Energetic proton spectra in the 11 June 1991 solar flare

Computer Science

Scientific paper

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Gamma-Ray

Scientific paper

We have studied a subset of the 11 June 1991 solar flare γ-ray
data that we believe arise from soft proton or ion spectra. Using data
from the COMPTEL instrument on the Compton Observatory we discuss the
gamma-ray intensities at 2.223 MeV, 4-7 MeV, and 8-30 MeV in terms of
the parent proton spectrum responsible for the emission. .

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