| 書目名稱 | Polar and Magnetospheric Substorms | | 編輯 | Syun-Ichi Akasofu | | 視頻video | http://file.papertrans.cn/750/749744/749744.mp4 | | 叢書名稱 | Astrophysics and Space Science Library | | 圖書封面 |  | | 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 ‘a(chǎn)uroral substorm‘ were first suggested by Sydney Chapman. The concept of the subs | | 出版日期 | Book 1968 | | 關(guān)鍵詞 | 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
|
|
|Archiver|手機(jī)版|小黑屋|
派博傳思國際
( 京公網(wǎng)安備110108008328)
GMT+8, 2026-1-31 07:01
發(fā)表于 2025-3-21 16:05:01
