1. H2 Chemistry and Protonation in the Dayside Venusian Upper Atmosphere
- Author
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Shiqi Wu, Xiaoshu Wu, Yanxing Liu, and Jun Cui
- Subjects
Planetary atmospheres ,Planetary ionospheres ,Venus ,Photoionization ,Astronomy ,QB1-991 - Abstract
Although H _2 is present in low concentrations, it critically controls the structure and composition of planetary upper atmospheres through protonation under solar extreme-ultraviolet and soft X-ray irradiation. Recent studies highlight the importance of protonation on Venus. As H _2 concentrations in its upper atmosphere remain poorly constrained, we conduct a systematic model investigation of how the structure of the topside Venusian ionosphere responds to varying H _2 distributions. Our model results suggest that protonated species could outnumber nonprotonated species in the topside ionosphere when ambient H _2 concentrations exceed 5 ppm. Generally, increasing H _2 concentrations enhances the degree of protonation, manifesting as elevated levels of most protonated species, while nonprotonated species are generally depleted due to rapid reactions with H _2 . These trends, however, are not universal; nonmonotonic variations among multiple species like OH ^+ and O ${}_{2}^{+}$ emerge, driven by the complex chemical network that intricately links species distributions throughout the upper atmosphere. The results presented here provide a foundation for improved characterization of hydrogen escape on Venus during its evolutionary history.
- Published
- 2025
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