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Magneto-Convection: Structure and Dynamics

Published online by Cambridge University Press:  14 March 2005

Robert F. Stein  and
Åke Nordlund
Robert F. Stein
Affiliation:
Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA, email: [email protected]
Åke Nordlund
Affiliation:
NBIfAFG, Copenhagen University, Copenhagen, DK, email: [email protected]
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Abstract

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We present results from realistic, high resolution, simulations of solar magneto-convection. Simulations were run with both a mean vertical and a mean horizontal field. The magnetic field is quickly swept out of the granules and meso-granules and concentrated in the intergranular lanes.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 179 - 182
Copyright
© 2004 International Astronomical Union