Figure S1. Validation of the temperature
vertical profiles from ACS MIR (T MIR) and ACS NIR
(T NIR; Fedorova et al., 2022) retrieved over 1.5
considered Martian years. a: differences
(T MIR-T NIR) as a function
of altitude for all the simultaneous observations (green points) made
during MY 34 and MY 35. Black curve is the average for points grouped in
the altitude interval of 2 km, error bars are corresponding standard
deviations. b: T MIR as a function ofT NIR. The gray dashed lines in these panels
indicate the expected trend if T MIR =T NIR.