Mass motions associated with solar flares

Details Mass motions associated with solar flares Mass motions associated with solar flares

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..215m&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Physics

23

Chromosphere, Mass Transfer, Solar Flares, Coronal Loops, Filtergrams, H Alpha Line, Stellar Mass Ejection

Scientific paper

Mass motions are a principal means by which components of solar flares can be distinguished. Typical patterns of mass motions in H-alpha are described for chromospheric flare ribbons, remote chromospheric flare patches, flare loops, flaring arches, surges, erupting filaments and some expanding coronal features. Interrelationships between these phenomena are discussed and illustrations of each are presented.

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