Physics
Scientific paper
Oct 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..175s&link_type=abstract
Space Science Reviews, Volume 70, Issue 1-2, pp. 175-180
Physics
Sun, Prominences, Uv Radiation
Scientific paper
Ultraviolet spectra of a quiescent prominence observed with theHigh Resolution Telescope and Spectrograph (HRTS) are analyzed. Different techniques lead to greatly different spatial scales for the prominence structures. The UV spectra show strong variations in intensity and Doppler shift on scales larger than 1700 km. Spectroscopic diagnostics employing line intensity ratios indicate the existence of scales between 400 m to some hundred kilometers. We attempt to interpret various aspects of the prominence intensities and velocities with a multiple thread model.
Dere Ken P.
Schmieder Brigitte
Wiik Jun Elin
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