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Large-scale patterns and ‘active longitudes’

Published online by Cambridge University Press:  26 February 2010

Vladimir N. Obridko
Vladimir N. Obridko*
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation RAS, Troitsk, Moscow Region, 142190Russia email: obridko@ismiran.ru
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Abstract

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The following aspects of the physics of large-scale solar magnetic fields are discussed: structure of large-scale fields (LSF) and connection with local fields; dynamo and origin of LSF; LSF cycle variation; meridional circulation and LSF; rotation of LSF; fine structure of the field in quiet regions and the concept of the pebble-shaped field; active longitudes, their manifestation in various solar indices, and dependence on the power of solar activity.

Keywords

Sun: magnetic fieldsrotationsunspots
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 241 - 250
Copyright
Copyright © International Astronomical Union 2010

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