Mathematics – Logic
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...8e..10g&link_type=abstract
Solar and Stellar Activity Cycles, 26th meeting of the IAU, Joint Discussion 8, 17-18 August 2006, Prague, Czech Republic, JD08,
Mathematics
Logic
Scientific paper
Differential rotational rate of the magnetic field measured in the photosphere was calculated and its temporal dependence was studied using two independent methods. It was found that the rotational rate has a periodical character: at high latitudes it is closely related to the solar activity cycle. The shorter periodicities of 5-6 years about have been revealed in the middle and low latitudes in addition to the torsional waves. The variability of solar magnetic field rotation with periods of 1 and 1.25 and 11 years has been analyzed and the results are presented in comparison with the helioseismological findings and the rotational rate of solar corona from UVCS/ SOHO data.
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