The middle Balmer decrement in quiescent prominences

Details The middle Balmer decrement in quiescent prominences The middle Balmer decrement in quiescent prominences

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...63...87l&link_type=abstract

Solar Physics, vol. 63, Aug. 1979, p. 87-92.

Physics

7

Balmer Series, Solar Prominences, Solar Spectra, H Lines, Iron, Luminous Intensity, Titanium

Scientific paper

Measurements of the middle Balmer decrement (n = 10-22) in a number of quiescent prominences are presented. The average decrement continues smoothly the trend of the decrement determined in our previous work on the earlier Balmer lines. The range of Tex is found to be 3450-11000 K, consistent with the generally accepted range of values for Te. In addition, some values for the hydrogen-to-metal integrated line intensities are given.

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