Time delay between H-alpha and soft X-ray emissions during solar flares

Details Time delay between H-alpha and soft X-ray emissions during solar flares Time delay between H-alpha and soft X-ray emissions during solar flares

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13..148v&link_type=abstract

Astronomical Society of India, Bulletin, vol. 13, June 1985, p. 148-152.

Astronomy and Astrophysics

Astronomy

3

H Alpha Line, Solar Flares, Solar X-Rays, Time Lag

Scientific paper

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.

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