| 書目名稱 | Cosmic Rays in Magnetospheres of the Earth and other Planets |
| 編輯 | Lev Dorman |
| 視頻video | http://file.papertrans.cn/239/238897/238897.mp4 |
| 概述 | A comprehensive account of the physics describing the interaction of Cosmic Rays with planetary atmospheres, and reference of missions and their results measuring cosmic rays on Earth. |
| 叢書名稱 | Astrophysics and Space Science Library |
| 圖書封面 |  |
| 描述 | The problem of cosmic ray (CR) geomagnetic effects came to the fore at the beg- ning of the 1930s after the famous expeditions by J. Clay onboard ship (Slamat) between the Netherlands and Java using an ionization chamber. Many CR la- tude expeditions were organized by the famous scientists and Nobel Laureates R. Millikan and A. Compton. From the obtained latitude curves it follows that CRs cannot be gamma rays (as many scientists thought at that time), but must be charged particles. From measurements of azimuthally geomagnetic effect at that time it also followed that these charged particles must be mostly positive (see Chapter 1, and for more details on the history of the problem see monographs of Irina Dorman, M1981, M1989). The ?rst explanations of obtained results were based on the simple dipole - proximation of the geomagnetic ?eld and the theory of energetic charged particles moving in dipole magnetic ?elds, developed in 1907 by C. Stormer ¨ to explain the aurora phenomenon. Let us note that it was made about 5 years before V. Hess discovered CRs, and received the Nobel Prize in 1936 together with K. Anderson (for the discovery of CR and positrons in CR). |
| 出版日期 | Book 2009 |
| 關(guān)鍵詞 | Cosmic Rays; Earth; Gamma ray; Magnetospheres; Planet; Planets; atmosphere; solar; spheric |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-1-4020-9239-8 |
| isbn_softcover | 978-90-481-8096-7 |
| isbn_ebook | 978-1-4020-9239-8Series ISSN 0067-0057 Series E-ISSN 2214-7985 |
| issn_series | 0067-0057 |
| copyright | Springer Science+Business Media B.V. 2009 |
|Archiver|手機版|小黑屋|
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