Helioseismic probing of the solar dynamo

Details Helioseismic probing of the solar dynamo Helioseismic probing of the solar dynamo

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517...71r&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

Physics

3

Helioseismology, Solar Dynamo

Scientific paper

According to theoretical predictions, the solar dynamo operating in the convection zone generates maximal magnetic fields near the base of the convection zone. Detection of this field is a challenging task for helioseismology. We discuss the ways of probing the magnetic field in the solar interior and estimate the magnitude of the field that can be detected with presently achievable accuracy. It is easier, however, to detect the flows that drive the dynamo. We describe the major flow parameters related to the dynamo flows and present the requirements for measurement of these parameters with local helioseismic techniques.

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