Published August 1985
| Version v1
Report
Observations of solar flare gamma-rays and protons
Creators
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
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19020479
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- EXPERIMENTAL DATA; GAMMA SPECTRA; SOLAR FLARES; SOLAR PROTONS
- Descriptors DEC
- BARYONS; CATIONS; CHARGED PARTICLES; DATA; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; INFORMATION; IONS; NUCLEONS; NUMERICAL DATA; PROTONS; RADIATIONS; SOLAR ACTIVITY; SOLAR PARTICLES; SOLAR RADIATION; SPECTRA; STELLAR ACTIVITY; STELLAR FLARES; STELLAR RADIATION