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Doppler observations of solar rotation
Author(s) -
P. H. Scherrer,
John M. Wilcox
Publication year - 1980
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/183298
Subject(s) - physics , sunspot , solar rotation , doppler effect , rotation (mathematics) , solar physics , astronomy , declination , astrophysics , photosphere , solar atmosphere , observatory , solar irradiance , earth's rotation , magnetic field , spectral line , geometry , mathematics , quantum mechanics
Daily observations of the photospheric equatorial rotation rate using the Doppler effect mode at the Sanford Solar Observatory are presented. These observations show no variations in the rotation rate that exceed the observational error of about one percent. The average rotation rate is indistinguishable from that of sunspots and large scale magnetic field structures.

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