Magnetic Tilts and Polarity Separations in Sunspot Groups and Active Regions the Cycle 23

Details Magnetic Tilts and Polarity Separations in Sunspot Groups and Active Regions the Cycle 23 Magnetic Tilts and Polarity Separations in Sunspot Groups and Active Regions the Cycle 23

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...8e..50z&link_type=abstract

Solar and Stellar Activity Cycles, 26th meeting of the IAU, Joint Discussion 8, 17-18 August 2006, Prague, Czech Republic, JD08,

Computer Science

Scientific paper

We present the analysis of magnetic tilts in active regions and sunspot groups for 1996-2005 that are automatically extracted from the Solar Feature Catalogues (http://solar.inf.brad.ac.uk ). We investigate the statistical variations of magnetic field tilt in sunspot groups and whole active regions, their longitudinal and latitudinal distributions, drifts and daily polarity separation during different phases of the solar cycle 23. The classification results are compared with the similar research for the previous cycles and the specifics on the cycle 23 is discussed in conjunction to the solar dynamo theory.

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