[Show/Hide Left Column]
[Show/Hide Right Column]


The Solar Flare Event on 15 June 1991

  • Authors: Rank, G.; Lockwood, J.; McConnell, M.; Ryan, J.; Schonfelder, V.; Bennett, K.; Debrunner, H.; Nieminen, P.; Kocharov, L.; Kovaltsov, G.
  • Publication: American Astronomical Society, 189th AAS Meeting, #18.07; Bulletin of the American Astronomical Society, Vol. 28, p.1298, 1996
  • Solar event of 1991 June 15
  • Case study
  • ADS link
  • Abstract: In June 1991 the Sun produced a series of six X-class flares. For the flare event on 15 June 1991 there exists a rich set of observations, including optical (Hα from Big Bear Observatory and Warsaw Observatory), radio and microwave emission from various stations, soft and hard X-rays (GOES, BATSE/CGRO) and gamma-rays (COMPTEL/CGRO and GAMMA-1). Also particle measurements of neutrons (COMPTEL) and interplanatary protons (neutron monitor network) have been obtained. We review these observations and we are able to obtain a composite photon spectrum spanning the energy range from about 25 keV to 4 GeV. As different features in the gamma-ray spectrum are sensitive to different energies of the accelerated proton spectrum, we can probe this proton spectrum from about 10 MeV to a few hundred MeV, showing that the measurements are consistent with a E^(-3.5) spectrum. Extended emission in gamma-rays can be measured for several hours after the impulsive phase by both COMPTEL (nuclear de-excitation lines and neutron capture line at 2.2 MeV) and GAMMA-1 (>50 MeV gamma-rays from pion decay). Within the statistical uncertainties, both instruments measure the same time behaviour, which can be described by a double exponential decay. This similarity of different energy regimes indicates that continued acceleration of particles dominates over particle trapping during the extended phase.


Created by mevali. Last Modification: Wednesday 23 of May, 2007 09:41:33 UTC by mevali.