Magnetohydrodynamic ``Shallow Water'' Equations for the Solar Tachocline

Details Magnetohydrodynamic ``Shallow Water'' Equations for the Solar Tachocline Magnetohydrodynamic ``Shallow Water'' Equations for the Solar Tachocline

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...544l..79g&link_type=abstract

The Astrophysical Journal, Volume 544, Issue 1, pp. L79-L82.

Astronomy and Astrophysics

Astronomy

40

Hydrodynamics, Magnetohydrodynamics: Mhd, Sun: Interior, Sun: Magnetic Fields, Sun: Rotation

Scientific paper

We argue that the classical ``shallow water'' equations of geophysical
fluid dynamics should be useful for studying the global dynamics of the
solar tachocline and demonstrate the existence of an MHD analog that
would allow taking into account the strong toroidal magnetic field
likely to be present there.

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