Nuclear Deexcitation Gamma-Ray Lines from Accelerated Particle Interactions

Details Nuclear Deexcitation Gamma-Ray Lines from Accelerated Particle Interactions Nuclear Deexcitation Gamma-Ray Lines from Accelerated Particle Interactions

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002apjs..141..523k&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 141, Issue 2, pp. 523-541.

Astronomy and Astrophysics

Astronomy

30

Acceleration Of Particles, Gamma Rays: Theory, Nuclear Reactions, Nucleosynthesis, Abundances, Sun: Abundances, Sun: Flares, Sun: X-Rays, Gamma Rays

Scientific paper

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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