White-light coronal transients observed from SKYLAB May 1973 to February 1974 - A classification by apparent morphology

Details White-light coronal transients observed from SKYLAB May 1973 to February 1974 - A classification by apparent morphology White-light coronal transients observed from SKYLAB May 1973 to February 1974 - A classification by apparent morphology

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...97..191m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 97, May 1985, p. 191-201.

Physics

19

Coronagraphs, Morphology, Skylab Program, Solar Activity, Solar Corona, Stellar Mass Ejection, Surges

Scientific paper

The apparent morphologies of the major coronal mass ejection transients observed during the Skylab mission with the High Altitude Observatory's white-light coronagraph are described and illustrated. The 77 major events are grouped into classes referred to as Loop, Filled Bottle, Material Injected into Streamer, Ray, Cloud, and Streamer Separation events, with 14 being Unclassifiable because of incomplete observations. One example of each class is shown, with references to others described in the literature. A chronological listing of all the events is given.

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