atmosphere; Mars; Trace Gas Orbiter; water vapor; Geochemistry and Petrology; Geophysics; Earth and Planetary Sciences (miscellaneous); Space and Planetary Science
Abstract :
[en] Slightly less than a Martian Year of nominal science (March 2018–January 2020) with the ExoMars Trace Gas Orbiter has furthered the ongoing investigation of dayside water vapor column abundance. These dayside observations span latitudes between 75°S and 75°N, and all longitudes, which can provide global snapshots of the total water column abundances. In addition to tracking the seasonal transport of water vapor between poles, geographic enhancements are noted, particularly in the southern hemisphere, both in Hellas Basin, and in other regions not obviously correlated to topography. We report consistent water vapor climatology with previous spacecraft observations, however, note a difference in total water vapor content is noted. Finally, we are unable to find evidence for substantial diurnal variation in the total dayside water vapor column.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Crismani, M.M.J. ; Planetary Systems Laboratory, NPP/USRA, NASA Goddard Space Flight Center, Greenbelt, United States ; Department of Physics, California State University, San Bernardino, San Bernardino, United States
Villanueva, G.L.; Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, United States
Liuzzi, G. ; Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, United States ; Department of Physics, College of Arts and Sciences, American University, Washington, United States
Smith, M.D. ; Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, United States
Knutsen, E.W. ; Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, United States ; Department of Physics, College of Arts and Sciences, American University, Washington, United States
Daerden, F. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Neary, L. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Mumma, M.J.; Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, United States
Aoki, Shohei ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Trompet, L. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Thomas, I.R. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Ristic, B. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Bellucci, G. ; Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy
Piccialli, A. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Robert, S. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium ; Institute of Condensed Matter and Nanosciences, Université catholique de Louvain, Louvain-la-Neuve, Belgium
Mahieux, A.; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
Lopez Moreno, J.-J. ; Instituto de Astrofísica de Andalucía, Granada, Spain
Sindoni, G.; Agenzia Spaziale Italiana (ASI), Rome, Italy
Giuranna, M.; Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy
Patel, M.R. ; School of Physical Sciences, The Open University, Milton Keynes, United Kingdom ; Space Science and Technology Department, Science and Technology Facilities Council, Rutherford Appleton Laboratory, Oxfordshire, United Kingdom
Vandaele, A.C. ; Royal Belgian Institute for Space Aeronomy, Brussels, Belgium
M. M. J. Crismani is supported by the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Universities Space Research Association (USRA) under contract with the NASA. This research was supported by the NASA, under grant number GSFC‐604796. ExoMars is a space mission of the European Space Agency (ESA) and Roscosmos. The NOMAD experiment is led by the Royal Belgian Institute for Space Aeronomy (IASB‐BIRA), assisted by Co‐PI teams from Spain (IAA‐CSIC), Italy (INAF‐IAPS), and the United Kingdom (Open University). This project acknowledges funding from the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office (PEA 4000103401 and 4000121493), the Spanish MICINN through its Plan Nacional, the European funds under grants PGC2018‐101836‐B‐I00 and ESP2017‐87143‐R (MINECO/FEDER), as well as the UK Space Agency through grants ST/V002295/1, ST/V005332/1, ST/R001405/1, and ST/S00145X/1, and the Italian Space Agency through grant 2018‐2‐HH.0. BIRA‐IASB acknowledges funding from the European Union's Horizon 2020 research and innovation program under grant agreement number 101004052. The IAA/CSIC team acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (SEV‐2017‐0709). This work was supported by the Belgian Fonds de la Recherche Scientifique – FNRS under grant numbers 30442502 (ET_HOME). This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No.101004052 and T.0171.16 (CRAMIC) and the BELSPO BrainBe SCOOP Project. US investigators were supported by the National Aeronautics and Space Administration. Canadian investigators were supported by the Canada Space Agency. S. Aoki is “Chargé de Recherches” at the F.R.S.‐FNRS. S. Robert thanks BELSPO for the FED‐tWIN funding (Prf‐2019‐077 – RT‐MOLEXO).M. M. J. Crismani is supported by the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Universities Space Research Association (USRA) under contract with the NASA. This research was supported by the NASA, under grant number GSFC-604796. ExoMars is a space mission of the European Space Agency (ESA) and Roscosmos. The NOMAD experiment is led by the Royal Belgian Institute for Space Aeronomy (IASB-BIRA), assisted by Co-PI teams from Spain (IAA-CSIC), Italy (INAF-IAPS), and the United Kingdom (Open University). This project acknowledges funding from the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office (PEA 4000103401 and 4000121493), the Spanish MICINN through its Plan Nacional, the European funds under grants PGC2018-101836-B-I00 and ESP2017-87143-R (MINECO/FEDER), as well as the UK Space Agency through grants ST/V002295/1, ST/V005332/1, ST/R001405/1, and ST/S00145X/1, and the Italian Space Agency through grant 2018-2-HH.0. BIRA-IASB acknowledges funding from the European Union's Horizon 2020 research and innovation program under grant agreement number 101004052. The IAA/CSIC team acknowledges financial support from the State Agency for Research of the Spanish MCIU through the ?Center of Excellence Severo Ochoa? award for the Instituto de Astrof?sica de Andaluc?a (SEV-2017-0709). This work was supported by the Belgian Fonds de la Recherche Scientifique ? FNRS under grant numbers 30442502 (ET_HOME). This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No.101004052 and T.0171.16 (CRAMIC) and the BELSPO BrainBe SCOOP Project. US investigators were supported by the National Aeronautics and Space Administration. Canadian investigators were supported by the Canada Space Agency. S. Aoki is ?Charg? de Recherches? at the F.R.S.-FNRS. S. Robert thanks BELSPO for the FED-tWIN funding (Prf-2019-077 ? RT-MOLEXO).
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