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Titlebook: Cosmic Ray Astrophysics; Reinhard Schlickeiser Textbook 2002 Springer-Verlag Berlin Heidelberg 2002 astrophysics.cosmic ray.cosmic rays.el

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發(fā)表于 2025-3-21 20:09:41 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Cosmic Ray Astrophysics
編輯Reinhard Schlickeiser
視頻videohttp://file.papertrans.cn/239/238889/238889.mp4
概述This is the only modern book on the market.All competitive titles date back to 1990 and do not take the latest developments into account.Includes supplementary material:
叢書名稱Astronomy and Astrophysics Library
圖書封面Titlebook: Cosmic Ray Astrophysics;  Reinhard Schlickeiser Textbook 2002 Springer-Verlag Berlin Heidelberg 2002 astrophysics.cosmic ray.cosmic rays.el
描述This book provides an exhaustive account of the origin and dynamics of cosmic rays. Divided into three parts, it first gives an up-to-date summary of the observational data, then -- in the following theory section -- deals with the kinetic description of cosmic ray plasma. The underlying diffusion-convection transport equation, which governs the coupling between cosmic rays and the background plasma, is derived and analyzed in detail. In the third part, several applications of the solutions of the transport equation are presented and how key observations in cosmic ray physics can be accounted for is demonstrated. The applications include cosmic ray modulation, acceleration near shock waves and the galactic propagation of cosmic rays. While the book is primarily of interest to scientists working at the forefront of research, the very careful derivations and explanations make it suitable also as an introduction to the field of cosmic rays for graduate students.
出版日期Textbook 2002
關鍵詞astrophysics; cosmic ray; cosmic rays; electron; particle astrophysics; planet; plasma waves; radiation; uni
版次1
doihttps://doi.org/10.1007/978-3-662-04814-6
isbn_softcover978-3-642-08573-4
isbn_ebook978-3-662-04814-6Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag Berlin Heidelberg 2002
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 21:32:51 | 只看該作者
Water Science and Technology Libraryce observable electromagnetic radiation they continuously lose energy and that should affect their propagation and their original energy spectrum. Second, we want to establish the relation between the observable electromagnetic radiation spectra and properties of the radiating particles. Armed with
板凳
發(fā)表于 2025-3-22 03:01:12 | 只看該作者
The Crex Crex Collective,Bob Jicklinge convective motion of the medium. As a consequence, the electromagnetic fields in the system are severely influenced by the cosmic ray particles, and the description of cosmic ray transport and acceleration is more complex than solving the equation of motion of charged cosmic ray test particles in
地板
發(fā)表于 2025-3-22 07:59:00 | 只看該作者
Interactions of Cosmic Ray Electrons,ce observable electromagnetic radiation they continuously lose energy and that should affect their propagation and their original energy spectrum. Second, we want to establish the relation between the observable electromagnetic radiation spectra and properties of the radiating particles. Armed with
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發(fā)表于 2025-3-22 12:16:18 | 只看該作者
Acceleration and Transport Processes of Cosmic Rays,e convective motion of the medium. As a consequence, the electromagnetic fields in the system are severely influenced by the cosmic ray particles, and the description of cosmic ray transport and acceleration is more complex than solving the equation of motion of charged cosmic ray test particles in
6#
發(fā)表于 2025-3-22 14:43:37 | 只看該作者
Textbook 2002the book is primarily of interest to scientists working at the forefront of research, the very careful derivations and explanations make it suitable also as an introduction to the field of cosmic rays for graduate students.
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發(fā)表于 2025-3-22 18:36:46 | 只看該作者
Introduction,tude above 5 km, and by noon the group was landing at Pieskow, some 50 km from Berlin. During the six hours of flight Hess had carefully recorded the readings of three electroscopes he used to measure the intensity of radiation and had noted a rise in the radiation level as the balloon rose in altitude.
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發(fā)表于 2025-3-22 23:25:38 | 只看該作者
Statistical Mechanics of Charged Particles, neutral (on the average) system of charged and neutral particles interacting with each other and with an external magnetic field. A gas containing so many free charged particles that their collective Lorentz forces influence the properties of the medium considerably is referred to as a ..
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發(fā)表于 2025-3-23 02:59:17 | 只看該作者
Test Wave Approach 1. Waves in Cold Magnetized Plasmas,e next chapter we are ready to investigate the situation characteristics for cosmic rays in space plasmas, where relativistic cosmic rays co-exist with a background interstellar or intergalactic plasma.
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