Fig. 15
Power per lengthscale derived from the 3D Fourier transform of the densities of the three fluids at t = 40. Formed structures are smaller for the dust species, with dust 1 being the dust species representing the smaller dust particles, and dust 2 representing the larger particles. The ripples at high wavenumber for the gas are due to the AMR, as we choose the active refinement to follow the density variations of the two dust fluids.
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