Three-Dimensional MHD Simulation of Convection and Emerging Flux

Details Three-Dimensional MHD Simulation of Convection and Emerging Flux Three-Dimensional MHD Simulation of Convection and Emerging Flux

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325...63i&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

1

Scientific paper

We present results of three dimensional magnetohydrodynamic simulation of convection and emerging flux. Although simulations of emerging flux tube have been presented in the literature, effect of convection on the dynamics of emerging flux has not been studied in detail. We carried out simulation of emergence of twisted flux tube from vigorously convecting convection zone. It is found that the flux tube emerges to the upper atmosphere and forms loop like structures, but finally it is broken by the convecting flows and loses its coherence in several turnover time of convection.

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