Dynamos with wind
Final Report Abstract
The box simulations of the ISM lead to a full non-linear description of the mean field dynamo in dependence on the local properties like rotation, density and star formation. The saturation mechanism of the dynamo by a wind could be identified. With this complete description of the local dynamo process a sub-grid model for global disk galaxies could be developed. The results mark an important step on which derived mean-field models rely to explain observed equipartition-strength fields. The inclusion of cosmic rays with a diffusion-advection description did not significantly change the growth rate of the dynamo, but the properties of the turbulence became more anisotropic. Under the assumption of equipartition between cosmic rays and magnetic field it was shown by analytic considerations and supported by a global disk simulation, that the effect of the Lorentz force on the gas rotation is rather limited and will not explain a flat rotation curve with the observable matter distribution. This is also supported by recent LOFAR measurements of the synchrotron scale length. The implementation of turbulence properties as sub-grid model in SPMHD is completed. In this connection also a new algorithm using the vector potential for the magnetic field could improve the accuracy of the method by fullfilling its solenoidality.
Publications
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MNRAS, 429, L60
Beck, A. M., Hanasz, M., Lesch, H., Remus, R.-S., Stasyszyn, F. A.
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2013, MNRAS, 428, 13
Stasyszyn, F. A., Dolag, K., Beck, A. M.
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2013, MNRAS, 429, 967
Gressel, O., Bendre, A., Elstner, D.
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2013, MNRAS, 435, 3575
Beck, A.M., Dolag, K., Lesch, H., Kronberg, P.P.
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2014, A&A, 568, 104
Elstner, D., Beck, R., Gressel, O.
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2014, MNRAS, 443, 3107
Lacerna, I., Padilla, N., Stasyszyn, F.
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2015, AN, 336, 991
Bendre, A., Gressel, O., Elstner, D.
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2015, CoPh, 282, 148
Stasyszyn, F.A., Elstner, D.
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2016, JCAP, 056
Beck, M.C., Beck, A.M., Beck, R., Dolag, K. et al.
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2016, MNRAS, 455, 1989
Goicovic, F. G., Cuadra, J., Sesana, A., Stasyszyn, F., Amaro-Seoane, P., Tanaka, T. L.