Published August 1985
| Version v1
Report
Observations of solar flare photon energy spectra from 20 keV to 7 MeV
Description
Solar flare photon energy spectra in the 20 keV to 7 MeV range are derived from the Apr. 1, Apr. 4, apr. 27 and May 13, 1981 flares. The flares were observed with a hard x-ray and gamma-ray spectrometers on board the Hinotori satellite. The results show that the spectral shape varies from flare to flare and the spectra harden in energies above about 400 keV. Effects of nuclear line emission on the continuum and of higher energy electron bremsstrahlung are considered to explain the spectral hardening
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
- 19020470
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- BREMSSTRAHLUNG; ENERGY SPECTRA; EXPERIMENTAL DATA; KEV RANGE 10-100; KEV RANGE 100-1000; MEV RANGE 01-10; PHOTON EMISSION; SOLAR ELECTRONS; SOLAR FLARES
- Descriptors DEC
- DATA; ELECTROMAGNETIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; EMISSION; ENERGY RANGE; FERMIONS; INFORMATION; KEV RANGE; LEPTONS; MEV RANGE; NUMERICAL DATA; RADIATIONS; SOLAR ACTIVITY; SOLAR PARTICLES; SOLAR RADIATION; SPECTRA; STELLAR ACTIVITY; STELLAR FLARES; STELLAR RADIATION