1 code implementation • 10 Sep 2018 • A. Shukurov, L. F. S. Rodrigues, P. J. Bushby, J. Hollins, J. P. Rachen
We present a simple, yet realistic and flexible model for large-scale magnetic fields in astrophysical discs (in particular, spiral galaxies and accretion discs) obtained as an approximate solution of the averaged induction equation in the turbulent disc and halo.
Astrophysics of Galaxies
