| 書目名稱 | The Near-Saturn Magnetic Field Environment |
| 編輯 | Ali Haidar Sulaiman |
| 視頻video | http://file.papertrans.cn/915/914645/914645.mp4 |
| 概述 | Nominated as an outstanding PhD thesis by Imperial College London, United Kingdom.Offers a concise introduction to collisionless shocks in space plasmas.Demonstrates the use of spacecraft data in stud |
| 叢書名稱 | Springer Theses |
| 圖書封面 |  |
| 描述 | This thesis focuses on the very high Mach number shock wave that is located sunward of Saturn‘s strong magnetic field in the continuous high-speed flow of charged particles from the Sun (the solar wind). The author exploits the fact that the Cassini spacecraft is the only orbiter in a unique parameter regime, far different from the more familiar near-Earth space, to provide in-situ insights into the unreachable exotic regime of supernova remnants. This thesis bridges the gap between shock physics in the Solar System and the physics of ultra-high Mach number shocks around the remnants of supernova explosions, since to date research into the latter has been restricted to theory, remote observations, and simulations. |
| 出版日期 | Book 2017 |
| 關(guān)鍵詞 | Cassini Spacecraft; Collisionless Shock Waves; Saturn Magnetosphere; Alfven Mach Number; Specular Reflec |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-319-49292-6 |
| isbn_softcover | 978-3-319-84124-3 |
| isbn_ebook | 978-3-319-49292-6Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer International Publishing AG 2017 |
|Archiver|手機(jī)版|小黑屋|
派博傳思國(guó)際
( 京公網(wǎng)安備110108008328)
GMT+8, 2026-1-18 22:35
發(fā)表于 2025-3-21 16:25:31
