The Cosmic-Ray Ionization Rate
The Cosmic-Ray Ionization Rate
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DOI：
10.1007/978-94-011-2761-5_116
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发表时间：
1992
期刊：
影响因子：
--
通讯作者：
S. Lepp
中科院分区：
文献类型：
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作者：
S. Lepp
在星际云中观察到了各种各样的分子。它们被认为是由宇宙射线电离开始的反应网络形成的。宇宙射线也是许多天体物理区域的重要加热机制。在这篇文章中，我将回顾用于推断宇宙线电离率的方法和已测量的值。
A wide variety of molecules have been observed in the interstellar clouds. They are believed to be formed by reaction networks which begin with ionization by cosmic-rays. Cosmic-rays are also an important heating mechanism for many astrophysical regions. In this paper I shall review the methods used to infer the cosmic-ray ionization rate and the values which have been measured.