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964.
J. Rich 《Astroparticle Physics》1996,4(4):387-390
We discuss the information that can be obtained from direct and indirect detection experiments of wimp dark matter. While individual experiments yield little information about wimp cross sections or galactic abundances, we consider the possibility that data from direct and indirect experiments can be combined to give a measurement of the low-energy wimp annihilation cross section. This turns out to be possible if the wimp annihilation rate in the Earth is not balanced by the capture rate. The derived low-energy annihilation cross section can be used to constrain the cosmological density of wimps. 相似文献
965.
We use the fully coupled, three-dimensional, global circulation Jovian Ionospheric Model (JIM) to calculate the coupling between ions in the jovian auroral ovals and the co-existing neutral atmosphere. The model shows that ions subject to drift motion around the auroral oval, as a result of the E×B coupling between a meridional, equatorward electric field and the jovian magnetic field, generate neutral winds in the planetary frame of reference. Unconstrained by the magnetic field, these neutral winds have a greater latitudinal extent than the corresponding ion drifts. Values of the coupling coefficient, k(h), are presented as a function of altitude and cross-auroral electric field strength, for different incoming electron fluxes and energies. The results show that, with ion velocities of several hundred metres per second to over 1 km s−1, k(h) can attain values greater than 0.5 at the ion production peak. This parameter is key to calculating the effective conductivities required to model magnetosphere-ionosphere coupling correctly. The extent to which angular momentum (and therefore energy) is transported vertically in JIM is much more limited than earlier, one-dimensional, studies have predicted. 相似文献
966.
A finite element model is developed for modelling coupled fluid expulsion/deformation behaviour of dewatering sediments subjected to external loadings under isothermal conditions. The non-linear deformation behaviour of the sediment (soil) skeleton is based on the force equilibrium equation in which the constitutive relationship of stress and strain is implemented by the modified Cam-Clay model in soil plasticity. The fluid flow behaviour in the model is described by the generalized porous media flow equation. The model allows temporal and spatial variations of porosity and permeability. The fluid viscosity and density are assumed to be temperature-dependent. The model also allows the development of single and multiple faults, depending upon the material (sediment and fluid) properties, loading and boundary conditions. Procedures are implemented for (1) updating the material properties such as porosity, permeability, fluid density and viscosity and (2) the development of faults which allow the formation of high-permeability conduits for fluid flow. The solution algorithm for displacements of the sediments and the excess pore (fluid) pressure is based on a residual load technique to handle the non-linear (elastic-plastic) deformation behaviour of the sediment skeleton. The model can be applied to one- and two-dimensional problems. Examples of a plane strain saturated sediment layer subjected to stepwise horizontal tractions versus time are given. 相似文献
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The study brings new information concerning a large slope deformation in the northern part of the Silesian Beskydy Mountains
in the territory of the Czech Republic. The studied area is a large-scale transformation of the forefront of a flysch nappe
formed especially by rigid sandstones upon a plastic underlying nappe. As a consequence of the vertical contact of mechanically
different formations and depositing conditions of rocks and tectonics on the nappe forefront, several generations of deep-seated
slope deformations occurred accompanied by shallow landslides in the historic period. Structural measurement and geophysical
sounding proved prevailing lateral spreading in the upper parts of the slopes as well as the occurrence of rotational landslides
whose landslide scarps overlap with the line of overthrust of the Godula Nappe on the Těšín Nappe. Radiocarbon dating determined
the period of the occurrence of rotational landslides as falling into the Subboreal up to Subatlantic. 相似文献
970.
Probabilistic Analysis of Tsunami Hazards* 总被引:2,自引:1,他引:2
Determining the likelihood of a disaster is a key component of any comprehensive hazard assessment. This is particularly true
for tsunamis, even though most tsunami hazard assessments have in the past relied on scenario or deterministic type models.
We discuss probabilistic tsunami hazard analysis (PTHA) from the standpoint of integrating computational methods with empirical
analysis of past tsunami runup. PTHA is derived from probabilistic seismic hazard analysis (PSHA), with the main difference
being that PTHA must account for far-field sources. The computational methods rely on numerical tsunami propagation models
rather than empirical attenuation relationships as in PSHA in determining ground motions. Because a number of source parameters
affect local tsunami runup height, PTHA can become complex and computationally intensive. Empirical analysis can function
in one of two ways, depending on the length and completeness of the tsunami catalog. For site-specific studies where there
is sufficient tsunami runup data available, hazard curves can primarily be derived from empirical analysis, with computational
methods used to highlight deficiencies in the tsunami catalog. For region-wide analyses and sites where there are little to
no tsunami data, a computationally based method such as Monte Carlo simulation is the primary method to establish tsunami
hazards. Two case studies that describe how computational and empirical methods can be integrated are presented for Acapulco,
Mexico (site-specific) and the U.S. Pacific Northwest coastline (region-wide analysis).
* The U.S. Government’s right to retain a non-exclusive, royalty-free license in and to any copyright is acknowledged. 相似文献