A study of the He 10,830-A line emission from quiescent prominences

Details A study of the He 10,830-A line emission from quiescent prominences A study of the He 10,830-A line emission from quiescent prominences

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...50..383l&link_type=abstract

Solar Physics, vol. 50, Nov.-Dec. 1976, p. 383-394.

Physics

11

Emission Spectra, Line Spectra, Solar Prominences, Solar Spectra, Spectral Line Width, Doppler Effect, Fine Structure, H Alpha Line, Helium, Optical Thickness, Spectrum Analysis

Scientific paper

Observations of the He 10,830-A line emission in a number of quiescent prominences are presented. The line shapes are analyzed to obtain values for the Doppler widths and optical thicknesses, leading to a determination of the 2(3)P-2(3)S excitation temperature as 4020 K. The results are compared with those of previous observational and theoretical research.

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