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in the middle atmosphere are among the most critical for understanding
oxygen chemistry in the Venus middle atmosphere.
Acknowledgments
Part of this research was carried out at the Jet Propulsion Laboratory, Cal-
ifornia Institute of Technology, under contract with NASA. Funding from
NASA's Planetary Atmospheres program, the Australian Research Coun-
cil, the Asia Oceania Geosciences Society, and the International Society of
Biometeorology Tromp Travel Fund is gratefully acknowledged.
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