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arXiv · 1210.6606

On the magnetic field required for driving the observed angular-velocity variations in the solar convection zone

H. M. Antia·S. M. Chitre·D. O. Gough
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Abstract

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.

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H. M. Antia, S. M. Chitre, D. O. Gough. 2012-10-11. On the magnetic field required for driving the observed angular-velocity variations in the solar convection zone. https://doi.org/10.1093/mnras%2Fsts040

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