Observations of Very Small Soft X-Ray Flares
Abstract
Data obtained from a proportional counter on OSO-5 are examined to study variations in emission from individual solar active regions within the waveband 0.3-0.9 nm. Flux levels are highly variable, even from the areas having a low mean emission, because increases characteristic of X-ray flares occur most of the time.
- Publication:
-
Solar Physics
- Pub Date:
- September 1974
- DOI:
- 10.1007/BF00161835
- Bibcode:
- 1974SoPh...38..183G
- Keywords:
-
- Radiant Flux Density;
- Solar Flares;
- Solar X-Rays;
- Spaceborne Astronomy;
- X Ray Astronomy;
- Atmospheric Heating;
- Oso-5;
- Proportional Counters;
- Solar Atmosphere;
- Solar Flux Density;
- Solar Physics;
- Flare;
- Active Region;
- Incident Energy;
- Proportional Counter;
- Impulsive Effect