Prominence fine structure

Details Prominence fine structure Prominence fine structure

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..127..109z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 127, May 1990, p. 109-118.

Physics

32

Fine Structure, Solar Prominences, Solar Spectra, H Alpha Line, Optical Thickness, Spectrum Analysis

Scientific paper

The vertical fine structure in a quiescent prominence was modeled as an
assembly of very narrow, optically thin threads. Random clusterings of
the threads can account for the observed contrast and H-alpha line
profiles of the fine structures. In this picture, each structure
consists of a cluster of 7-20 elementary threads.

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