Mars

Martian Atmospheric Disturbances From Orbital Images And Surface Pressure At Jezero Crater, Mars, During Martian Year 36

By Keith Cowing
Status Report
astro-ph.EP
January 11, 2025
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Martian Atmospheric Disturbances From Orbital Images And Surface Pressure At Jezero Crater, Mars, During Martian Year 36
The double annular cyclone (DAC). (a) and (b) Two views of DAC on 12 Nov. 2021 (sol 260, Ls = 126°) (MARCI). (c) DAC well developed on 29 Oct. 2021 (sol 247, Ls = 119.6°) (MARCI).. (d)DAC on 17 Nov. 2021 (sol 265, Ls = 128.6°) (VMC). (e) Plot showing the longitude location of the two DAC cyclones in time (West and East edges and Center). (f) Map showing the displacement in longitude and latitude of the two DAC components. — astro-ph.EP

We present a study of atmospheric disturbances at Jezero Crater, Mars, using ground-based measurements of surface pressure by the Perseverance rover in combination with orbital images from the Mars Express and Mars Reconnaissance Orbiter missions.

The study starts at Ls ∼ 13.3° in MY36 (March 6th, 2021) and extends up to Ls ∼ 30.3° in MY37 (February 28th, 2023). We focus on the characterization of the major atmospheric phenomena at synoptic and planetary-scales. These are the thermal tides (measured up to the sixth component), long-period pressure oscillations (periods > 1 sol), the Aphelion Cloud Belt, and the occasional development of regional dust storms over Jezero.

We present the seasonal evolution of the amplitudes and phases of the thermal tides and their relation with the atmospheric dust content (optical depth). Three regional dust storms and one polar storm extending over Jezero produced an increase in the diurnal and semidiurnal amplitudes but resulted in inverse responses in their phases.

We show that the primary regular wave activity is due to baroclinic disturbances with periods of 2-4 sols and amplitudes ∼ 1-15 Pa increasing with dust content, in good agreement with theoretical predictions by model calculations. The spacecraft images show a number of arc-shaped, spiral and irregular cyclonic vortices, traced by dust and clouds at the edge of the North Polar Cap, that could be behind some of the pressure oscillations measured at Jezero.

A. Sánchez-Lavega, E. Larsen, T. del Río-Gaztelurrrutia, J. Hernández-Bernal, I. Ordóñez-Etxebarría, R. Hueso, B. Tanguy, M. Lemmon, M. de la Torre Juarez, G. M. Martínez, A. Munguira, J. A. Rodríguez-Manfredi, A.-M. Harri, J. Pla-García, D. Toledo, C. Newman

Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2501.05337 [astro-ph.EP] (or arXiv:2501.05337v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2501.05337
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Related DOI:
https://doi.org/10.1029/2024JE008565
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Submission history
From: Teresa del Rio Gaztelurrutia Dr
[v1] Thu, 9 Jan 2025 16:07:21 UTC (5,288 KB)
https://arxiv.org/abs/2501.05337
Astrobiology,

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