的地幔流应力场的驱动机制，可以证明岛弧内侧的边缘海具有不同于大洋、大陆的独特构造动力格局和特征. 相似文献
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New satellite technology to measure changes in the Earth’s gravity field gives new possibilities to detect layers of low viscosity inside the Earth. We used density models for the Earth mantle based on slab history as well as on tomography and fitted the viscosity by comparison of predicted gravity to the new CHAMP gravity model. We first confirm that the fit to the observed geoid is insensitive to the presence of a low viscosity anomaly in the upper mantle as long as the layer is thin ( 200 km) and the viscosity reduction is less than two orders of magnitude. Then we investigated the temporal change in geoid by comparing two stages of slablet sinking based on subduction history or by advection of tomography derived densities and compared the spectra of the geoid change for cases with and without a low viscosity layer, but about equal fit to the observed geoid. The presence of a low viscosity layer causes relaxation at smaller wavelength and thus leads to a spectrum with relatively stronger power in higher modes and a peak around degrees 5 and 6. Comparing the spectra to the expected degree resolution for GRACE data for a 5 years mission duration shows a weak possibility to detect changes in the Earth’s gravity field due to large scale mantle circulation, provided that other causes of geoid changes can be taken into account with sufficient accuracy. A discrimination between the two viscosity cases, however, demands a new generation of gravity field observing satellites. 相似文献
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The origin of the high topography of the Norwegian Mountains is currently much debated. Several geophysical studies show that the uppermost mantle below southern Norway has anomalously low velocities as compared to other parts of the Baltic Shield. This study aims to shed lights on the structure of the lithospheric mantle below southern Norway by adapting and further refining a method based on isostatic and thermal equilibrium to compute temperature, temperature-related density and synthetic S-wave velocity in stable continental domains. The one-dimensional steady-state heat equation is used with topographic, Moho depth, crustal density and surface heat flow data. A condition of local isostasy is assumed and geoid undulations are used to constrain the range of possible lithosphere models.Results derived from this method suggest a thickening of the thermal lithosphere below southern Norway from west to east. The western part is found to have higher temperatures, lower densities and lower synthetic S-wave velocities than the eastern part, compatible with results from a recent P-wave travel time residual study. Comparison of the synthetic shear-velocity profiles beneath southwestern Norway with velocity profiles inverted from Rayleigh wave dispersion data suggests that the higher temperatures associated with a thinner lithosphere can explain parts of the seismic low-velocity anomaly.The inferred lithospheric structure is sensitive to uncertainties in the crustal input model, but the main features remain undisturbed by changes in the input data. The results show that the lithosphere of southwestern Norway can be in local isostatic equilibrium, if it is thinner and warmer than the lithosphere of eastern Norway. The present-day high topography may therefore be partially sustained by lower densities in the mantle lithosphere. 相似文献
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Choon-Ki Lee Shin-Chan Han Bernhard Steinberger 《Physics of the Earth and Planetary Interiors》2011,184(1-2):51-62
The radial viscosity structure of the Earth is explored on the basis of the geoid observations. The variations of uncertainty in seismic tomography models are accounted for when finding the radial viscosity structure. The new methodology we propose attempts to fit more closely those features of the geoid that are better constrained by tomography models and avoids to fit those features that are poorly constrained. This approach is particularly important because the error of geoid predictions caused by uncertainties in seismic tomography models is overwhelmingly larger than the noise in the geoid measurements. The synthetic tests indicate that the viscosity structures obtained by disregarding the uncertainty variations in seismic tomography models can be biased depending on the geoid spectral band and on the ‘input’ seismic tomography model. When the uncertainty variations in seismic models are considered in the inversion process, results do not indicate a viscosity in the transition zone lower than in the upper mantle. A robust feature found with the new method is a viscosity in the upper mantle two orders of magnitude smaller than in the lower mantle. The error covariance of seismic tomography models is critical for the method we suggest. A covariance matrix rigorously derived by seismologists should help to even more reliably infer the viscosity structure and relation between anomalies in density and seismic velocities from surface observations such as the geoid, and thus lead to a better knowledge of the Earth interior. 相似文献
