The recurrent surges in McMath 9760 and associated surge brightenings

Details The recurrent surges in McMath 9760 and associated surge brightenings The recurrent surges in McMath 9760 and associated surge brightenings

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...73..331z&link_type=abstract

Solar Physics, vol. 73, Oct. 1981, p. 331-339.

Physics

Solar Activity, Solar Physics, Surges, Sunspots, Time Dependence

Scientific paper

A description and discussion are presented concerning the surge activity of Nov. 7-16, 1968 in McMath 9760 region. More than 70 surges were observed, of which some were highly energetic. Some of the surges were accompanied by surge brightenings that were caused by a sharp increase in the velocity of the ejected matter. The region, studied at H-alpha -0.5 A, appeared to be highly stable despite the enhanced activity. Among the characteristics of the surge brightenings are that: (1) they could be seen in the line center while wavelength-scanning; (2) many brightenings started after the surge was already in progress; and (3) only one radio event was recorded during the whole period of observation.

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