Numerical Modelling of Convection and Dynamo Processes in Fully Convective Stars

  • Wolfgang Dobler
Conference paper


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.


Magnetic Field Differential Rotation Meridional Circulation Protoplanetary Disc Stellar Surface 
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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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