Physics
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..134..145f&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 134, July 1991, p. 145-169.
Physics
10
H Alpha Line, Solar Flares, Solar X-Rays, Ultraviolet Radiation, Solar Magnetic Field, Solar Prominences
Scientific paper
Detailed H-alpha, UV-line, and X-ray observations are presented of an extended arch that developed as a consequence of a compact subflare to a length of 300,000 km, in an 'included' magnetic polarity of low magnetic field strength. This great arch was preceded by one an order of magnitude smaller, which masked the polarity inversion line filament in the subflare's early phase. The fact that both arches were simultaneously observed in all spectral domains, as well as their fine structure in H-alpha, is explainable only in terms of an arch composition that encompassed several unresolved portions of material having widely different temperatures.
Farnik Frantisek
Fontenla Juan Manuel
Svestka Zdenek
Tang Frances Y.
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