Solar differential rotation reflected in the distribution of background magnetic fields

Details Solar differential rotation reflected in the distribution of background magnetic fields Solar differential rotation reflected in the distribution of background magnetic fields

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987baicz..38...29b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 38, Jan. 1987, p. 29-36.

Astronomy and Astrophysics

Astronomy

9

Magnetic Flux, Solar Activity, Solar Magnetic Field, Solar Rotation, Angular Velocity, Polar Regions, Solar Radiation

Scientific paper

It is demonstrated that the differential rotation rates estimated with the use of weak remnants of magnetic fields measured with a very low resolution during the periods of low solar activity and in regions of the photosphere with very low density of new magnetic flux sources are between the differential rotation values obtained with the aid of highly averaged sunspot data and from the daily magnetic field measurements. The effects disturbing the smooth changes of solar rotation velocity values with heliographic latitude, seen clearly in the distribution of magnetic fields as solar differential rotation parabolas, are briefly discussed.

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