Motions in the solar atmosphere associated with the white light flare of 11 July 1978

Physics

Scientific paper

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H Alpha Line, Solar Atmosphere, Solar Flares, Solar Prominences, Sunspots, Coronagraphs, Filaments, Filtergrams, Spatial Resolution, Spectroheliographs, Umbras

Scientific paper

Series of white light heliograms and off- and on-band H-alpha filtergrams were obtained with an average spatial resolution of 1 in. The white light flare patches and several H-alpha flare knots were determined for the umbrae, along with the principal zero filament and an arch prominence. It was suggested that the fully developed flare consisted almost entirely of loops; the zero filament activated prior to the flare was located between two umbrae of common penumbra and opposite polarity. The white light flare developed on both sides of the filament where it passed between the two umbrae; observations indicate that the erupted filament reformed from below.

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