Abstract
We consider the effect of vertical outflows on the mean-field dynamo in a thin disk. These outflows could be due to winds or magnetic buoyancy. We analyse both two-dimensional finite-difference numerical solutions of the axisymmetric dynamo equations and a free-decay mode expansion using the thin-disk approximation. Contrary to expectations, a vertical velocity can enhance dynamo action, provided the velocity is not too strong. In the nonlinear regime this can lead to super-exponential growth of the magnetic field.
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Bardou, A., Von Rekowski, B., Dobler, W., Brandenburg, A., & Shukurov, A. (2001). The effects of vertical outflows on disk dynamos. Astronomy and Astrophysics, 370(2), 635–648. https://doi.org/10.1051/0004-6361:20010267
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