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Fig. 6

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Venus composition profiles for PH3, PO, and H3PO4 predicted with our photochemistry model for scenarios 1a (solid blue line), 1b (dashed blue line), 2a (solid orange line), and 2b (dashed orange line). We additionally show the observational ranges from Greaves et al. (2020, 2021b) and upper limits of Trompet et al. (2021).

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