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. 24

Spider: singularity spectrum and noise reduction. Top panel: singularity exponents of the Herschel observation of Spider at 250 μm. Left: display of the singularity exponents of the raw, unfiltered map. Right: after noise reduction: p = 1.3, q = −1, λ = 0.1. Bottom panel: zoom onto subregion (filtered map).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.