The GAMMA-1 data on the March 26, 1991 solar flare

Details The GAMMA-1 data on the March 26, 1991 solar flare The GAMMA-1 data on the March 26, 1991 solar flare

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..294..130a&link_type=abstract

High-energy solar phenomena-A new era of spacecraft measurements. AIP Conference Proceedings, Volume 294, pp. 130-133 (1994).

Computer Science

10

Scientific paper

Two different components of γ-emission with energies from 30 MeV to several hundred MeV were observed in the solar flare with total duration of 10 minutes. The first, impulsive one, originates as a bremsstrahlung of electrons accelerated at high plasma density (n>~1014 cm-3). The second, delayed component, is associated with a pion production of high energy ions accelerated at low densities in the corona during the stage of magnetic field restoration.

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