Published August 1985 | Version v1
Report

Observations of solar flare gamma-rays and protons

Description

Solar flare gamma-rays (4 to 7 MeV) and protons (8 to 500 MeV) were simultaneously observed from six flares on 1 Apr., 4 Apr., 27, Apr. 13, May 1981, 1 Feb. and 6 June 1982 by the Hinotori and GMS satellites. The relationship between 4 to 7 MeV gamma-ray fluences and peak 16 to 34 MeV proton fluxes for these flares are analyzed. It does not reveal an apparent correlation between these two parameters. The present result implies that the protons producing gamma-rays and the protons observed near the Earth do not always belong to the same population

Additional details

Publishing Information

Imprint Title
Ninteenth International Cosmic Ray Conference. SH sessions, volume 4
Journal Page Range
vp.
Report number
N--85-34729