A coronal condensation observed at the total solar eclipse of June 11, 1983 and a related transient prominence

Details A coronal condensation observed at the total solar eclipse of June 11, 1983 and a related transient prominence A coronal condensation observed at the total solar eclipse of June 11, 1983 and a related transient prominence

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..285s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 116, no. 2, 1988, p. 285-290.

Physics

1

Coronal Loops, Solar Eclipses, Solar Prominences, Filtergrams, H Alpha Line, Solar Flares, Transient Response

Scientific paper

A coronal condensation was observed simultaneously with Fe XIV λ5303, Fe X λ6374, Fe XI λ7892, and Hα filtergraphs. The size and shape of the condensation in λ5303 are different from those in other filtergrams. Hα filtergrams taken around the eclipse time show that a small transient prominence exists in close proximity to the condensation core and behaves like a post-flare loop system, though the appearance is quite different and no flare-report exists. A small-scale energetic phenomenon seems to have occurred at the top of magnetic loops.

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