Titlebook: Cosmic Electrodynamics; Electrodynamics and Gregory D. Fleishman,Igor N. Toptygin Book 2013 Springer Science+Business Media New York 2013

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书目名称Cosmic Electrodynamics影响因子(影响力)




书目名称Cosmic Electrodynamics影响因子(影响力)学科排名




书目名称Cosmic Electrodynamics网络公开度




书目名称Cosmic Electrodynamics网络公开度学科排名




书目名称Cosmic Electrodynamics被引频次




书目名称Cosmic Electrodynamics被引频次学科排名




书目名称Cosmic Electrodynamics年度引用




书目名称Cosmic Electrodynamics年度引用学科排名




书目名称Cosmic Electrodynamics读者反馈




书目名称Cosmic Electrodynamics读者反馈学科排名

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美色花钱

Nonlinear MHD Waves and Discontinuities,es often rise to large-amplitude perturbations, which cannot be fully accommodated by the linear theory and so require non-linear treatment. In this chapter we consider a number of important examples of the nonlinear waves—simple waves, solitons, and discontinuities—with the use of exact or approxim

Corporeal

地名词典

Particle Transport in Turbulent Cosmic Media, distribution of heavy elements released by supernova explosions, dust particle distribution and evolution, propagation of energetic particles away from their sources, and many more. The particles under study can either be dynamically important for the entire system or play a passive role. In the la

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Emission Processes,ms of computing the Poynting vector flux through a closed infinitely distant surface surrounding the radiation source (Melrose 1980;Rybicki and Lightman 1986; Ginzburg 1987;Nagirner 2007b). In contrast, computing the emission from a plasma, which is an anisotropic, dispersive, and absorbing matter,

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Radiation Transfer,thus, the radiation intensity, spectral distribution, polarization, and directivity can all vary in space and time. The theory of radiation transfer represents a broad field of the physics with numerous astrophysical applications (Chandrasekhar 1961;Mihalas 1978;Dolginov etal.1979;Ginzburg 1987; Nag

六个才偏离

Particle Acceleration in Astrophysical Media,arge Hadron collider (LHC) recently commissioned in Europe. These specially designed accelerating devices are needed because high-energy particles lose their energy very quickly due to interaction with matter and external fields and, thus, become thermally assimilated by the medium.

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