Analysis of instability of latitudinal differential rotation and toroidal field in the solar tachocline using a magnetohydrodynamic shallow-water model. I. Instability for broad toroidal field profiles

Gilman, A.; Dikpati, Mausumi

doi:10.1086/341799

Gilman, P. A., & Dikpati, M. (2002). Analysis of instability of latitudinal differential rotation and toroidal field in the solar tachocline using a magnetohydrodynamic shallow-water model. I. Instability for broad toroidal field profiles. The Astrophysical Journal, 576, 1031-1047. doi:10.1086/341799

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Journal Articles

Published Version: http://dx.doi.org/10.1086/341799

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Author(s)

Peter A. Gilman-NCAR/UCAR

Mausumi Dikpati-NCAR/UCAR

Title

Analysis of instability of latitudinal differential rotation and toroidal field in the solar tachocline using a magnetohydrodynamic shallow-water model. I. Instability for broad toroidal field profiles

Publication Title

The Astrophysical Journal

Date

2002-09-10

Volume

576

Issue

Pages

1031-1047

Resource Type

article

Peer Review

Refereed

Copyright Information

Publisher's Version of Record

http://dx.doi.org/10.1086/341799

OpenSky Citable URL

http://n2t.net/ark:/85065/d74q7vcj

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Analysis of instability of latitudinal differential rotation and toroidal field in the solar tachocline using a magnetohydrodynamic shallow-water model. I. Instability for broad toroidal field profiles

In collections