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Numerical Modelling of Convection and Dynamo Processes in Fully Convective Stars

  • Wolfgang Dobler
Conference paper

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.

Keywords

Magnetic Field Differential Rotation Meridional Circulation Protoplanetary Disc Stellar Surface 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • Wolfgang Dobler
    • 1
  1. 1.Kiepenheuer-Institut für SonnenphysikFreiburg

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