Flares and coronal heating

Details Flares and coronal heating Flares and coronal heating

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986iraj...17..216b&link_type=abstract

Irish Astronomical Journal (ISSN 0021-1052), vol. 17, March 1986, p. 216-226.

Astronomy and Astrophysics

Astronomy

Solar Corona, Solar Flares, Stellar Coronas, Stellar Flares, Dwarf Stars, Heating, Light Curve, M Stars, X Rays

Scientific paper

Attention is given to a growing body of evidence obtained through both solar and stellar X-ray observations which indicates that flares play a direct role in coronal heating. An evaluation is made of X-ray light curves of impulsive events, the correlation between mean X-ray luminosity and time-averaged luminosity in U-band flare light, and Einstein Observatory X-ray observations of Prox Cen. The optical flares of the latest type M dwarfs, such as Prox Cen, are noted to bear a striking resemblance to solar impulsive X-ray events.

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