Time delay between H-alpha and soft X-ray emissions during solar flares
Abstract
A statistical analysis of time delays between H-alpha and soft X-ray (SXR) emissions at onset and peak respectively during solar flares is presented. The authors find that at the onset of flares SXR emission starts simultaneously or up to two min earlier than H-alpha emissions. At peak flux the SXR emission is found to be peaked between 2 min before to 3 min after the H-alpha emissions.
- Publication:
-
Bulletin of the Astronomical Society of India
- Pub Date:
- June 1985
- Bibcode:
- 1985BASI...13..148V
- Keywords:
-
- H Alpha Line;
- Solar Flares;
- Solar X-Rays;
- Time Lag;
- Solar Physics