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The future of helioseismology

Published online by Cambridge University Press:  21 October 2010

Alexander G. Kosovichev
Alexander G. Kosovichev*
Affiliation:
Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA email: AKosovichev@solar.stanford.edu
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Abstract

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Helioseismology has provided us with the unique knowledge of the interior structure and dynamics of the Sun, and the variations with the solar cycle. However, the basic mechanisms of solar magnetic activity, formation of sunspots and active regions are still unknown. Determining the physical properties of the solar dynamo, detecting emerging active regions and observing the subsurface dynamics of sunspots are among the most important and challenging problems. The current status and perspectives of helioseismology are briefly discussed.

Keywords

Sun: helioseismologyactivityinterior magnetic fieldsoscillationssunspots
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 352 - 353
Copyright
Copyright © International Astronomical Union 2010

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