Physics
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12..1.1s&link_type=abstract
"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,
Physics
Scientific paper
The all-encompassing ab-initio simulation reaching from the tachocline out to the solar wind is not feasible within the foreseeable future. Therefore, we have to approach the problems of magnetic flux generation, transport, emergence, magneto-convective interaction, equilibrium, dynamics, and dissipation in a piecemeal fashion, focussing upon a realistic (as far as possible) description of the physics in more restricted domains. The last decade has seen significant progress along this line with large-scale simulations of the deep convection zone, of the near-surface layers and photosphere, and in the corona. It has been realized that the magnetic field is the coupling agent of all these domains and first attempts have been made to address the magnetic coupling in simulations. I will go through the various physical domains, and briefly review the respective state of the art, but mainly focus upon the open questions, problems and challenges ahead - of which there are plenty.
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