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Titlebook: Microphysics of Cosmic Plasmas; André Balogh,Andrei Bykov,John Raymond Book 2014 Springer Science+Business Media New York 2014 Collisionle

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发表于 2025-3-21 20:08:11 | 显示全部楼层 |阅读模式
书目名称Microphysics of Cosmic Plasmas
编辑André Balogh,Andrei Bykov,John Raymond
视频video
概述Presents a comprehensive and up-to-date review of physical processes in space and astrophysical plasmas, from the near-Earth space to the most distant parts of the Universe.Broadly discusses topics in
丛书名称Space Sciences Series of ISSI
图书封面Titlebook: Microphysics of Cosmic Plasmas;  André Balogh,Andrei Bykov,John Raymond Book 2014 Springer Science+Business Media New York 2014 Collisionle
描述Presents a comprehensive review of physical processes in astrophysical plasmas..This title presents a review of the detailed aspects of the physical processes that underlie the observed properties, structures and dynamics of cosmic plasmas. An assessment of the status of understanding of microscale processes in all astrophysical collisionless plasmas is provided. The topics discussed include turbulence in astrophysical and solar system plasmas as a phenomenological description of their dynamic properties on all scales; observational, theoretical and modelling aspects of collisionless magnetic reconnection; the formation and dynamics of shock waves; and a review and assessment of microprocesses, such as the hierarchy of plasma instabilities, non-local and non-diffusive transport processes and ionisation and radiation processes. In addition, some of the lessons that have been learned from the extensive existing knowledge of laboratory plasmas as applied to astrophysical problems are also covered. This volume is aimed at graduate students and researchers active in the areas of cosmic plasmas and space science. Originally published in Space Science Reviews journal, Vol. 278/2-4, 2013.
出版日期Book 2014
关键词Collisionless Magnetic Reconnection; Collisionless Shocks; Hierarchy Plasma Instabilities; Microphysics
版次1
doihttps://doi.org/10.1007/978-1-4899-7413-6
isbn_softcover978-1-4899-7869-1
isbn_ebook978-1-4899-7413-6Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer Science+Business Media New York 2014
The information of publication is updating

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发表于 2025-3-21 22:01:08 | 显示全部楼层
Solar Wind Turbulence and the Role of Ion Instabilities,obability distribution functions of different plasma parameters are not Gaussian, indicating presence of intermittency. At the moment there is no global model taking into account all these observed properties of the inertial range. At ion scales, turbulent spectra have a break, compressibility incre
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Solar Surface and Atmospheric Dynamics,ism inferred from Hanle measurements are converging towards a similar description. They are both described as randomly oriented, largely transverse fields in the several hecto-Gauss range. These similarities are ever making more natural to assume that they are the same. However, and because of the l
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Notes on Magnetohydrodynamics of Magnetic Reconnection in Turbulent Media, the reconnecting system—can make reconnection independent on the microphysical properties of plasmas. We will also show how relaxation theory can be used to calculate the energy dissipated in turbulent reconnecting fields. As well as heating the plasma, the energy dissipated by turbulent reconnecti
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The Dynamic Quasiperpendicular Shock: Cluster Discoveries,lly dependent upon the characteristic spatial scales of the ramp and foot region provided that the shock is stationary. The process of shock formation consists of the steepening of a large amplitude nonlinear wave. At some point in its evolution the steepening is arrested by processes occurring with
发表于 2025-3-23 04:32:05 | 显示全部楼层
Book 2014the extensive existing knowledge of laboratory plasmas as applied to astrophysical problems are also covered. This volume is aimed at graduate students and researchers active in the areas of cosmic plasmas and space science. Originally published in Space Science Reviews journal, Vol. 278/2-4, 2013.
发表于 2025-3-23 09:24:18 | 显示全部楼层
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