Preprints
https://doi.org/10.5194/egusphere-2025-2908
https://doi.org/10.5194/egusphere-2025-2908
08 Aug 2025
 | 08 Aug 2025
Status: this preprint is open for discussion and under review for Geoscientific Model Development (GMD).

Benchmarking Photolysis Rates: Species for Earth and Exoplanets

Sophia Adams, James Manners, Nathan Mayne, Mei Ting Mak, and Eric Hebrard

Abstract. Using the Socrates photolysis scheme, we present newly calculated photolysis rates under modern Earth atmospheric conditions for species directly relevant to Earth and species relevant to different atmospheric compositions. We compare to a previous photolysis comparison exercise, namely PhotoComp 2011. Overall, we find good agreement between our results and previous work, with discrepancies usually caused by the implementation of temperature dependent cross-sections or quantum yields and updated or higher resolution input data. We provide a new set of benchmark photolysis rates for additional species both for Solar irradiance and when irradiated by an M dwarf host star. In general, the higher actinic flux at far-UV and shorter wavelengths of the M dwarf compared to the Sun drives increased photolysis rates for reactions with high threshold energies. This work provides an updated set of benchmark results for further studies of photolysis in the Earth's atmosphere and that of other planets.

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Sophia Adams, James Manners, Nathan Mayne, Mei Ting Mak, and Eric Hebrard

Status: open (until 19 Oct 2025)

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  • CEC1: 'Comment on egusphere-2025-2908', Astrid Kerkweg, 10 Sep 2025 reply
Sophia Adams, James Manners, Nathan Mayne, Mei Ting Mak, and Eric Hebrard
Sophia Adams, James Manners, Nathan Mayne, Mei Ting Mak, and Eric Hebrard

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Short summary
We perform calculations of photolysis reactions using an existing model but including updated input data. These reactions are important in shaping the composition of our upper atmosphere and that of other planets, for example, controlling ozone formation and destruction. The results of our model are compared with those of previous benchmarks, and rates of various reactions provided to facilitate other researchers in developing accurate schemes to capture photolysis in planetary atmospheres.
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