| 书目名称 | Coronal Expansion and Solar Wind |
| 编辑 | A. J. Hundhausen |
| 视频video | http://file.papertrans.cn/239/238290/238290.mp4 |
| 丛书名称 | Physics and Chemistry in Space |
| 图书封面 |  |
| 描述 | Little more than ten years have passed since spaceprobe-borne instruments con clusively demonstrated the existence of the solar wind. These observations con firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of the interplanetary plasma near the orbit of the earth are now known in great detail. The theory of the coronal ex pansion has also been highly refilled both in the sense of including additional physical processes, and of treating more realistic (time-dependent and non spheri cally-symmetric) coronal boundary conditions. The present volume is an attempt to synthesize the solar wind observations and coronal expansion models from this decade of rapid development. The ultimate goal is, of course, the interpretation of observed solar wind phenomena as the effects of basic physical processes occurring in the coronal and interplanetary plasma and as the natural manifestations of solar properties and structures. This approach implies an emphasis upon the "l |
| 出版日期 | Book 1972 |
| 关键词 | Korona (Astron; ); Orbit; Scale; Sonnenwind; instruments; wind |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-642-65414-5 |
| isbn_softcover | 978-3-642-65416-9 |
| isbn_ebook | 978-3-642-65414-5Series ISSN 0079-1938 |
| issn_series | 0079-1938 |
| copyright | Springer-Verlag Berlin · Heidelberg 1972 |
|Archiver|手机版|小黑屋|
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