A Sandwich Interface Dynamo: Linear Dynamo Waves in the Sun

Details A Sandwich Interface Dynamo: Linear Dynamo Waves in the Sun A Sandwich Interface Dynamo: Linear Dynamo Waves in the Sun

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004apj...602..468z&link_type=abstract

The Astrophysical Journal, Volume 602, Issue 1, pp. 468-480.

Astronomy and Astrophysics

Astronomy

9

Magnetohydrodynamics: Mhd, Sun: Magnetic Fields

Scientific paper

The existence of the solar tachocline inferred from helioseismology leads to the concept of an interface dynamo. The tachocline, where the strong toroidal magnetic field is generated and stored, is sandwiched between and magnetically coupled to the radiative interior and the overlying convection zone. We investigate a linear sandwich interface dynamo in Cartesian geometry. The dynamo model consists of four horizontal layers: an electrically conducting layer at -∞

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