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

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

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...97..107v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 97, May 1985, p. 107-112.

Physics

2

H Alpha Line, Solar Flares, Solar X-Rays, Time Lag, Microwaves, Solar Magnetic Field

Scientific paper

This investigation shows that statistically there are significant time delays between Hα and hard X-ray (HXR) emissions during solar flares; most impulsive flares produce HXR emissions up to ≡1 min before and up to 2 min after the onset of Hα emission. HXR emissions are also found to be peaked up to 2 min before the Hα emissions.

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