Physics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..313k&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 129, Oct. 1990, p. 313-324.
Physics
3
Solar Flares, Solar Prominences, Sunspots, H Alpha Line, Solar Corona, Solar Magnetic Field, Stellar Mass Ejection
Scientific paper
On October 22, 1980, near the solar central meridian in the western vicinity of a large spot group, a subflare of the two-ribbon type was observed. Three surges were associated with this flare. Their starting points were situated close to the principal flare patches on both sides of a short filament that was visible for only a few hours. True flow velocities and decelerations along the arch-shaped surge trajectories have been determined for two of the surges. The highest velocities were found at the onset of the surges. The event was studied from a series of H-alpha on- and off-band filtergrams taken with a coronagraph of 53-cm aperture.
Dezso L.
Kovacs Agnes
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