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Simulations, Data Analysis and Algorithms

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Figure 7 | Computational Astrophysics and Cosmology

Figure 7

From: Stationary relativistic jets

Figure 7

Structure of steady-state magnetized jets obtained via time-dependent 1D simulations. The plots show the co-moving density distribution for model A with \(\kappa=0.5\) and \(\kappa=1\). The distance along the vertical axis is defined as \(z=ct/r_{j}\), where \(r_{j}\) is the initial jet radius. The white contour shows the jet boundary, located using the passive scalar.

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