Fine structure of the Fraunhofer lines: observation results and their interpretation.

Details Fine structure of the Fraunhofer lines: observation results and their interpretation. Fine structure of the Fraunhofer lines: observation results and their interpretation.

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990knft....6r...3a&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 6, No. 6, p. 3 - 20

Physics

Fraunhofer Lines: Fine Structure

Scientific paper

The review embraces results of the spectral line observations and their theoretical interpretation. The empirical data on the line asymmetry and absolute wavelength shifts are presented for the solar centre, for different positions on the solar limb and for the Sun as a star. Their dependence on the phase of the solar activity cycle is also reviewed. Interpretation of these data on the basis of semiempirical models is discussed. The multidimensional numerical simulation results of convective motions in the superadiabatic region and in the solar photosphere are presented.

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