Flaring arches. III - The subflare of June 27, 1980, and its related extended arch

Physics

Scientific paper

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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.

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