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821.
美国哈佛大学1977——2004年的矩心矩张量结果显示, 我国川西北次级地块、 滇中次级地块的西部及滇中次级地块的东部的应力场特征有明显的差别. 应用滑动矢量拟合法, 反演了这三个区域的应力场特征: 川西北次级地块以近南北向的水平主张应力轴和西倾的主压应力轴为特征; 滇中次级地块的西部以倾向北东东的主张应力轴以及近南北的水平中等主应力轴为特征; 滇中次级地块的东部以南西西——北东东向的水平主张应力轴以及北北西——南南东向的水平主压应力轴为特征. 有限元模拟结果清楚地显示出, 川滇地块在阿萨姆楔附近受到来自印度板块的强烈挤压, 随着远离阿萨姆楔, 这种挤压应力逐渐衰减; 同时, 该地区的主张应力方向明显地形成了围绕阿萨姆楔的环线. 其中, 内部物质性质均匀、 地表和底部边界自由、 侧部边界采用GPS观测约束的弹性有限元模拟显示, 在川西北次级地块, 模拟结果与震源机制解结果相一致; 在滇中次级地块, 模拟结果所显示的图象与震源机制解观测结果有差别, 不仅没有显示出与大面积的东部地区的震源机制解相一致的特征, 反而显示出与该地区西部震源机制解相一致的特征. 通过调节地块内部物质的弹性常数, 可以实现在滇中次级地块东部部分地区出现与震源机制 相似文献
822.
823.
824.
825.
The vertical stability character of the families of short and long period solutions around the triangular equilibrium points
of the restricted three-body problem is examined. For three values of the mass parameter less than equal to the critical value
of Routh (μ
R
) i.e. for μ = 0.000953875 (Sun-Jupiter), μ = 0.01215 (Earth-Moon) and μ = μ
R
= 0.038521, it is found that all such solutions are vertically stable. For μ > (μ
R
) vertical stability is studied for a number of ‘limiting’ orbits extended to μ = 0.45. The last limiting orbit computed by
Deprit for μ = 0.044 is continued to a family of periodic orbits into which the well known families of long and short period
solutions merge. The stability characteristics of this family are also studied. 相似文献
826.
S. Ichtiaroglou K. Katopodis Michalodimitrakis 《Journal of Astrophysics and Astronomy》1989,10(4):367-380
Three-dimensional planetary systems are studied, using the model of the restricted three-body problem for Μ =.001. Families
of three-dimensional periodic orbits of relatively low multiplicity are numerically computed at the resonances 3/1, 5/3, 3/5
and 1/3 and their stability is determined. The three-dimensional orbits are found by continuation to the third dimension of
the vertical critical orbits of the corresponding planar problem 相似文献
827.
Alessandro Morbidelli Antonio Giorgilli 《Celestial Mechanics and Dynamical Astronomy》1989,47(2):173-204
The general theory exposed in the first part of this paper is applied to the following resonances with Jupiter's motion : 3/2, 2/1, 5/2, 3/1, 7/2, 4/1; these are the most relevant resonances for the asteroids. The whole analysis is performed in the framework of the spatial problem of three bodies, both in the circular and in the elliptic case. The results are also compared with the observed distribution of the asteroids. 相似文献
828.
J. A. DE ROO 《Journal of Metamorphic Geology》1989,7(3):311-322
Microstructures in slate belt rocks at the Elura Mine, near Cobar, south-eastern Australia, indicate that volume loss by syntectonic dissolution is coupled with mass accretion by reprecipitation of the dissolved material in dilational sites. The mass accretion is sustained primarily by repetitive tensile microfracturing at high pore-fluid pressures. Oriented growth in the inter- and intragranular microcracks is locally host-controlled, creating lattice- and shape-preferred orientations. The grain-scale crack-seal features throughout the rock reflect rhythmic fluid pressure fluctuations; a balance is achieved between the fracture-induced permeability (and consequent flushing rates), and the rate of fluid build-up in a relatively sealed environment.
Instability in the balancing factors can lead to localization and intensification of tensile failure (and hence, tension vein formation) in the grain aggregate. Growth of veins by crack-seal also reflects a steady state, but with more localized fluctuations of fluid flow on the aggregate scale. Still larger imbalances between flushing and fluid accumulation (i.e. pressure variations) induce breccia veining. The larger pressure gradients over greater distances, associated with dilation localization (from pervasive microfracturing to spaced breccia domains), allow fluid channelling with an increased potential for chemical fluid/rock disequilibrium. Therefore, large breccia vein systems tend to be sites of extensive fluid/rock interaction and replacement, as spectacularly illustrated by the syntectonic sulphide orebodies at Elura. The huge amounts of silicate, carbonate and sulphide accumulated during folding at Elura illustrate the large scale of source and sink couples possible in solute mass transfer. 相似文献
Instability in the balancing factors can lead to localization and intensification of tensile failure (and hence, tension vein formation) in the grain aggregate. Growth of veins by crack-seal also reflects a steady state, but with more localized fluctuations of fluid flow on the aggregate scale. Still larger imbalances between flushing and fluid accumulation (i.e. pressure variations) induce breccia veining. The larger pressure gradients over greater distances, associated with dilation localization (from pervasive microfracturing to spaced breccia domains), allow fluid channelling with an increased potential for chemical fluid/rock disequilibrium. Therefore, large breccia vein systems tend to be sites of extensive fluid/rock interaction and replacement, as spectacularly illustrated by the syntectonic sulphide orebodies at Elura. The huge amounts of silicate, carbonate and sulphide accumulated during folding at Elura illustrate the large scale of source and sink couples possible in solute mass transfer. 相似文献
829.
重力仪的周期误差是精密重力测量的一个误差源。本文阐述由于齿轮组合所产生的周期误差,给出全部可能存在的周期数。以G584仪器为例,发现除已被普遍采用的1、7.33、73.33、220周期数外,尚存在22周期数。用大量程静电反馈装置进行测量,验证22周期数的周期误差幅值为4.33×10~(-6)m/S~2。同时讨论了为标定该项误差增强现有基线的必要性。 相似文献
830.
在应变分析基础上,用本文提出的方法估算了岩石体耗,初步探讨了应变、体耗与矿脉的成因联系。认为矿脉主要是矿源层岩石在变形过程中,由压溶、压实作用产生体耗而排出的热液所形成的。 相似文献