Calculation of the populations of He levels in a flare

Details Calculation of the populations of He levels in a flare Calculation of the populations of He levels in a flare

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53..832m&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, July-Aug. 1976, p. 832-835. In Russian.

Astronomy and Astrophysics

Astronomy

Atomic Energy Levels, Helium Atoms, Line Spectra, Population Theory, Solar Flares, Astronomical Models, D Lines, Density Distribution, Optical Density, Stellar Models

Scientific paper

Equations for the stationary populations of the 1 1-S, 2 3-S, and 2 3-P
levels of helium in a solar flare are obtained and they are solved using
a flare model of Pikel'ner and Kostyuk (1974). The model allows one to
determine the optical depths of the D3 and 10830 A He lines in a flare
and He column densities in the 2 3-P states.

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