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Mass Motions Associated with Solar Flares

Published online by Cambridge University Press:  12 April 2016

Sara F. Martin
Sara F. Martin*
Affiliation:
Big Bear Solar Observatory, California Institute of Technology, Pasadena, CÁ 91125, U.S.A.

Abstract

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Mass motions are a principal means by which components of solar flares can be distinguished. Typical patterns of mass motions in Ha are described for chromospheric flare ribbons, remote chromo-spheric 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.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 104 , Issue 1: Solar and Stellar Flares , 1989 , pp. 215 - 238
Copyright
Copyright © Kluwer 1989

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