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Gravity Wave Observations by the Mars Science Laboratory REMS Pressure Sensor and Comparison with Mesoscale Atmospheric Modeling with MarsWRFSurface pressure measurements on Mars have revealed a wide variety of atmospheric phenomena. The Mars Science Laboratory Rover Environmental Monitoring Station pressure sensor dataset is now the longest duration record of surface pressure on Mars. We use the first 2580 martian sols, nearly 4 Mars years,of measurements to identify atmospheric pressure waves with periods of tens of minutes to hours using wavelet analysis on residual pressure after the tidal harmonics are removed. We find these waves have a clear diurnal cycle with strongest activity in the early morning and late evening and a seasonal cycle with the strongest waves in the second half of the martian year (Ls= 180-360°). The strongest such waves of the entire mission occurred during the Mars Year 34 global dust storm. Comparable atmospheric waves are identified using atmospheric modeling with the MarsWRF general circulation model in a “nested” high spatial resolution mode. With the support of the modeling, we find these waves best fit the expected properties of inertia-gravity waves with horizontal wavelengths of O(100s) of km.

PLAIN LANGUAGE SUMMARY

Measuring air pressure from the surface of Mars has revealed a wide variety of atmospheric phenomena. The Curiosity rover's record or surface air pressure is now the longest yet made on Mars.We use the first ~8 years of Curiosity's pressure observations to look for atmospheric waves with periods of tens of minutes to hours. We find these waves have a clear pattern in their daily behavior with the strongest activity in the early morning and late evening and a seasonal cycle with the strongest waves in the second half of the martian year (Northern hemisphere fall and winter). The strongest such waves occurred in 2018 during a global dust storm. We find comparable waves in atmospheric modeling. With the support of modeling, we find these waves best fit the expected properties of buoyancy waves forced by airflow over topography with horizontal wavelengths of 100-1000 km.
Document ID
20210022894
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Scott D Guzewich
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Manuel De La Torre Juarez
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Claire E Newman
(Aeolis Research (United States) Pasadena, California, United States)
Emily Mason
(University of Maryland, Baltimore Baltimore, Maryland, United States)
Michael D Smith
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Nina Miller
(University of Nevada Reno Reno, Nevada, United States)
Alain S J Khayat
(University of Maryland, College Park College Park, Maryland, United States)
Henrik Kahanpaa
(Aalto University Helsinki, Finland)
Daniel Viudez-Moreiras
(Centro de Astrobiología Torrejón de Ardoz, Spain)
Mark I Richardson
(Aeolis Research (United States) Pasadena, California, United States)
Date Acquired
October 15, 2021
Publication Date
July 15, 2021
Publication Information
Publication: Journal of Geophysical Research Planets
Publisher: Wiley/AGU
Volume: 126
Issue: 8
Issue Publication Date: August 1, 2021
ISSN: 2169-9097
e-ISSN: 2169-9100
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
WBS: 857464.04.09.04.07
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee