Rotation of the solar photosphere according to observations of the central depths of Fraunhofer lines

Details Rotation of the solar photosphere according to observations of the central depths of Fraunhofer lines Rotation of the solar photosphere according to observations of the central depths of Fraunhofer lines

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1r..53g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Nov.-Dec. 1985, p. 53-55. In Russian.

Computer Science

2

Fraunhofer Lines, Photosphere, Solar Atmosphere, Solar Rotation, Solar Spectra, Angular Velocity, Spectral Resolution

Scientific paper

The solar rotation velocity for different heliographic latitudes was
determined from a comparison of the central depths of Fraunhofer lines
in the spectrum of the sun as a star with the central depths of the same
lines at different distances from the solar center. A value of
(2.07-0.30 sin squared phi)cos phi was obtained.

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