High-resolution observations of H-alpha flare regions

Details High-resolution observations of H-alpha flare regions High-resolution observations of H-alpha flare regions

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ssrv...51...49k&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 51, Oct. 1989, p. 49-84.

Physics

36

H Alpha Line, High Resolution, Solar Activity, Solar Flares, Solar Magnetic Field, Light Curve, Magnetic Field Configurations, Solar Optical Telescope, Spatial Resolution, Temporal Distribution

Scientific paper

Recent high-resolution H-alpha observations of solar flares and flare-productive active regions are reviewed. Two types of two-ribbon flares, separating and confined two-ribbon flares, are discussed. Temporal relationships between H-alpha line intensities or profiles and hard X-ray or microwave emissions are examined. It is suggested that the production of a major flare may require the successive emergence of a twisted magnetic flux rope.

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