Changing Magnetic Fields in the Solar Interior

Details Changing Magnetic Fields in the Solar Interior Changing Magnetic Fields in the Solar Interior

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..289b&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

Astronomy and Astrophysics

Astronomy

Scientific paper

Even-order a-coefficients show changes that are correlated with solar activity. We analyze Michelson Doppler Imager (MDI) data that are available for solar cycle 23 to try and determine the change in solar magnetic fields, particularly in the upper part of the convection zone. This is the region where the even-order a-coefficients show the largest change. We use a forward calculation to determine the change in the magnetic fields between the last solar minimum and solar maximum.

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