Free Access

Fig. 16


Left panel: polar transform of the spectral brightness of the smallest dust size bin of the insolation-driven outgassing model with an absorbing surface. Right panel: integrated brightness at a given radial distance multiplied by the radial distance, I(r)r, as a function of the radial distance, r, calculated according to Eq. (16). The two curves shown correspond to the smallest (8 nm, green line) and largest size bins (0.32 mm, dashed red line) that we ran. The values have been scaled relative to each other at a radial distance of 4000 m from the comet’s centre

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.