The gas pressure in solar prominences

Details The gas pressure in solar prominences The gas pressure in solar prominences

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...140..449h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 140, no. 2, Nov. 1984, p. 449-452. Sponsorship: Deutsche Forschungsgemeinschaf

Astronomy and Astrophysics

Astrophysics

3

Gas Pressure, Solar Prominences, Solar Spectra, Calcium, Emission Spectra, H Alpha Line, H Beta Line

Scientific paper

Attention is given to the results of new measurements of the emission relation of Ca(+)8542 and H-beta, which indicate that the emission ratio E(Ca/+/8542)/E(H-beta), at about 0.16, is significantly lower than the value of about 0.3 obtained by Landsman et al. (1977). The presently undertaken comparison of these results with those of the Heasley and Milkey (1978) model indicates that a much higher value of the gas pressure, approximately 0.1 dyn/sq cm, must be assumed in order to match the observed lower ratio.

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