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Titlebook: Cosmic Plasma Physics; Boris V. Somov Book 2000 Springer Science+Business Media Dordrecht 2000 MHD.Plasma.astronomy.magnetic field.magneto

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樓主
發(fā)表于 2025-3-21 18:50:09 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Cosmic Plasma Physics
編輯Boris V. Somov
視頻videohttp://file.papertrans.cn/239/238886/238886.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Cosmic Plasma Physics;  Boris V. Somov Book 2000 Springer Science+Business Media Dordrecht 2000 MHD.Plasma.astronomy.magnetic field.magneto
描述of the approximation at hand will be outlined from the viewpoint of physics rather than of many possible astronomical applications. After that, as an aid to detailed understanding, please return with pencil and paper to work out the missing steps (if any) in the formal mathematics. On the basis of such an approach the student interested in modern astro- physics, its current practice, will find the answers to two key questions: (1) what approximation is the best one (the simplest but sufficient) for descrip- tion of a phenomenon in cosmic plasma; (2) how tO,build an adequate model for the phenomenon, for example, a solar flare. Practice is really important for understanding the theory of cosmic plasma. Related exercises (problems and answers supplemented to each chapter) to improve skill do not thwart the theory but serve to better understanding of cosmic plasma physics. As for the applications, preference evidently is given to physical processes in the solar plasma. Why? - Much attention to solar plasma physics is con- the possibility of th~ all-round observational test of theoretical ditioned by models. This statement primarily relates to the processes in the solar atmo- sphere. F
出版日期Book 2000
關(guān)鍵詞MHD; Plasma; astronomy; magnetic field; magnetohydrodynamics; plasma physics
版次1
doihttps://doi.org/10.1007/978-94-015-9592-6
isbn_softcover978-90-481-5538-5
isbn_ebook978-94-015-9592-6Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 2000
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 22:16:42 | 只看該作者
0067-0057 ossibility of th~ all-round observational test of theoretical ditioned by models. This statement primarily relates to the processes in the solar atmo- sphere. F978-90-481-5538-5978-94-015-9592-6Series ISSN 0067-0057 Series E-ISSN 2214-7985
板凳
發(fā)表于 2025-3-22 02:11:55 | 只看該作者
Introduction,conductor. By contrast, .. It is precisely the poor knowledge of cosmic phenomena and cosmic plasma properties that explains the retarded development of cosmic electrodynamics. It has been distinguished as an independent branch of physics in the pioneering works of Alfvén (see Alfvén, 1950).
地板
發(fā)表于 2025-3-22 07:23:03 | 只看該作者
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發(fā)表于 2025-3-22 13:51:03 | 只看該作者
0067-0057 at, as an aid to detailed understanding, please return with pencil and paper to work out the missing steps (if any) in the formal mathematics. On the basis of such an approach the student interested in modern astro- physics, its current practice, will find the answers to two key questions: (1) what
7#
發(fā)表于 2025-3-22 17:39:35 | 只看該作者
Introduction, of cosmic matter. Two factors are specific to the latter: its gaseous state and high conductivity. As you know, such a combination is unlikely to be found under natural conditions on earth; the matter is either a non-conducting gas (the case of gas dynamics or hydrodynamics) or a liquid or a solid
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發(fā)表于 2025-3-22 21:17:47 | 只看該作者
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發(fā)表于 2025-3-23 02:56:54 | 只看該作者
Discretization of the Region of InterestIn a system which consists of many interacting particles, the statistical mechanism of ‘mixing’ in phase space works and makes the system’s behaviour . more simple.
10#
發(fā)表于 2025-3-23 08:04:15 | 只看該作者
Mary Kingsley and the Ghosts of West Africa,Among a variety of kinetic phenomena related to fast particles in space, the simplest effect is Coulomb collisions under propagation of the particles in a plasma.
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