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将地形高、地球内部质量异常以及重力、大地水准面展开成球谐级数，依据岩石圈弹性挠曲均衡补偿理论建立地形—均衡补偿重力、大地水准面异常的球谐级数表达式.由此我们可以研究地形—均衡补偿重力、大地水准面异常与球谐级数阶次的关系，以及不同波长地形荷载与岩石圈挠曲补偿的关系，探讨地形—均衡补偿重力、大地水准面的频谱特性.从观测大地水准面异常和自由空气重力异常扣除地形—均衡补偿大地水准面、重力异常，可以得到均衡大地水准面异常和均衡重力异常.均衡大地水准面异常已经消除了浅层物质不均匀的影响，反映的是地球深部物质密度不均匀分布.均衡重力异常显示出中短波长特性，反映的是地壳上地幔物质分布的失衡和物质调整的动力学特征. 相似文献
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Important though indirect information about the internal structure of Venus is provided by its topography and geoid. In the last decades this information has been used to constrain the Venus mantle viscosity structure and its dynamic regime. Recently, the geodynamic inversion of the Venus?? geoid and topography resulted in a group of best fitting viscosity profiles. We use these viscosity models here as an input to our mantle convection code. We carry out simulations of the Venus?? mantle evolution in a 3D spherical shell with depth dependent viscosity and check whether the character of the dynamic topography and the geoid represented by their power spectra fits the observed quantities. We compare the results with several other models obtained for different viscosity stratifications (constant, constant with highly viscous lithosphere, linear increase of viscosity). Further, we estimate the effect of other factors such as internal heating and varying Rayleigh number. We use a 2D spherical axisymmetric convection code to study the effect of lateral viscosity variations. In these 2D models we monitor the topography and the geoid developing above the axisymmetric plume and compare them with the observed elevations of Venus?? geoid and topography in several Regia. Though none of the models fits observed data perfectly, we can generally conclude, that the best fit between the observed and predicted quantities is reached for viscosity profiles with 200 km thick lithosphere followed by a gradual increase of viscosity with depth and with the upper mantle viscosity of 2 × 10 21 Pa s. For all viscosity profiles the predicted geoid and topography spectra match the observed ones only up to the degree 40, thus indicating other than dynamic origin of these quantities for higher degrees. 相似文献
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Tide gauge recordings of the secular variation of relative sea level are known to be strongly influenced by the ongoing global process of glacial isostatic adjustment. The east coast of the North American continent is heavily instrumented with tide gauge installations, many of which have been carefully maintained for over 50 years. Since this region traverses the collapsing forebulge of the Laurentide ice sheet and since the process of collapse is extremely well constrained on the basis of radio-carbon dated relative sea level histories from a dense set of locations, the region is globally unique in enabling an accurate decontamination of the tide gauge data using the 14C records themselves. It is shown herein that the decontaminated data define a residual signal which varies only slightly along the coast and which consists of an average rate of sea level rise near 2 mm yr-1.The relative sea level histories from sites along this coast also provide an excellent basis for testing theoretical models of the global glacial isostatic adjustment process that must be employed to decontaminate the tide gauge records at sites for which 14C records are unavailable. It is demonstrated that a mantle viscosity profile determined by the formal inversion of 14C controlled relative sea level histories from sites within the margins of the northern hemisphere ice sheets that existed at last glacial maximum enables a gravitationally and topographically self-consistent global model of glacial isostatic adjustment to accurately reconcile east coast rsl data. No viscosity structure has previously been derived that was successful in this regard. The global model based on this structure is therefore expected to provide an excellent basis for the removal of glacial isostatic adjustment effects from tide gauge recordings. The viscosity structure itself is also extremely close to models of the radial variation that have previously been shown to fit the requirements of non-hydrostatic geoid anomalies. This has important geodynamic implications concerning mantle rheology as it would appear to establish that transient and therefore non-linear creep mechanisms are not involved, since short timescale and long timescale viscosities are the same. 相似文献