Fig. 5
Top left: example of a column density map, in logarithmic scale, from a simulation of interstellarMHD turbulence (class 5, see Appendix B). Top right: synthetic Gaussian random field with the same power spectrum. Bottom left: synthetic random field with the same m = 0, m = 1, and m = 2 WST coefficients. Bottom right: synthetic random field with the same m = 0, m = 1, and m = 2 RWST coefficients.
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