Invited Review 1.0: High-Resolution Surface Observations and What They Can Tell MHD Simulations

Abstract

Previous work on the angular momentum balance and meridional circulation of the solar convective zone (SCZ) generally consists either of semi-analytic approaches in which a simple turbulence model is adopted, or full direct numerical simulation (DNS) of the hydrodynamics or magnetohydrodynamics (MHD). In both instances the inclusion of magnetic fields has… (More)

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Cite this paper

@inproceedings{Keller2005InvitedR1, title={Invited Review 1.0: High-Resolution Surface Observations and What They Can Tell MHD Simulations}, author={Christoph Keller and Lokesh Bharti}, year={2005} }