Physics
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998soph..183..263c&link_type=abstract
Solar Physics, v. 183, Issue 2, p. 263-276 (1998).
Physics
16
Scientific paper
We present a new method for measuring the solar magnetic meridional flow, and provide a comparison with other recent work. We have performed a least-squares fit to azimuthally averaged Mount Wilson Observatory synoptic data encompassing Carrington rotations 1722 to 1929 to produce an estimate of the solar meridional flow. A parametric fit to our results expresses the solar meridional flow as v(phi) = 28.5sin2.5phicosphi.
Cameron Robert
Hopkins Andrew
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