| 书目名称 | Polar and Magnetospheric Substorms | | 编辑 | Syun-Ichi Akasofu | | 视频video | | | 丛书名称 | Astrophysics and Space Science Library | | 图书封面 |  | | 描述 | It has become increasingly clear that the magnetosphere becomes intermittently unstable and explosively releases a large amount of energy into the polar upper atmos phere. This particular magnetospheric phenomenon is called the magnetospheric sub storm. It is manifested as an activity or disturbance ofvarious polar upper atmospheric phenomena, such as intense auroral displays and X-ray bursts. Highly active conditions in the polar upper atmosphere result from a successive occurrence of such an element ary activity, the polar substorm, which lasts typically of order one to three hours. The concept of the magnetospheric substorm and its manifestation in the polar upper atmosphere, the polar substorm, has rapidly crystallized during the last few years. We can find a hint of such a concept in the term ‘polar elementary storm‘ introduced by Kristian Birkeland as early as 1908. However, we are greatly indebted to Sydney Chapman, who established the basic foundation of magnetospheric physics and has led researches in this field during the last half century. Indeed, the terms ‘polar magnetic substorm‘ and ‘auroral substorm‘ were first suggested by Sydney Chapman. The concept of the subs | | 出版日期 | Book 1968 | | 关键词 | Variation; aurora; ionosphere; magnetosphere; solar wind | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-010-3461-6 | | isbn_softcover | 978-94-010-3463-0 | | isbn_ebook | 978-94-010-3461-6Series ISSN 0067-0057 Series E-ISSN 2214-7985 | | issn_series | 0067-0057 | | copyright | D. Reidel Publishing Company, Dordrecht, Holland 1968 |
The information of publication is updating
|
|
发表于 2025-3-21 16:05:01
