A study of velocity fields of flare regions

Details A study of velocity fields of flare regions A study of velocity fields of flare regions

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acasn..26..251x&link_type=abstract

(Acta Astronomica Sinica, vol. 26, no. 3, 1985, p. 251-253) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, March

Astronomy and Astrophysics

Astrophysics

Magnetic Flux, Radial Velocity, Solar Flares, Solar Magnetic Field, Velocity Distribution, Current Sheets, H Alpha Line, Magnetic Energy Storage

Scientific paper

In the present analysis of velocity field maps for four instants before and during the July 14, 1980 solar flare, obvious changes in the velocity field are held to furnish support for the emergent magnetic flux model. The characteristic time of energy storage is noted to be as short as 1 hr, if newly emergent flux is the primary energy source. Observations also indicate that there may be more than one current sheet at the flare maximum.

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