Fig. 11.
Three-dimensional rendering of a symmetric (quadrupolar) halo field combined with a quadrupolar disc field with two reversals at s = 7 kpc and 12 kpc. The domain is a (17 kpc)3 box. The field lines were seeded uniformly along a diagonal through the box. The arrows show the magnetic field at points randomly sampled within the slice of a thickness 2.5 kpc around the galactic mid-plane (which is indicated by the semi-transparent surface) and are scaled according to the magnitude of the magnetic field.
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