Fig. 3.

Fiducial runs with kturb = 2: maps of the gas density (top panels), cosmic-ray energy density (middle panels), and Alfvénic Mach number (bottom panels) in the plane z = 20 pc at a time corresponding to 2tcross. From left to right panels: CR diffusion coefficient is D0 = 1022, 1024, 1026, and 1028 cm2 s−1. The arrows on the density maps represent the velocity vectors (normalised to a value of 14 km s−1, see upper right panel), and the streamlines on the CR energy density maps represent the magnetic field lines, both in the xy-plane.
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