A loop prominence system observed on May 24, 1972.
Abstract
A flare-loop prominence appeared over a complex sunspot group in McMath region No. 11895, on May 24,1972. The evolution of the loop prominence and its relation to a flare were observed using Hα and Ca K filters. Soft X-ray emission between 0.5-20 Å was found to be emitted from the flare-loop prominence system.
- Publication:
-
Solar Physics
- Pub Date:
- October 1978
- DOI:
- 10.1007/BF00951840
- Bibcode:
- 1978SoPh...59..357D
- Keywords:
-
- H Alpha Line;
- Solar Flares;
- Solar Prominences;
- Solar X-Rays;
- Sunspots;
- K Lines;
- Solar Spectra;
- X Ray Spectra;
- Solar Physics;
- Flare;
- Sunspot Group;
- Prominence System;
- Loop Prominence;
- Complex Sunspot;
- Solar Flares:Solar Prominences