Generation of γ-rays in solar flares by energetic neutrons and the possibility of determining the model of accelerated particle interaction with the solar atmosphere

Details Generation of γ-rays in solar flares by energetic neutrons and the possibility of determining the model of accelerated particle interaction with the solar atmosphere Generation of γ-rays in solar flares by energetic neutrons and the possibility of determining the model of accelerated particle interaction with the solar atmosphere

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994arep...38..127k&link_type=openurl

Astronomy Reports, Volume 38, Issue 1, January 1994, pp.127-133

Astronomy and Astrophysics

Astronomy

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