Strong Variability of the Modeled Venus NO Nightglow

Abstract The ultraviolet nightglow of nitric oxide (NO) on Venus offers a unique window into the dynamics and chemistry of its upper atmosphere. We present three‐dimensional simulations of Venus' NO nightglow using a ground‐to‐thermosphere model, revealing a strong, short‐timescale variability consistent with observations. The Venus Planetary Climate Model accurately reproduces the altitude of peak emission at 115 km, matching SPICAV data, and shows an average peak brightness of 53 ± 33 kR, only 5% below the observed values. Crucially, the observed variability and morphology of the NO emission are tightly linked to atmospheric dynamics; its maxima strongly correlate with horizontal wind convergence, leading to localized subsidence. This downward transport is essential for delivering nitrogen atoms to fuel the nightglow, making it a critical tracer for understanding Venus's complex atmospheric circulation. Our findings underscore the importance of the NO nightglow as a powerful diagnostic for the solar‐to‐antisolar circulation on Venus.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2026-04-01
DOI
https://doi.org/10.1029/2025je009316
Citations
1
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
13.98

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article

Strong Variability of the Modeled Venus NO Nightglow

Anni Määttänen, Franck Lefèvre, Aurélien Stolzenbach, Antoine Martinez et al.
1 citations
Journal of Geophysical Research Planets
Planetary Science and Exploration
13.98
article

Strong Variability of the Modeled Venus NO Nightglow

Anni Määttänen, Franck Lefèvre, Aurélien Stolzenbach, Antoine Martinez, S. Lebonnois, Nicolas Streel, Lauriane Soret, J. C. Gérard
article en
1 citations

Abstract

Abstract The ultraviolet nightglow of nitric oxide (NO) on Venus offers a unique window into the dynamics and chemistry of its upper atmosphere. We present three‐dimensional simulations of Venus' NO nightglow using a ground‐to‐thermosphere model, revealing a strong, short‐timescale variability consistent with observations. The Venus Planetary Climate Model accurately reproduces the altitude of peak emission at 115 km, matching SPICAV data, and shows an average peak brightness of 53 ± 33 kR, only 5% below the observed values. Crucially, the observed variability and morphology of the NO emission are tightly linked to atmospheric dynamics; its maxima strongly correlate with horizontal wind convergence, leading to localized subsidence. This downward transport is essential for delivering nitrogen atoms to fuel the nightglow, making it a critical tracer for understanding Venus's complex atmospheric circulation. Our findings underscore the importance of the NO nightglow as a powerful diagnostic for the solar‐to‐antisolar circulation on Venus.

Journal of Geophysical Research PlanetsVol. 131(4)
Centre National de la Recherche Scientifique (FR), École Polytechnique (FR), University of Liège (BE), Université de Versailles Saint-Quentin-en-Yvelines (FR), Université Paris-Saclay (FR), Sorbonne Université (FR), Institute for Basic Science (KR), Institut Pierre-Simon Laplace (FR), Laboratoire atmosphères, milieux, observations spatiales (FR), Instituto de Astrofísica de Andalucía (ES)
Ministerio de Ciencia, Innovación y Universidades, European Commission, Fonds De La Recherche Scientifique - FNRS, Institute for Basic Science, Junta de Andalucía, Agencia Estatal de Investigación
Climate action
Openalex Percentile: Top 1%
Planetary Science and Exploration
13.98
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