Abstract
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 2563 to 5123.
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© 2005 Springer-Verlag Berlin Heidelberg
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Dobler, W. (2005). Numerical Modelling of Convection and Dynamo Processes in Fully Convective Stars. In: Krause, E., Jäger, W., Resch, M. (eds) High Performance Computing in Science and Engineering’ 04. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-26589-9_5
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DOI: https://doi.org/10.1007/3-540-26589-9_5
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-22943-8
Online ISBN: 978-3-540-26589-4
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