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

Open Access

Fig. 18

Noise reduction on Taurus L1495. Top panel: singularity exponents of the Herschel observation of Taurus L1495 at 250 μm after noise reduction: p = 1.5, q = −1, λ = 0.1. Bottom panel: zoom onto southern subregion.

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