Statistical regularities in the solar spectrum

Details Statistical regularities in the solar spectrum Statistical regularities in the solar spectrum

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..260k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, March 1990, p. 260-263. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Solar Atmosphere, Solar Spectra, Spectral Line Width, Fraunhofer Lines, Iron, Statistical Analysis

Scientific paper

The paper examines the dependence of halfwidth and equivalent width for
Fe I lines on their excitation potential observed in the solar spectrum
(Babiia, 1988). It is shown that the dependence can be explained within
the framework of the modern theory of the formation of spectral lines.

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