@inproceedings{c44072cff5ed4b4abd1f615112dc6038,
title = "Toroidal field reversals",
abstract = "I present axisymmetric numerical simulations of the solar interior, with differential rotation imposed in the convection zone and tachocline and a dipolar poloidal field confined to the radiative interior. In these simulations toroidal field reversals which are equator-ward propagating are driven in the absence of a dynamo. These reversals are driven in the tachocline and are seen at the top of the convection zone. While not solar-like in many ways, these reversals do show some solar-like properties not previously seen in full MHD simulations.",
keywords = "Magnetic fields, Sun: interior",
author = "Rogers, {T. M.}",
year = "2010",
month = jun,
doi = "10.1017/S1743921311017455",
language = "English (US)",
isbn = "9780521197397",
series = "Proceedings of the International Astronomical Union",
number = "S271",
pages = "62--68",
editor = "Nicholas Brummell and Sacha Brun and Mark Boulder and Yannick Ponty",
booktitle = "Astrophysical Dynamics",
edition = "S271",
}