The possibility of improving a homogeneous model of the solar photosphere

Details The possibility of improving a homogeneous model of the solar photosphere The possibility of improving a homogeneous model of the solar photosphere

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...18g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, May-June 1988, p. 18-24. In Russian.

Physics

4

Photosphere, Solar Spectra, Stellar Models, Fraunhofer Lines, Oscillator Strengths, Solar Temperature, Solar Velocity

Scientific paper

The differences in oscillator strengths derived from equivalent widths and central intensities of different Fraunhofer lines are analyzed in the case of variations of the photospheric model nominal temperature and velocity field characteristics. These features are found to be dependent on the equivalent width and excitation potential; they can be used to improve the photospheric model on the basis of an analysis of a large number of empirical solar oscillator strengths derived from different Fraunhofer lines.

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