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Fig. 15.

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Face-on rendering of the divergence error of the magnetic field in the galactic disk after t = 2 Gyr. We can clearly see that there is a reduction in divergence error throughout the disk for higher Jeans floor. The mean divergence error in the NJ = 8 is around ϵdiv, B = 10−1 and in the NJ = 16 around ϵdiv, B = 6 × 10−2.
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