Description of turbulent dynamics in the interstellar medium: Multifractal microcanonical analysis - II. Sparse filtering of Herschel observation maps and visualization of filamentary structures at different length scales

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Fig. D.2

Same experiment as in Fig. D.1, but with λ = 10⁻¹. This figure demonstrates the sensitivity of the optimization process in Eq. 8 with respect to parameter λ.

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