Fig. 1.
Position of the CO2 (gray), PH3 (red), and SO2 (blue) ro-vibrational transitions in the 2348 to 2501 cm−1 region, corresponding to the SOIR 105 to 111 diffraction orders from HITRAN (Gordon et al. 2017). The line intensities were multiplied by typical Venus abundances, see legend. The SOIR orders are given at the top, with the vertical dashed lines showing their wavenumber extensions.
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