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Titlebook: Cosmic Rays in Magnetospheres of the Earth and other Planets; Lev Dorman Book 2009 Springer Science+Business Media B.V. 2009 Cosmic Rays.E

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書目名稱Cosmic Rays in Magnetospheres of the Earth and other Planets
編輯Lev Dorman
視頻videohttp://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Titlebook: Cosmic Rays in Magnetospheres of the Earth and other Planets;  Lev Dorman Book 2009 Springer Science+Business Media B.V. 2009 Cosmic Rays.E
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
doihttps://doi.org/10.1007/978-1-4020-9239-8
isbn_softcover978-90-481-8096-7
isbn_ebook978-1-4020-9239-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media B.V. 2009
The information of publication is updating

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Main Results of Cosmic Ray Survey to Antarctica on the Ship , in 1996/97,rs, the technique of continuous measurements of the secondary components by groundbased detectors is a unique source of information on the temporal variations of the CR distribution function external to the magnetosphere, as well as the cutoff rigidity planetary distribution. These variations contai
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Magnetospheric Models and their Checking by Cosmic Rays,turbances. The structure of the geomagnetic field and plasma in this region is extremely variable, since it is just here that the boundary between the “spheres of influence” of the earth‘s internal field sources and the magnetotail currents, controlled by the solar wind, is located. Several experime
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Galactic Cosmic Rays in Atmospheres and Magnetospheres of Other Planets,he last 40 years, it is of interest to estimate the expected properties of the CR secondary components, the integral generation multiplicities, the coupling functions, and the meteorological and magnetic effects for the planets and satellites. However, as I mentioned in Preface, to our pity we did n
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0067-0057 heir results measuring cosmic rays on Earth.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
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