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On the magnetic field required for driving the observed angular-velocity variations in the solar convection zone View all abstracts by submitter

Douglas Gough   Submitted: 2012-10-03 07:47

A putative temporally varying circulation-free magnetic-field configuration is inferred in an equatorial segment of the solar convection zone from the helioseismologically inferred angular-velocity variation, assuming that the predominant dynamics is angular acceleration produced by the azimuthal Maxwell stress exerted by a field whose surface values are consistent with photospheric line-of-sight measurements.

Authors: H.M. Antia, S.M. Chitre, D.O.Gough
Projects: None

Publication Status: to appear in MNRAS
Last Modified: 2012-10-03 11:24
Go to main E-Print page  Heliophysics gleaned from seismology  Magnetic Field Structures Triggering Solar Flares and Coronal Mass Ejections  Edit Entry  Download Preprint  Delete Entry 

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