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Fig. 1

image

Spectra recorded by ACS MIR at 5.5 km using secondary grating position 12 during occultation 2476 N1 on Ls = 192.7°: (a) contributions from O3, H2O, and CO2 to the best-fit for orders 180–182; (b) data and best-fits for orders 180–182.

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