EMIRS Observations of the Aphelion‐Season Mars Atmosphere

Abstract Thermal infrared spectra taken by the Emirates Mars Infrared Spectrometer (EMIRS) on‐board the Emirates Mars Mission (EMM) spacecraft are well suited for the retrieval of surface temperatures, the atmospheric temperature profile from the surface to ∼40 km, and the column abundance of dust a...

Full description

Saved in:
Bibliographic Details
Main Authors: Michael D. Smith, Khalid Badri, Samuel A. Atwood, Christopher S. Edwards, Philip R. Christensen, Michael J. Wolff, Tanguy Bertrand, François Forget, Eman Al Tunaiji, Christopher Wolfe, Nathan Smith, Saadat Anwar
Format: Article
Language:English
Published: Wiley 2022-08-01
Series:Geophysical Research Letters
Online Access:https://doi.org/10.1029/2022GL099636
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1850198383928541184
author Michael D. Smith
Khalid Badri
Samuel A. Atwood
Christopher S. Edwards
Philip R. Christensen
Michael J. Wolff
Tanguy Bertrand
François Forget
Eman Al Tunaiji
Christopher Wolfe
Nathan Smith
Saadat Anwar
author_facet Michael D. Smith
Khalid Badri
Samuel A. Atwood
Christopher S. Edwards
Philip R. Christensen
Michael J. Wolff
Tanguy Bertrand
François Forget
Eman Al Tunaiji
Christopher Wolfe
Nathan Smith
Saadat Anwar
author_sort Michael D. Smith
collection DOAJ
description Abstract Thermal infrared spectra taken by the Emirates Mars Infrared Spectrometer (EMIRS) on‐board the Emirates Mars Mission (EMM) spacecraft are well suited for the retrieval of surface temperatures, the atmospheric temperature profile from the surface to ∼40 km, and the column abundance of dust aerosols, water ice clouds, and water vapor. A constrained linear inversion retrieval routine that includes multiple scattering has been developed and optimized for this purpose. Here, we present a brief overview of the retrieval algorithm and first atmospheric science results from observations taken by EMIRS over the first Earth year of EMM Science Phase operations. These retrievals show extensive water ice clouds, typical for the aphelion season of these observations, and the expected north polar summer maximum and subsequent equatorward transport of water vapor is well documented. An unusually strong and early regional dust storm and its associated thermal response were also observed.
format Article
id doaj-art-18d59def9c574f35862ccb066e1dcda3
institution OA Journals
issn 0094-8276
1944-8007
language English
publishDate 2022-08-01
publisher Wiley
record_format Article
series Geophysical Research Letters
spelling doaj-art-18d59def9c574f35862ccb066e1dcda32025-08-20T02:12:53ZengWileyGeophysical Research Letters0094-82761944-80072022-08-014915n/an/a10.1029/2022GL099636EMIRS Observations of the Aphelion‐Season Mars AtmosphereMichael D. Smith0Khalid Badri1Samuel A. Atwood2Christopher S. Edwards3Philip R. Christensen4Michael J. Wolff5Tanguy Bertrand6François Forget7Eman Al Tunaiji8Christopher Wolfe9Nathan Smith10Saadat Anwar11NASA Goddard Space Flight Center Greenbelt MD USAMohammed bin Rashid Space Center Dubai UAESpace and Planetary Science Center, and Department of Earth Sciences Khalifa University Abu Dhabi UAEDepartment of Astronomy and Planetary Science Northern Arizona University Flagstaff AZ USASchool of Earth and Space Exploration Arizona State University Tempe AZ USASpace Science Institute Boulder CO USALaboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique (LESIA) Observatoire de Paris Université PSL CNRS Sorbonne Université Univ. Paris Diderot Sorbonne Paris Cité FranceLMD/IPSL Sorbonne Université PSL Research Université École Normale Supérieure, École Polytechnique CNRS Paris FranceMohammed bin Rashid Space Center Dubai UAEDepartment of Astronomy and Planetary Science Northern Arizona University Flagstaff AZ USADepartment of Astronomy and Planetary Science Northern Arizona University Flagstaff AZ USASchool of Earth and Space Exploration Arizona State University Tempe AZ USAAbstract Thermal infrared spectra taken by the Emirates Mars Infrared Spectrometer (EMIRS) on‐board the Emirates Mars Mission (EMM) spacecraft are well suited for the retrieval of surface temperatures, the atmospheric temperature profile from the surface to ∼40 km, and the column abundance of dust aerosols, water ice clouds, and water vapor. A constrained linear inversion retrieval routine that includes multiple scattering has been developed and optimized for this purpose. Here, we present a brief overview of the retrieval algorithm and first atmospheric science results from observations taken by EMIRS over the first Earth year of EMM Science Phase operations. These retrievals show extensive water ice clouds, typical for the aphelion season of these observations, and the expected north polar summer maximum and subsequent equatorward transport of water vapor is well documented. An unusually strong and early regional dust storm and its associated thermal response were also observed.https://doi.org/10.1029/2022GL099636
spellingShingle Michael D. Smith
Khalid Badri
Samuel A. Atwood
Christopher S. Edwards
Philip R. Christensen
Michael J. Wolff
Tanguy Bertrand
François Forget
Eman Al Tunaiji
Christopher Wolfe
Nathan Smith
Saadat Anwar
EMIRS Observations of the Aphelion‐Season Mars Atmosphere
Geophysical Research Letters
title EMIRS Observations of the Aphelion‐Season Mars Atmosphere
title_full EMIRS Observations of the Aphelion‐Season Mars Atmosphere
title_fullStr EMIRS Observations of the Aphelion‐Season Mars Atmosphere
title_full_unstemmed EMIRS Observations of the Aphelion‐Season Mars Atmosphere
title_short EMIRS Observations of the Aphelion‐Season Mars Atmosphere
title_sort emirs observations of the aphelion season mars atmosphere
url https://doi.org/10.1029/2022GL099636
work_keys_str_mv AT michaeldsmith emirsobservationsoftheaphelionseasonmarsatmosphere
AT khalidbadri emirsobservationsoftheaphelionseasonmarsatmosphere
AT samuelaatwood emirsobservationsoftheaphelionseasonmarsatmosphere
AT christophersedwards emirsobservationsoftheaphelionseasonmarsatmosphere
AT philiprchristensen emirsobservationsoftheaphelionseasonmarsatmosphere
AT michaeljwolff emirsobservationsoftheaphelionseasonmarsatmosphere
AT tanguybertrand emirsobservationsoftheaphelionseasonmarsatmosphere
AT francoisforget emirsobservationsoftheaphelionseasonmarsatmosphere
AT emanaltunaiji emirsobservationsoftheaphelionseasonmarsatmosphere
AT christopherwolfe emirsobservationsoftheaphelionseasonmarsatmosphere
AT nathansmith emirsobservationsoftheaphelionseasonmarsatmosphere
AT saadatanwar emirsobservationsoftheaphelionseasonmarsatmosphere