Measurements of line emission in quiescent prominences - Ca/+/, H and He

Astronomy and Astrophysics – Astrophysics

Scientific paper

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H Lines, Solar Corona, Solar Prominences, Solar Spectra, Stellar Spectrophotometry, Abundance, Astronomical Models, Calcium, Helium Atoms, Hydrogen Atoms, Metal Ions

Scientific paper

The paper presents observations of Ca(+) H, K, and infrared-triplet integrated line intensities, as well as H-beta, H-gamma and He 5876-A throughout eight quiescent prominences. The data were obtained with a multichannel coronal spectrophotometer system. The presently available theoretical models appear to be insufficient to provide a consistent basis for the interpretation of the data.

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