The spectral dependence of solar soft X-ray flux values obtained by SOLRAD 9.
Abstract
The determination of solar energy flux values from ionization chamber experiments is discussed. Procedures and calculations necessary for the correction of SOLRAD 9 0.5-3 Å and 1-8 Å data and for the determination of the flare plasma temperature and emission measure are presented. These calculations are based on the continuum spectrum of CULHANE (1969), the line spectrum of TUCKER and KOREN (1971), and experimental values of the detector efficiencies.
- Publication:
-
Journal of Atmospheric and Terrestrial Physics
- Pub Date:
- June 1974
- DOI:
- 10.1016/0021-9169(74)90008-7
- Bibcode:
- 1974JATP...36..989D