Flaring arches. II - Events in the arch system of 6/7 November, 1980

Details Flaring arches. II - Events in the arch system of 6/7 November, 1980 Flaring arches. II - Events in the arch system of 6/7 November, 1980

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..123..317s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 123, no. 2, 1989, p. 317-341. Research supported by SRON.

Physics

17

Coronal Loops, Solar Flares, Solar X-Rays, X Ray Spectra, H Alpha Line, Oxygen Spectra, Solar Activity

Scientific paper

A characterization is developed for the 57,000-km long arch-shaped coronal structure of November 6, 1980, which became the site, first, of 13 quasi-periodic X-ray brightenings, and then of a series of 17 flaring arches. A comparison of H-alpha, O V, and X-ray data for the SB arch has qualitatively confirmed that a hot conduction front producing X-rays in the least dense plasma is first present, and is followed by a decelerating, denser plasma bulk in O V, with an eventual, still-further-decelerating very dense plasma becoming visible in H-alpha emission.

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