Parameter dependences of convection-driven dynamos in rotating spherical fluid shells

@inproceedings{Simitev2006ParameterDO,
  title={Parameter dependences of convection-driven dynamos in rotating spherical fluid shells},
  author={Radostin D. Simitev},
  year={2006}
}
For the understanding of planetary and stellar dynamos an overview of the major parameter dependences of convection driven dynamos in rotating spherical fluid shells is desirable. Although the computationally accessible parameter space is limited, earlier work is extended with emphasis on higher Prandtl numbers and uniform heat flux condition at the outer boundary. The transition from dynamos dominated by non-axisymmetric components of the magnetic field to those dominated by the axisymmetric… CONTINUE READING

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