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Simulations, Data Analysis and Algorithms

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Figure 21 | Computational Astrophysics and Cosmology

Figure 21

From: The black hole accretion code

Figure 21

Magnetisation on large scales comparing AMR and uniform resolution. 2D logarithmic averaged magnetisation of the magnetised torus with three levels of AMR (left) and uniform resolution \(512 \times512\) (right). Magnetic field lines are traced out by white contour-lines. The averaged quantities are calculated in the time interval of \(t\in[6{,}000\mbox{ M},10{,}000\mbox{ M}]\).

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