期刊
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
卷 141, 期 2, 页码 523-541出版社
UNIV CHICAGO PRESS
DOI: 10.1086/340545
关键词
acceleration of particles; gamma rays : theory; nuclear reactions, nucleosynthesis, abundances Sun : abundances; Sun : flares; Sun : X-rays, gamma rays
Total cross sections for the production of gamma-ray lines from nuclear deexcitation as a function of the projectile energy are evaluated and presented. Included are proton and reactions with He, C, N, O, Ne, Mg, Al, Si, S, Ca, and Fe. Such functions are essential for interpretation of gamma-ray line observations of astrophysical sites which contain large fluxes of energetic particles such as solar flares, the Earth's atmosphere, planetary atmospheres and surfaces, the interstellar medium, and galactic nebulae.
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