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Simulations, Data Analysis and Algorithms

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Figure 4 | Computational Astrophysics and Cosmology

Figure 4

From: Riemann solvers and Alfven waves in black hole magnetospheres

Figure 4

Torsional Alfven wave dissipation test. Figure 4 shows the results of the torsional Alfven wave dissipation test. A second order WENO reconstruction was used in all these tests. Figure 4a shows the decay in the z-component of the velocity as a function of time. Figure 4b shows the same for the z-component of the magnetic field.

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