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Three-dimensional simulations of turbulent spectra in the local interstellar medium

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Academic year: 2021

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Figure

Fig. 1. Schematic of the Mach number as determined from the scale flows (left) and small-scale fluctuations (right)
Fig. 2. Snap-shot of turbulent magnetic field in three dimensions.
Fig. 4. Nonlinear compressible magnetofluid MHD simula- simula-tions, in both three and two dimensions, show a decay of tur-bulent supersonic Mach number M˜ s to below unity
Fig. 5. Spectral energy transfer among shear Alfv´en mode (k SAM ) and slow/fast magnetosonic waves (k SFM ) during a dissipative com-pressible MHD simulation is shown (left y-axis)
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