Angle distribution and time variation of gamma ray flux from solar and stellar winds, 1. Generation by flare energetic particles

Details Angle distribution and time variation of gamma ray flux from solar and stellar winds, 1. Generation by flare energetic particles Angle distribution and time variation of gamma ray flux from solar and stellar winds, 1. Generation by flare energetic particles

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1178d&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1178-1182 (1997).

Computer Science

Cosmic Rays, Particle Emission, Solar Wind, Mass Loss And Stellar Winds

Scientific paper

On the basis of data on flare energetic particle (FEP) generation and
its propagation in solar (or stellar) wind we calculate the interaction
of these particles with matter and estimate the angle distribution and
time variation of generated gamma ray (GR) fluxes for local and distant
observers.

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