High-Latitude Zonal Jets in the Martian Upper Atmosphere Driven by Non-Orographic Gravity Waves

Fuente: arXiv
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Main Authors: Liu, Jiandong, Forget, François, Millour, Ehouarn, Galindo, Francisco González, Chaufray, Jean-Yves
Format: Preprint
Published: 2026
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author Liu, Jiandong
Forget, François
Millour, Ehouarn
Galindo, Francisco González
Chaufray, Jean-Yves
author_facet Liu, Jiandong
Forget, François
Millour, Ehouarn
Galindo, Francisco González
Chaufray, Jean-Yves
contents We investigate thermosphere responses to non-orographic gravity waves (GWs) using wind measurements from the Neutral Gas and Ion Mass Spectrometer onboard the Mars Atmosphere and Volatile EvolutioN mission, alongside simulations from the Mars Planetary Climate Model. We focus on zonal jets in high-latitude regions of the upper atmosphere. Jet acceleration and deceleration (280 m/s ) arise from momentum divergence (1,300 m/s/sol ) driven by wave saturation and wind filtering. Simulations and observations indicate that GWs modulate these jets in the hemisphere associated with the descending branches of the Hadley Cell, due to the absence of wave critical layers in the middle atmosphere. Interactions between GWs and the mean flow can shape the circulation and dynamics of the upper atmosphere of Mars.
format Preprint
id arxiv_https___arxiv_org_abs_2605_21730
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle High-Latitude Zonal Jets in the Martian Upper Atmosphere Driven by Non-Orographic Gravity Waves
Liu, Jiandong
Forget, François
Millour, Ehouarn
Galindo, Francisco González
Chaufray, Jean-Yves
Earth and Planetary Astrophysics
We investigate thermosphere responses to non-orographic gravity waves (GWs) using wind measurements from the Neutral Gas and Ion Mass Spectrometer onboard the Mars Atmosphere and Volatile EvolutioN mission, alongside simulations from the Mars Planetary Climate Model. We focus on zonal jets in high-latitude regions of the upper atmosphere. Jet acceleration and deceleration (280 m/s ) arise from momentum divergence (1,300 m/s/sol ) driven by wave saturation and wind filtering. Simulations and observations indicate that GWs modulate these jets in the hemisphere associated with the descending branches of the Hadley Cell, due to the absence of wave critical layers in the middle atmosphere. Interactions between GWs and the mean flow can shape the circulation and dynamics of the upper atmosphere of Mars.
title High-Latitude Zonal Jets in the Martian Upper Atmosphere Driven by Non-Orographic Gravity Waves
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2605.21730