Turbulent transport coefficients in spherical wedge dynamo simulations of solar-like stars

To analyze the dynamo mechanism we apply the test-field method for azimuthally averaged fields to determine the 27 turbulent transport coefficients of the electromotive force, of which six are related to the alpha tensor.


Run directories:

  • Fig. B.1

    References:

    Warnecke, J., Rheinhardt, M., Käpylä, P. J., Käpylä, M. J., & Brandenburg, A.: 2018, ``Turbulent transport coefficients in spherical wedge dynamo simulations of solar-like stars,'' Astron. Astrophys. 609, A51 (arXiv:1601.03730, ADS, DOI, PDF)


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    Axel Brandenburg
    $Date: 2020/01/17 04:16:51 $, $Author: brandenb $, $Revision: 1.2 $