| 書目名稱 | The Solar Chromosphere and Corona: Quiet Sun |
| 編輯 | R. Grant Athay |
| 視頻video | http://file.papertrans.cn/921/920068/920068.mp4 |
| 叢書名稱 | Astrophysics and Space Science Library |
| 圖書封面 |  |
| 描述 | The widespread tendency in solar physics to divide the solar atmosphere into separate layers and to distinguish phenomena of solar activity from phenomena of the quiet Sun emphasizes the wide ranging diversity of physical conditions and events occurring in the solar atmosphere. This diversity spans the range from a neutral, essentially quiescent atmosphere to a highly ionized, violently convective atmosphere; from a domain in which magnetic field effects are unimportant to a domain in which the magnetic pressure exceeds the gas pressure, and from a domain in which the particle motions are Maxwellian to a domain in which an appreciable fraction of the particles is accelerated to relativistic energies. It is now widely recognized that the chromosphere and corona have a common origin in the mechanical energy flux generated in the hydrogen convection zone lying beneath the photosphere. Furthermore, magnetic field phenomena appear to be as vital to the structure of th~ quiet Sun as to the active Sun. For these reasons it appears desirable to present a unified treatment of the entire solar atmosphere, both active and quiet, in a single volume. On the other hand, such a treatise must be v |
| 出版日期 | Book 1976 |
| 關鍵詞 | chromosphere; solar activity; solar physics; solar wind |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-94-010-1715-2 |
| isbn_softcover | 978-94-010-1717-6 |
| isbn_ebook | 978-94-010-1715-2Series ISSN 0067-0057 Series E-ISSN 2214-7985 |
| issn_series | 0067-0057 |
| copyright | D. Reidel Publishing Company, Dordrecht, Holland 1976 |
|Archiver|手機版|小黑屋|
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