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Simulations, Data Analysis and Algorithms

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Figure 6 | Computational Astrophysics and Cosmology

Figure 6

From: The black hole accretion code

Figure 6

Error quantification: magnetised Bondi flow. Error of density ρ in the highly magnetised Bondi flow: \(\sigma=10^{3}\) (left) and \(\sigma=10^{4}\) (right). The black data points are obtained with the standard 2D inversion and the red datapoints switch to the entropy inversion at \(\beta\le10^{-2}\). One can see that both recipes are convergent with the expected order and that the error in the entropy strategy is decreased by roughly a factor of two.

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