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Mars 2020 Perseverance Rover Studies of the Martian Atmosphere Over Jezero From Pressure MeasurementsThe pressure sensors on Mars rover Perseverance measure the pressure field in the Jezero crater on regular hourly basis starting in sol 15 after landing. The present study extends up to sol 460 encompassing the range of solar longitudes from Ls ∼ 13°–241° (Martian Year (MY) 36). The data show the changing daily pressure cycle, the sol-to-sol seasonal evolution of the mean pressure field driven by the CO2 sublimation and deposition cycle at the poles, the characterization of up to six components of the atmospheric tides and their relationship to dust content in the atmosphere. They also show the presence of wave disturbances with periods 2–5 sols, exploring their baroclinic nature, short period oscillations (mainly at night-time) in the range 8–24 min that we interpret as internal gravity waves, transient pressure drops with duration ∼1–150 s produced by vortices, and rapid turbulent fluctuations. We also analyze the effects on pressure measurements produced by a regional dust storm over Jezero at Ls ∼ 155°.
Document ID
20230001083
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
A. Sánchez-Lavega ORCID
(University of the Basque Country Leioa, Spain)
T. Del Rio-Gaztelurrutia ORCID
(University of the Basque Country Leioa, Spain)
R. Hueso ORCID
(University of the Basque Country Leioa, Spain)
M. De La Torre Juárez ORCID
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
G. M. Martínez
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
A.-M. Harri
(Finnish Meteorological Institute Helsinki, Finland)
M. Genzer
(Finnish Meteorological Institute Helsinki, Finland)
M. Hieta ORCID
(Finnish Meteorological Institute Helsinki, Finland)
J. Polkko ORCID
(Finnish Meteorological Institute Helsinki, Finland)
J. A. Rodríguez-Manfredi
(Centro de Astrobiología Torrejón de Ardoz, Spain)
M. T. Lemmon ORCID
(Space Science Institute Boulder, Colorado, United States)
J. Pla-García ORCID
(Centro de Astrobiología Torrejón de Ardoz, Spain)
D. Toledo ORCID
(National Institute for Aerospace Technology Madrid, Spain)
A. Vicente-Retortillo
(Centro de Astrobiología Torrejón de Ardoz, Spain)
D. Viúdez-Moreiras ORCID
(Centro de Astrobiología Torrejón de Ardoz, Spain)
A. Munguira ORCID
(University of the Basque Country Leioa, Spain)
L. K. Tamppari ORCID
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
C. Newman ORCID
(Aeolis Research (United States) Pasadena, California, United States)
J. Gómez-Elvira
(National Institute for Aerospace Technology Madrid, Spain)
S. Guzewich ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
T. Bertrand
(Paris Observatory Paris, Île-de-France, France)
V. Apéstigue ORCID
(National Institute for Aerospace Technology Madrid, Spain)
I. Arruego ORCID
(National Institute for Aerospace Technology Madrid, Spain)
M. Wolff ORCID
(Space Science Institute Boulder, Colorado, United States)
D. Banfield
(Cornell University Ithaca, New York, United States)
I. Jaakonaho ORCID
(Finnish Meteorological Institute Helsinki, Finland)
T. Mäkinen
(Finnish Meteorological Institute Helsinki, Finland)
Date Acquired
January 23, 2023
Publication Date
November 1, 2022
Publication Information
Publication: Journal of Geophysical Research: Planets
Publisher: American Geophysical Union / Wiley
Volume: 128
Issue: 1
Issue Publication Date: January 1, 2023
ISSN: 2169-9097
e-ISSN: 2169-9100
Subject Category
Space Sciences (General)
Instrumentation and Photography
Funding Number(s)
WBS: 588733.04.04
CONTRACT_GRANT: J-090011
CONTRACT_GRANT: 80NM0018D0004
CONTRACT_GRANT: J-090015
CONTRACT_GRANT: 1511125
CONTRACT_GRANT: PID2019-109467GB-I00
CONTRACT_GRANT: USRA 1638782
PROJECT: MDM-2017-0737
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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