On the magnetic field required for driving the observed angular-velocity variations in the solar convection zone
Solar and Stellar Astrophysics
2015-06-11 v1
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.
Keywords
Cite
@article{arxiv.1210.6606,
title = {On the magnetic field required for driving the observed angular-velocity variations in the solar convection zone},
author = {H. M. Antia and S. M. Chitre and D. O. Gough},
journal= {arXiv preprint arXiv:1210.6606},
year = {2015}
}
Comments
to appear in MNRAS