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Impacts of Gravity Waves in the Martian Thermosphere: The Mars Global Ionosphere-Thermosphere Model Coupled With a Whole Atmosphere Gravity Wave Scheme
dc.contributor.authorRoeten, K. J.
dc.contributor.authorBougher, S. W.
dc.contributor.authorYiğit, E.
dc.contributor.authorMedvedev, A. S.
dc.contributor.authorBenna, M.
dc.contributor.authorElrod, M. K.
dc.date.accessioned2023-01-11T16:22:24Z
dc.date.available2024-01-11 11:22:21en
dc.date.available2023-01-11T16:22:24Z
dc.date.issued2022-12
dc.identifier.citationRoeten, K. J.; Bougher, S. W.; Yiğit, E. ; Medvedev, A. S.; Benna, M.; Elrod, M. K. (2022). "Impacts of Gravity Waves in the Martian Thermosphere: The Mars Global Ionosphere- Thermosphere Model Coupled With a Whole Atmosphere Gravity Wave Scheme." Journal of Geophysical Research: Planets 127(12): n/a-n/a.
dc.identifier.issn2169-9097
dc.identifier.issn2169-9100
dc.identifier.urihttps://hdl.handle.net/2027.42/175413
dc.description.abstractGravity waves are a key mechanism that facilitates coupling between the lower and upper atmosphere of Mars. In order to better understand the mean, large-scale impacts of gravity waves on the thermosphere, a modern whole atmosphere, nonlinear, non-orographic gravity wave parameterization scheme has been incorporated into a three-dimensional ground-to-exosphere Mars general circulation model, the Mars Global Ionosphere-Thermosphere Model (M-GITM). M-GITM simulations utilizing the gravity wave parameterization indicate that significant gravity wave momentum is deposited in the thermosphere, especially within the altitude range of 90–170 km. This impacts the winds in the thermosphere; in particular, M-GITM simulations show a decrease in speed of the wind maximum in the summer hemisphere by over a factor of two. Gravity wave effects also impact the temperatures above 120 km in the model, producing a cooler simulated thermosphere at most latitudes. M-GITM results were also compared to upper atmospheric temperature and wind data sets from the MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft. Some aspects of wind data-model comparisons improved once the gravity wave scheme was added to M-GITM; furthermore, a cooler temperature profile produced by these new M-GITM simulations for the MAVEN Deep Dip 2 observational campaign resulted in a closer data-model comparison, particularly above 180 km. Overall, these modeling results show that gravity waves play an important role for the energy and momentum budget of the Martian thermosphere.Plain Language SummaryAtmospheric gravity waves are an important physical process in the upper atmosphere of Mars. To better understand the average effects of gravity waves on the temperatures and winds above 100 km, a modern numerical scheme designed to represent the relevant physics has been added to a 3-D general circulation model, M-GITM (Mars Global Ionosphere-Thermosphere Model), which extends from the surface to about 250 km. Results from these M-GITM simulations show that in the upper atmosphere, the wind maximum in the summer hemisphere decreases in speed by over a factor of two once the effects of gravity waves are added to the model. Additionally, above 120 km, the model now produces a cooler upper atmosphere, on average. The new M-GITM results were also compared to select upper atmospheric temperature and wind data sets from the MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft. Data-model comparisons in upper atmospheric wind speeds for a January 2017 observational campaign improve with the addition of gravity wave effects, as do data-model comparisons for upper atmospheric temperatures for a MAVEN Deep Dip campaign. Overall, these model results show that gravity waves can have significant impacts on the winds and temperature structure in the Martian upper atmosphere.Key PointsLarge-scale impacts of gravity waves in the thermosphere are examined using a modern gravity wave scheme in a Mars general circulation modelSignificant gravity wave momentum deposition is found in model simulations from 90 to 170 km altitudeGravity waves which propagate to the upper atmosphere of Mars can have an appreciable impact on thermospheric winds and temperatures
dc.publisherCambridge University Press
dc.publisherWiley Periodicals, Inc.
dc.subject.othergeneral circulation model
dc.subject.othergravity waves
dc.subject.otherMAVEN
dc.subject.otherthermosphere
dc.subject.otherM-GITM
dc.subject.otherMars
dc.titleImpacts of Gravity Waves in the Martian Thermosphere: The Mars Global Ionosphere-Thermosphere Model Coupled With a Whole Atmosphere Gravity Wave Scheme
dc.typeArticle
dc.rights.robotsIndexNoFollow
dc.subject.hlbsecondlevelGeological Sciences
dc.subject.hlbtoplevelScience
dc.description.peerreviewedPeer Reviewed
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/175413/1/jgre22076.pdf
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/175413/2/jgre22076_am.pdf
dc.identifier.doi10.1029/2022JE007477
dc.identifier.sourceJournal of Geophysical Research: Planets
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dc.working.doiNOen
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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