Determination of the rotation parameters of the solar atmosphere from asymmetries of the Fraunhofer lines

Details Determination of the rotation parameters of the solar atmosphere from asymmetries of the Fraunhofer lines Determination of the rotation parameters of the solar atmosphere from asymmetries of the Fraunhofer lines

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...43g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Jan.-Feb. 1990, p. 43-47. In Russian.

Computer Science

Angular Velocity, Fraunhofer Lines, Rotational Spectra, Solar Atmosphere, Solar Spectra, Spectrum Analysis, Stellar Rotation

Scientific paper

Solar rotation parameters are determined from a comparison between the
central depths and asymmetries of Fraunhofer lines of the sun and at
different distances from the solar center. The effect of rotation on the
central depths and asymmetries of spectral lines is analyzed. A method
for determining the rotation rate of slowly rotating stars is proposed.

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