Rp. Enriquez et Li. Miroshnichenko, Frequency distributions of solar gamma ray events related and not related with SPEs in 1980-1995, SOLAR PHYS, 188(1), 1999, pp. 169-185
The advent of new and better instruments in space has resulted in a conside
rable increase in the number of solar gamma-ray events (GRE) detected. In t
his paper, we analyze available SMM/GRS and GRANAT/PHEBUS data on the hard
X-ray and gamma-ray events, and their associations with solar proton events
(SPE) at the Earth's orbit, for the observation period of 1980-1995. About
58% of the GREs under study were found to be SPE-related ones. Size (frequ
ency) distributions have been obtained, for the first time, for the events
with different types of emissions (bremsstrahlung, narrow GR lines, positro
n annihilation line, neutron capture line, SPEs, etc.). We discuss the poss
ible relationships between size distributions implied by the parameter corr
elation. The distribution for GR events turns out to be generally harder th
an that for X-ray bursts. The GREs involving energetic particles in space a
re shown to have a harder frequency distribution in comparison with that fo
r GREs without detectable SPEs. There is also a tendency for the GREs with
highest fluences to be related with SPEs. Finally, no correlation seems to
exist between the GRL fluence and maximum flux of > 10 MeV protons near the
Earth.