The rotation of the solar atmosphere at different altitudes

Details The rotation of the solar atmosphere at different altitudes The rotation of the solar atmosphere at different altitudes

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1066g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Sept.-Oct. 1987, p. 1066-1071. In Russian.

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Solar Atmosphere, Solar Rotation, Velocity Distribution, Vertical Distribution, Altitude, Computational Astrophysics, Line Spectra

Scientific paper

A new method for determining the solar rotation velocity is proposed. A comparison was made between the observed central depths of Fraunhofer lines in the spectrum of the sun as a star and calculations based on center-limb observations. For altitudes in the range of 100-1100 km above the level of the continuous spectrum, the solar rotation velocity hardly changes.

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