A model of a quiescent prominence on the basis of studying the K Ca(+) line fine structure

Details A model of a quiescent prominence on the basis of studying the K Ca(+) line fine structure A model of a quiescent prominence on the basis of studying the K Ca(+) line fine structure

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...87...43g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 87, Aug. 1983, p. 43-46.

Physics

1

K Lines, Solar Prominences, Solar Spectra, Fine Structure, Radial Velocity, Stellar Structure

Scientific paper

A model of a quiescent prominence with nonparallel structural elements is given, based on a study of the K Ca+ line fine structure of two quiescent prominences. The dependences of the radial velocities on the height found for the structural elements making up the prominence (Gigolashvili and Zhugzhda, 1982) gives the information on the inner spatial structure of the prominence. Analysis of the available data allows to suggest an alternative model of a quiescent prominence.

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