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Simulations, Data Analysis and Algorithms

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Figure 3 | Computational Astrophysics and Cosmology

Figure 3

From: Riemann solvers and Alfven waves in black hole magnetospheres

Figure 3

HLL Riemann solver vs. HLLI Riemann solver contact discontinuity. Figure 3 shows two simulations of an isolated, stationary Alfven wave. The transverse velocity and magnetic field are shown. The result from the HLL Riemann solver is shown with crosses while the result from the HLLI Riemann solver is shown with dots.

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