On the branching in the emission relations of Ca/+/ in prominences

Details On the branching in the emission relations of Ca/+/ in prominences On the branching in the emission relations of Ca/+/ in prominences

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...71..299s&link_type=abstract

Solar Physics, vol. 71, June 1981, p. 299-309.

Physics

6

Calcium, Emission Spectra, Line Spectra, Solar Prominences, Solar Spectra, Spectral Correlation, Balmer Series, Branching (Physics), H Beta Line, K Lines, Spectral Line Width

Scientific paper

Spatially well resolved prominence spectra of the three lines Ca(+) K,
H-beta and Ca(+) 8542 are analyzed. It is confirmed that the branching
in the emission relations of Ca(+) versus H-beta correlates with the
magnitude of nonthermal (turbulent) broadening.

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