Continuous-spectrum energy distribution of flares, moustaches, and emission grains
Abstract
Data on the continuous spectra of solar flares, moustaches, and grains are reviewed. The contrast of emission grains increases towards the violet; the contrast of moustaches is practically independent of wavelength; the contrast of flares slightly increases towards the red. Energy distribution curves have a maximum at 4100-4200 A for the grains and 4400-4500 A for moustaches and flares.
- Publication:
-
Izvestiya Ordena Trudovogo Krasnogo Znameni Krymskoj Astrofizicheskoj Observatorii
- Pub Date:
- 1979
- Bibcode:
- 1979IzKry..59...64K
- Keywords:
-
- Continuous Spectra;
- Solar Flares;
- Solar Spectra;
- Spectral Energy Distribution;
- Solar Granulation;
- Spectrograms;
- Solar Physics