Directivity of gamma-rays from flare loops

Details Directivity of gamma-rays from flare loops Directivity of gamma-rays from flare loops

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1822k&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1822-1824. In Russian.

Astronomy and Astrophysics

Astronomy

Coronal Loops, Gamma Ray Astronomy, Particle Acceleration, Solar Flares, Angular Distribution, Equations Of Motion, Radiation Distribution, Solar Electrons

Scientific paper

The angular distribution of gamma-rays generated by accelerated particles moving in loop structures in the solar atmosphere is calculated. The directivity of radiation with an energy exceeding 10 MeV is calculated for specific loop models with an isotropic initial distribution of accelerated electrons. The angular gamma-ray distribution in an intense excited C-12 line at 4.4 MeV is also calculated.

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