Free Access

Fig. A.8


Panel a: spatial distribution of dust optical depth at 9.3 μm (Montabone et al. 2020) averaged between Ls = 107.5–117.5° over a map of Mars. We also show the tangent point locations of ACS MIR solar occultations. We highlight occultations made using position 11, those in which HCl was observed, and those with coincident TIRVIM observation (northern only). Panel b: vertical profiles of HCl VMR from ACS MIR and dustmass loading from ACS TIRVIM (Luginin et al. 2020) for the coincident observation at (46°N, 97°W).

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.