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Solar rotation measurements at Mount Wilson
Authors:Barry J. Labonte  Robert Howard
Affiliation:(1) Mount Wilson and Las Campanas Observatories, Carnegie Institution of Washington, U.S.A.
Abstract:The lsquoearsrsquo velocity pattern described in Paper I (Howard et al., 1980) had no physical explanation. A reanalysis shows that the large scale solar velocity patterns are better described by a nonmonotonic limbshift and a meridional flow. The results of the new analysis imply that the study of solar velocity pattern at the level of a few ms–1 required that magnetic regions be treated separately from nonmagnetic regions.Now at: Institute for Astronomy, University of Hawaii, Honolulu, Hawaii 96822, U.S.A.
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