Hydroxide salts in the clouds of Venus: their effect on the sulfur cycle and cloud droplet pH
Paul B. Rimmer, Sean Jordan, Tereza Constantinou, Peter, Woitke, Oliver Shorttle, Alessia Paschodimas, Richard Hobbs

TL;DR
This study investigates how hydroxide salts in Venus's cloud droplets influence the sulfur cycle and pH, proposing that salts buffer SO$_2$ depletion and can be tested by future atmospheric probes.
Contribution
It introduces the role of hydroxide salts in cloud droplets as a key factor in Venus's sulfur chemistry and cloud pH regulation, expanding current understanding.
Findings
SO$_2$ depletion explained by low SO$_2$ levels or salt-buffered dissolution.
Cloud droplet pH around 1 at 50 km due to salts.
Salts flux of approximately 10^{-13} mol cm^{-2} s^{-1} inferred.
Abstract
The depletion of SO and HO in and above the clouds of Venus (45 -- 65 km) cannot be explained by known gas-phase chemistry and the observed composition of the atmosphere. We apply a full-atmosphere model of Venus to investigate three potential explanations for the SO and HO depletion: (1) varying the below-cloud water vapor (HO), (2) varying the below-cloud sulfur dioxide (SO), and (3) the incorporation of chemical reactions inside the sulfuric acid cloud droplets. We find that increasing the below-cloud HO to explain the SO depletion results in a cloud top that is 20 km too high, above-cloud O three orders of magnitude greater than observational upper limits and no SO above 80 km. The SO depletion can be explained by decreasing the below-cloud SO to . The depletion of SO in the clouds can also be explained by the SO…
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