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

descriptionPublicationkeyboard_double_arrow_right Article 01 Sep 1988 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 116, pages 285-290 (issn: 0038-0938, eissn: 1573-093X,

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Authors: Yoshinori Suematsu; Sumisaburo Saito; Yasuhiro Funakoshi; Hiroki Kurokawa;

doi: 10.1007/bf00157479

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

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Abstract

A coronal condensation was observed simultaneously with Fexiv λ5303, Fex 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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Kyoto University
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Shiga University
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