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On the branching in the emission relations of Ca+ in prominences
Authors:G Stellmacher  E Wiehr
Institution:(1) Institut d'Astrophysique de Paris, CNRS, 98 bis, Bd. Arago, F75014 Paris, France;(2) Universitäts-Sternwarte, Geismarlandstr. 11, D34 Göttingen, Germany
Abstract:Spatially well resolved prominence spectra of the three lines Ca+ K, Hbeta, and Ca+ 8542 are analysed. It is confirmed that the branching in the emission relations of Ca+ versus Hbeta correlates with the magnitude of non-thermal (turbulent) broadening.
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