Polarization properties of synchrotron sources from simulations of relativistic magnetohydrodynamic turbulence

Open Access

Fig. 2.

Time sequences of rms quantities for a selection of four runs, choosing a varying σ₀ while keeping σ₁ = 0.1 fixed. In the upper panels we show the total current density, J = |∇×B|, J_∥ (along B₀), and J_⊥, whereas in the bottom ones we plot $B / \sqrt{E_{0}}$ $B/\sqrt{\mathcal{E}_0}$ , basically the Alfvén speed, and v, again total, parallel, and perpendicular components, adopting the same notations.

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