| 書目名稱 | Plasma Astrophysics | | 副標題 | Kinetic Processes in | | 編輯 | Arnold O. Benz | | 視頻video | http://file.papertrans.cn/750/749100/749100.mp4 | | 叢書名稱 | Astrophysics and Space Science Library | | 圖書封面 |  | | 描述 | This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. So- ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena – such as one period of a high-frequency wave – or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses. Study of the Sun is no | | 出版日期 | Book 2002Latest edition | | 關鍵詞 | Corona; MHD; Magnetohydrodynamics; Plasma; Sun; astrophysics; solar | | 版次 | 2 | | doi | https://doi.org/10.1007/0-306-47719-X | | isbn_softcover | 978-94-017-5088-2 | | isbn_ebook | 978-0-306-47719-5Series ISSN 0067-0057 Series E-ISSN 2214-7985 | | issn_series | 0067-0057 | | copyright | Springer Science+Business Media Dordrecht 2002 |
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