A Shallow-Water Theory for the Sun's Active Longitudes

and

Published 2005 December 6 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Mausumi Dikpati and Peter A. Gilman 2005 ApJ 635 L193 DOI 10.1086/499626

1538-4357/635/2/L193

Abstract

We show that the global MHD shallow-water instability of differential rotation and toroidal field bands in the solar tachocline provides a possible mechanism for the formation and evolution of active longitudes seen in synoptic maps of photospheric magnetic fields. The mechanism involves the production of upward bulges at selected longitudes in the overshoot tachocline that contain significant toroidal fields.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/499626