Nuclear Deexcitation Gamma‐Ray Lines from Accelerated Particle Interactions
The Astrophysical Journal Supplement Series2002Vol. 141(2), pp. 523–541
Citations Over TimeTop 10% of 2002 papers
Abstract
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 α 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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