Doppler observations of solar rotation

Details Doppler observations of solar rotation Doppler observations of solar rotation

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239l..89s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 239, July 15, 1980, p. L89, L90.

Astronomy and Astrophysics

Astrophysics

7

Doppler Effect, Equatorial Atmosphere, Photosphere, Solar Rotation, Magnetic Signatures, Periodic Variations, Solar Atmosphere, Solar Magnetic Field, Sunspots

Scientific paper

Daily observations of the photospheric equatorial rotation rate using the Doppler effect are made at the Stanford Solar Observatory. These observations show no variations in the rotation rate that exceed the observational error of about 1%. The average rotation rate is indistinguishable from that of sunspots and large-scale magnetic field structures.

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