Coronal mass ejection associated with the stationary post-flare arch of 21-22 May 1980

Details Coronal mass ejection associated with the stationary post-flare arch of 21-22 May 1980 Coronal mass ejection associated with the stationary post-flare arch of 21-22 May 1980

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..103..399m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 103, no. 2, 1986, p. 399-408. Research supported by the Netherlands Ministry for Education

Physics

14

Solar Corona, Solar Flares, Stellar Mass Ejection, Helios 1, Solar Prominences, Solar X-Rays

Scientific paper

By using a combination of X-ray (HXIS), Hα (Haleakala), white-light corona (Soiwind), and zodiacal light (Helios) images on 21-22 May, 1980 we demonstrate, and try to explain, the co-existence of a coronal mass ejection with a stationary post-flare coronal arch. The mass ejection was seen, both by Solwind and Helios, in prolongation of the path of a powerful spray, whereas the active region filament did not erupt. A tentative comparison is made with other occurrences of stationary, or quasi-stationary post-flare coronal arches.

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