Differential rotation and the SPOT zones

Details Differential rotation and the SPOT zones Differential rotation and the SPOT zones

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...43...87d&link_type=abstract

Solar Physics, vol. 43, July 1975, p. 87-90.

Physics

12

Angular Velocity, Astronomical Models, Photosphere, Solar Rotation, Sunspots, Velocity Measurement, Doppler Effect, Fine Structure, Line Spectra, Solar Atmosphere, Solar Cycles, Spectroheliographs

Scientific paper

Doppler measurements, using the Capri magnetograph, of the latitudinal fine structure of the solar differential rotation have been carried out. The positions of the photospheric lines C I 5380.32 and Fe I 5364.88 have been simultaneously recorded. In contrast to Gilman's model (1972) which predicted an equatorial deceleration of the differential rotation, a minimum of angular velocity is found at a latitude of 6 degrees in both hemispheres.

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