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. 19

Taurus: singularity spectrum and noise reduction. Left panel: singularity spectra of Taurus L1495 observation map with and without noise reduction. Middle panel: log-normal fit to raw data. Right panel: log-normal fit after noise reduction: p = 1.5, q = −1, λ = 0.1.

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