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.
AIP Conference Proceedings
Digital Object Identifier (DOI)
Energetic proton spectra in the 11 June 1991 solar flare Young, C. A. and Arndt, M. B. and Connors, A. and McConnell, M. and Rank, G. and Ryan, J. M. and Suleiman, R. and Schönfelder, V., AIP Conference Proceedings, 510, 564-568 (2000), DOI:http://dx.doi.org/10.1063/1.1303266
© 2000 American Institute of Physics