Some evidences of prolonged particle acceleration in the high-energy gamma-ray flare of June 15, 1991

Details Some evidences of prolonged particle acceleration in the high-energy gamma-ray flare of June 15, 1991 Some evidences of prolonged particle acceleration in the high-energy gamma-ray flare of June 15, 1991

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..294..106a&link_type=abstract

High-energy solar phenomena-A new era of spacecraft measurements. AIP Conference Proceedings, Volume 294, pp. 106-111 (1994).

Computer Science

4

Scientific paper

The γ-ray emission extending to energies greater than 1.5 GeV and lasting at least for two hours was observed from the 3B/X12 two-ribbon flare of June 15, 1991 with the telescope GAMMA-1 aboard the GAMMA satellite. A nuclear line emission was also registered in this flare by COMPTEL aboard the CGRO satellite. A comparison of the γ-ray flux time history with that of microwave emission and analysis of the data on solar cosmic ray fluxes provide an evidence of a long-term particle acceleration well after the impulsive phase of the flare. It is suggested that such an acceleration may be associated with a long post-eruptive energy release after a coronal mass ejection (CME).

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