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<正>最近一些大地震如2014年4月1日智利地震之前的地震活动分析结果揭示,一些大地震是有可能被预测的。大地震之前是否有可测量的、明显的前兆异常来警示我们?一直以来,前震被认为是地震预测最有希望的指标。至少一半以上的大地震有前震,但这些前震很难从非前兆地震活动中区分出来。2014年4月1日智利地震及近期其他大地震的前震活动表明,大地震前可能存在可观测的前兆异常。地震相互作用的统计模型表明,当区域 相似文献
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大地震发生后立即在断层带上进行钻探可以帮助我们获取更多的地震信息,尤其是可获得决定断层动态破裂的摩擦水平和强度,观测断层的愈合过程及可能触发余震的应力变化,并可获取控制破裂过程的重要的物理和化学属性。在2008年11月由国际大陆科学钻探项目（ICDP）和南加州地震中心（SCEC）联合在日本东京举办的为期3天的“震后快速钻探：历史、现状与未来”研讨会上, 相似文献
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Yu. A. Brodsky 《地球物理与天体物理流体动力学》2013,107(3-4):223-255
Abstract By using perturbation methods an analytical study has been carried out of large-scale dynamo models, which previously were mainly investigated by numerical methods. 相似文献
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Harold Brodsky 《The Professional geographer》2003,55(2):250-258
A retail dealer was given an exclusive market area in which to sell the product of a manufacturer. Later, this manufacturer assigned part of that exclusive area to another dealer. The first dealer subsequently sued the manufacturer for a breach of contract and damages resulting from the overlap. The attorney for the defense (the manufacturer's attorney) asked me to form an opinion on damages as an expert witness in economic geography. I used two methods: (1) a thought experiment based on a retail gravity model, and (2) an elementary regional shift‐share analysis. This case study in applied geography is presented here in the form of a narrative. 相似文献
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Yu. A. Brodsky 《地球物理与天体物理流体动力学》2013,107(3-4):281-304
Abstract Perturbation theory methods are developed for the kinematic geodynamo equations. The vector Green's function is constructed for the unperturbed equation, which includes the axisymmetric differential rotation. While investigating the perturbation series, we consider a special case in which the decay rates of the axisymmetric toroidal and poloidal dipoles are degenerate. For a number of models within the framework of the theory developed, estimates are given for generation conditions and for observed characteristics of the geomagnetic field. 相似文献
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M. A. Brodsky 《Geophysical Journal International》1981,66(3):727-732
Summary. The inverse gravity potential problem consists in the determination of the form and the density of the body by its exterior gravity potential. We describe two similar classes of bodies for which this problem has a unique constructive solution.
(1) The first class contains the cylindrical bodies with finite length, arbitrary form of section and ρ( R , ø, z) =ρ1 ( z )ρ2 ( R , ø) density distribution, where z is the cylindrical coordinate; R , ø are the polar coordinates in a section plane. This class is important for prospecting geophysics in that it allows us to determine in a unique and constructive way, the function ρ1 ( R , ø), the length, form and orientation of the cylinder if we know the function ρ1 ( z ) and the exterior potential. The classical moment problem of functions is the basis for the solution of this problem.
(2) The analogous problem for the class of the spherical cylinders, or bodies bounded by arbitrary similar sections of two different concentric spheres and the radial lateral surface, appears when bodies of planetary size are studied. (An example of these bodies would be the Moon mascons.) The density distribution of these cylinders is ρ(τ, θ, ø) =ρ1 (τ)ρ2 (θ, ø) where τ, θ, ø are the spherical coordinates. The function ρ1 (θ, ø), length and form of spherical sections can be uniquely determined by exterior potential if we know the function ρ1 (τ). We propose a new constructive method for harmonic continuation of the gravity potential into the region containing the perturbing masses for the solution of the problem. 相似文献
(1) The first class contains the cylindrical bodies with finite length, arbitrary form of section and ρ( R , ø, z) =ρ
(2) The analogous problem for the class of the spherical cylinders, or bodies bounded by arbitrary similar sections of two different concentric spheres and the radial lateral surface, appears when bodies of planetary size are studied. (An example of these bodies would be the Moon mascons.) The density distribution of these cylinders is ρ(τ, θ, ø) =ρ
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