Figure S3. Latitude cross-sections of ACS MIR
CO2 density profiles, grouped in 5° bins corresponding
to equinox seasons: northern spring (a; LS = 330°-30° of
MY 34&35) and northern autumn (b; LS = 160°-220° of MY
35). The color code indicates different orders of magnitude of
CO2 density in the logarithmic scale. Panels c, d show
corresponding data from MCD (Millour et al., 2018) adopted for geography
of the considered MIR occultations. The latitude cross-sections look a
bit nonsmooth (c, d), since each latitude bit correspond to different
longitude and local
time.