Flare spray 1982 June 4, 14:24 UT

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photography, H Alpha Line, Pinch Effect, Solar Flares, Solar Prominences, Magnetic Disturbances, Photosphere, Solar Atmosphere, Solar Magnetic Field

Scientific paper

The H-alpha morphology of the white-light impulsive 1B/X2 flare of June 4, 1982, exhibits a pinch-effect signature in the form of a conical plasmoid H-alpha flare structure feature which grew in size at 200 km/sec along the cone's axis (from base to apex). The base of the emission cone was formed by two close ribbons. A narrow emission filament was located along the axis of the flare cone. The flare spray was generated as the final product of the flare cone's development; it 'gushed' from the top of the axial high-energy descending filament. After the generation of the flare spray, an abrupt decrease was observed in the flare cone's length as well as in its H-alpha intensity.

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