共查询到20条相似文献,搜索用时 15 毫秒
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A global isostatic gravity model of the Earth 总被引:3,自引:0,他引:3
Mikhail K. Kaban Peter Schwintzer & Sergey A. Tikhotsky 《Geophysical Journal International》1999,136(3):519-536
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The relationship between depth, age and gravity in the oceans 总被引:2,自引:0,他引:2
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Phase change and thermal subsidence of the Williston basin 总被引:1,自引:0,他引:1
Yvette Hamdani Jean-Claude Mareschal Jafar Arkani-Hamed 《Geophysical Journal International》1994,116(3):585-597
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Adrian E. Scheidegger 《Geomorphology》2001,38(3-4)
This note seeks to reconcile the widespread small-scale fractographic observations indicating that surface joints are extension fractures with the frequently observed occurrence of such joints as what appear to be nearly orthogonal conjugate sets, their strikes fitting the shear lines of the neotectonic stress field. It is suggested that the local appearance of joints as extension fractures may have nothing to do with their orientation in the large-scale neotectonic stress field, inasmuch as extrapolations from a local scale to plate-tectonic dimensions are quite speculative. Thus, the local extension-characteristics of the joint surfaces may be acquired at the latest stage of their genesis as a result of the corresponding rock faces becoming exposed, but the geometrically orientational attributes may be conditioned by the shear in the surrounding large-scale neotectonic stress field; a new possible mechanism for reconciling the conflicting local and large-scale observations is suggested. 相似文献
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W. F. Waite L. A. Stern S. H. Kirby W. J. Winters D. H. Mason 《Geophysical Journal International》2007,169(2):767-774
Thermal conductivity, thermal diffusivity and specific heat of sI methane hydrate were measured as functions of temperature and pressure using a needle probe technique. The temperature dependence was measured between −20°C and 17°C at 31.5 MPa. The pressure dependence was measured between 31.5 and 102 MPa at 14.4°C. Only weak temperature and pressure dependencies were observed. Methane hydrate thermal conductivity differs from that of water by less than 10 per cent, too little to provide a sensitive measure of hydrate content in water-saturated systems. Thermal diffusivity of methane hydrate is more than twice that of water, however, and its specific heat is about half that of water. Thus, when drilling into or through hydrate-rich sediment, heat from the borehole can raise the formation temperature more than 20 per cent faster than if the formation's pore space contains only water. Thermal properties of methane hydrate should be considered in safety and economic assessments of hydrate-bearing sediment. 相似文献
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中国互联网发展的区域差异分析 总被引:17,自引:2,他引:17
互联网发展的区域差异及其与区域发展的相互影响研究已成为地理学研究中一个新的问题。从网络普及率、网络信息资源丰度及互联网商业应用三个角度初步探讨了中国互联网发展存在的区域差异,并设计了互联网发展指数(IDI)、从人均的角度反映互联网发展的综合水平。表明:东部地区的发展水平明显高于中部和西部地区,但与传统意义上的经济发展梯度不同的是,西部地区的互联网发展水平稍高于中部地区;中国大陆31个省、直辖市、自治区的互联网发展综合水平的差异同样显著,按照IDI值大小被划分为6个等级。互联网发展区域差异的影响因素是多方面的,应用多元回归分析方法研究发现,区域人口素质水平、区域信息和知识生产能力对我国互联网发展区域差异的解释能力最强,区域对外开放程度和区域城市化水平的影响也较显著。 相似文献
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Summary. A thermal history model for the Earth is described in which the energetically important effects of convection are parameterized through the Nusselt number. The validity of the resulting quasi-steady-state thermal model is shown to depend upon the separation of two time-scales—a dynamic time-scale associated with the overturn time for an assumed mantle-wide convective circulation, and a thermal time-scale associated with the cooling of the planet. Provided the initial thermal state of the Earth was 'hot', the assumption of a time-scale separation can be shown under certain conditions, to be valid throughout the Earth's history. In this connection, the temperature-dependent mantle rheology plays a key role in regulating the thermal history. It is shown that the present-day, gross thermal structure of the Earth can be understood within the context of a quasi-steady-state model which is driven mainly by primordial heat. The notion of whole-mantle convection is shown to be consistent with several additional observational constraints, including the observed mean lithospheric thickness and the mean plate velocities. We briefly consider the extension of the parameterized thermal model to Venus. 相似文献
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Mantle convection with a brittle lithosphere: thoughts on the global tectonic styles of the Earth and Venus 总被引:5,自引:0,他引:5
Plates are an integral part of the convection system in the fluid mantle, but plate boundaries are the product of brittle faulting and plate motions are strongly influenced by the existence of such faults. The conditions for plate tectonics are studied by considering brittle behaviour, using Byerlee's law to limit the maximum stress in the lithosphere, in a mantle convection model with temperature-dependent viscosity.
When the yield stress is high, convection is confined below a thick, stagnant lithosphere. At low yield stress, brittle deformation mobilizes the lithosphere which becomes a part of the overall circulation; surface deformation occurs in localized regions close to upwellings and downwellings in the system. At intermediate levels of the yield stress, there is a cycling between these two states: thick lithosphere episodically mobilizes and collapses into the interior before reforming.
The mobile-lid regime resembles convection of a fluid with temperature-dependent viscosity and the boundary-layer scalings are found to be analogous. This regime has a well defined Nusselt number–Rayleigh number relationship which is in good agreement with scaling theory. The surface velocity is nearly independent of the yield stress, indicating that the 'plate' motion is resisted by viscous stresses in the mantle.
Analysis suggests that mobilization of the Earth's lithosphere can occur if the friction coefficient in the lithosphere is less than 0.03–0.13—lower than laboratory values but consistent with seismic field studies. On Venus, the friction coefficient may be high as a result of the dry conditions, and brittle mobilization of the lithosphere would then be episodic and catastrophic. 相似文献
When the yield stress is high, convection is confined below a thick, stagnant lithosphere. At low yield stress, brittle deformation mobilizes the lithosphere which becomes a part of the overall circulation; surface deformation occurs in localized regions close to upwellings and downwellings in the system. At intermediate levels of the yield stress, there is a cycling between these two states: thick lithosphere episodically mobilizes and collapses into the interior before reforming.
The mobile-lid regime resembles convection of a fluid with temperature-dependent viscosity and the boundary-layer scalings are found to be analogous. This regime has a well defined Nusselt number–Rayleigh number relationship which is in good agreement with scaling theory. The surface velocity is nearly independent of the yield stress, indicating that the 'plate' motion is resisted by viscous stresses in the mantle.
Analysis suggests that mobilization of the Earth's lithosphere can occur if the friction coefficient in the lithosphere is less than 0.03–0.13—lower than laboratory values but consistent with seismic field studies. On Venus, the friction coefficient may be high as a result of the dry conditions, and brittle mobilization of the lithosphere would then be episodic and catastrophic. 相似文献
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以平面区域内偏微分方程定解问题的离散代数方程组为基础,给出了由平面区域内任意分布点上的值求整个区域中值的一种新播值方法──数值微分插值.该方法可直接推广到一维和高维空间的区域中,有较广的应用背景。 相似文献