The rotation of the Sun: Observations at Stanford

Details The rotation of the Sun: Observations at Stanford The rotation of the Sun: Observations at Stanford

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8021240s&link_type=abstract

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Physics

Doppler Effect, Imaging Techniques, Magnetic Signatures, Solar Rotation, Telescopes, Diurnal Variations, Pattern Registration, Periodic Variations, Solar Magnetic Field

Scientific paper

Daily observations of the photospheric rotation rate using the Doppler effect made at the Stanford Solar Observatory since May 1976 are analyzed. Results show that these observations show no daily or long period variations in the rotation rate that exceed the observational error of about one percent. The average rotation rate is the same as that of the sunspot and the large-scale magnetic field structures.

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