H2 Chemistry and Protonation in the Dayside Venusian Upper Atmosphere
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...
| Published in: | The Astronomical Journal |
|---|---|
| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-3881/ad9d43 |
