On the Orientational Relaxation of Bipolar Active Regions

Details On the Orientational Relaxation of Bipolar Active Regions On the Orientational Relaxation of Bipolar Active Regions

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003padeu..13...95t&link_type=abstract

In: Contributions to NATO Advanced Research Workshop Turbulence, Waves, and Instabilities in the Solar Plasma; Hungary, 16-20 Se

Astronomy and Astrophysics

Astronomy

Scientific paper

Our work on the basis of selected regular bipolar magnetic regions (BMRs) strengthens the assumption that the scatter of tilt angles of BMRs around Joy`s law is determined by the convective turbulence. Furthermore, regular BMRs grouped by age do not show the phenomenon of toroidal relaxation, which may probably mean the disconnection of Omega-loops from the bottom of the convection zone.

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