2005 | OriginalPaper | Chapter
Numerical Modelling of Convection and Dynamo Processes in Fully Convective Stars
Author : Wolfgang Dobler
Published in: High Performance Computing in Science and Engineering’ 04
Publisher: Springer Berlin Heidelberg
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In the current project, we simulate thermal convection and generation of magnetic fields inside a fully convective star, like an M-dwarf or a T-tauri star. The numerical resolution required to reasonably well describe convection properties inside the star is 256
3
to 512
3
.