On the origin of the pion-decay radiation in the 1982 June 3 solar flare

Details On the origin of the pion-decay radiation in the 1982 June 3 solar flare On the origin of the pion-decay radiation in the 1982 June 3 solar flare

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...316l..41r&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 316, May 1, 1987, p. L41-L44.

Astronomy and Astrophysics

Astrophysics

31

Energetic Particles, Gamma Rays, Neutron Emission, Pions, Radioactive Decay, Solar Flares, Particle Acceleration, Positrons, Time Dependence

Scientific paper

The 1982 June 3 flare produced a wealth of observed gamma-ray, energetic particle, and neutron emissions. The authors show that the predictions of an interaction model developed for the June 3 flare by Murphy, Dermer, and Ramaty in 1987 compare favorably with new data on the time-dependent flux of pion-decay emission from this flare. It is concluded that the particles which produced the bulk of the pions could have the same origin as the particles observed in interplanetary space from the June 3 flare.

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