Prominence fine structure. II - Diagnostics

Details Prominence fine structure. II - Diagnostics Prominence fine structure. II - Diagnostics

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..131..107z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 131, Jan. 1991, p. 107-118.

Physics

24

Fine Structure, H Alpha Line, Solar Magnetic Field, Solar Prominences, Normal Density Functions, Solar Corona

Scientific paper

A random-clustering model of prominence fine structure has been applied
to observations of prominence H-alpha spectra. The model yields an
estimate of the number of unresolved elements that form an individual
resolved feature, and sets limits on their velocity and H-alpha profile
dispersions.

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