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

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書目名稱Cosmic Electrodynamics
副標(biāo)題Electrodynamics and
編輯Gregory D. Fleishman,Igor N. Toptygin
視頻videohttp://file.papertrans.cn/239/238876/238876.mp4
概述Naturally illustrates the fundamental plasma physics laws by applying these to diverse astrophysical applications.Offers more distinct levels of problems and worked out examples than competing textboo
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Cosmic Electrodynamics; Electrodynamics and  Gregory D. Fleishman,Igor N. Toptygin Book 2013 Springer Science+Business Media New York 2013
描述This book presents the fundamental concepts of the theory, illustrated by numerous examples of astrophysical applications. Classical concepts are combined with new developments and the authors demarcate what is well established and what is still under debate. To book illustrates how apparently complicated phenomena can be addressed and understood using well-known physical principles and equations within appropriate approximations and simplifications. For this purpose, a number of astrophysical examples are considered in greater detail than what is normally presented in a regular textbook. In particular, a number of nonlinear self-consistent models are considered, which is motivated by the latest observational data and modern theory.
出版日期Book 2013
關(guān)鍵詞MHD examples; cosmic electrodynamics; galactic superbubble MHD; interstellar winds plasma; nonlinear sel
版次1
doihttps://doi.org/10.1007/978-1-4614-5782-4
isbn_softcover978-1-4939-4193-3
isbn_ebook978-1-4614-5782-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media New York 2013
The information of publication is updating

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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
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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
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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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