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Simulations, Data Analysis and Algorithms

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Figure 10 | Computational Astrophysics and Cosmology

Figure 10

From: Stationary relativistic jets

Figure 10

As Figure 8 for model B with \(\pmb{\kappa=1}\) . As the Poynting-flux vanishes on the axis (and the thermal energy is negligible), we obtain a hollow jet with fastest region away from the axis. Due to the increased fast-magneto-sonic speed (thus lower Mach-number) compared to the case of Figure 8, no reconfinement-shock forms and the jet-oscillation frequency is increased.

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