HDO and SO2 thermal mapping on Venus - V. Evidence for a long-term anti-correlation

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Fig. 9

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Maps of the line depth ratio of the weak HDO transition (at 1344.90 cm⁻¹) to the CO₂ transition at 1345.22 cm⁻¹, recorded during the February 2019 run. Data are the same as in Figs. 2 and 5. The sub-solar point is shown as a white dot. Times refer to the mid-times of the observations.

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