Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model

We examined the observed temperature data from Thermal Emission Spectrometer (TES) between heliocentric longitude L_s = 141° and 146° (∼10 Martian days in northern summer) during the mapping phase, then compared them with the simulated results using the NASA/Ames Mars general circulation model. Both...

Full description

Bibliographic Details
Published in:Journal of Geophysical Research: Planets
Main Authors: Zhang, Kate Q., Ingersoll, Andrew P., Kass, David M., Pearl, John C., Smith, Michael D., Conrath, Barney J., Haberle, Robert M.
Format: Article in Journal/Newspaper
Language:English
Published: American Geophysical Union 2001
Subjects:
Online Access:https://authors.library.caltech.edu/37499/
https://authors.library.caltech.edu/37499/1/2000JE001330.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411
id ftcaltechauth:oai:authors.library.caltech.edu:37499
record_format openpolar
spelling ftcaltechauth:oai:authors.library.caltech.edu:37499 2023-05-15T17:39:56+02:00 Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model Zhang, Kate Q. Ingersoll, Andrew P. Kass, David M. Pearl, John C. Smith, Michael D. Conrath, Barney J. Haberle, Robert M. 2001-12-25 application/pdf https://authors.library.caltech.edu/37499/ https://authors.library.caltech.edu/37499/1/2000JE001330.pdf https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411 en eng American Geophysical Union https://authors.library.caltech.edu/37499/1/2000JE001330.pdf Zhang, Kate Q. and Ingersoll, Andrew P. and Kass, David M. and Pearl, John C. and Smith, Michael D. and Conrath, Barney J. and Haberle, Robert M. (2001) Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model. Journal of Geophysical Research E, 106 (E12). pp. 32863-32877. ISSN 0148-0227. doi:10.1029/2000JE001330. https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411 <https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411> other Article PeerReviewed 2001 ftcaltechauth https://doi.org/10.1029/2000JE001330 2021-11-11T18:53:10Z We examined the observed temperature data from Thermal Emission Spectrometer (TES) between heliocentric longitude L_s = 141° and 146° (∼10 Martian days in northern summer) during the mapping phase, then compared them with the simulated results using the NASA/Ames Mars general circulation model. Both show a strong polar vortex at the winter pole, higher equatorial temperatures near the ground and larger tropospheric lapse rates during daytime than at night. However, the simulation is colder than the observation at the bottom and top of the atmosphere and warmer in the middle. The highest wave activities are found in the polar front in both the simulations and the observations, but it is at a much higher altitude in the former. Experiments show that larger dust opacity improves the temperature field in the lower atmospheric levels. Using a steady state Kalman filter, we attempted to obtain a model state that is consistent with the observations. The assimilation did achieve better agreement with the observations overall, especially over the north pole. However, it is hard to make any further improvement. Dust opacity is the key factor in determining the temperature field; correcting temperature alone improves the spatial and temporal variations, it degrades the mean state in the south pole. Assimilation cannot improve the simulation further, unless more realistic dust opacity and its vertical profile are considered. Article in Journal/Newspaper North Pole South pole Caltech Authors (California Institute of Technology) South Pole North Pole Journal of Geophysical Research: Planets 106 E12 32863 32877
institution Open Polar
collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language English
description We examined the observed temperature data from Thermal Emission Spectrometer (TES) between heliocentric longitude L_s = 141° and 146° (∼10 Martian days in northern summer) during the mapping phase, then compared them with the simulated results using the NASA/Ames Mars general circulation model. Both show a strong polar vortex at the winter pole, higher equatorial temperatures near the ground and larger tropospheric lapse rates during daytime than at night. However, the simulation is colder than the observation at the bottom and top of the atmosphere and warmer in the middle. The highest wave activities are found in the polar front in both the simulations and the observations, but it is at a much higher altitude in the former. Experiments show that larger dust opacity improves the temperature field in the lower atmospheric levels. Using a steady state Kalman filter, we attempted to obtain a model state that is consistent with the observations. The assimilation did achieve better agreement with the observations overall, especially over the north pole. However, it is hard to make any further improvement. Dust opacity is the key factor in determining the temperature field; correcting temperature alone improves the spatial and temporal variations, it degrades the mean state in the south pole. Assimilation cannot improve the simulation further, unless more realistic dust opacity and its vertical profile are considered.
format Article in Journal/Newspaper
author Zhang, Kate Q.
Ingersoll, Andrew P.
Kass, David M.
Pearl, John C.
Smith, Michael D.
Conrath, Barney J.
Haberle, Robert M.
spellingShingle Zhang, Kate Q.
Ingersoll, Andrew P.
Kass, David M.
Pearl, John C.
Smith, Michael D.
Conrath, Barney J.
Haberle, Robert M.
Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model
author_facet Zhang, Kate Q.
Ingersoll, Andrew P.
Kass, David M.
Pearl, John C.
Smith, Michael D.
Conrath, Barney J.
Haberle, Robert M.
author_sort Zhang, Kate Q.
title Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model
title_short Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model
title_full Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model
title_fullStr Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model
title_full_unstemmed Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model
title_sort assimilation of mars global surveyor atmospheric temperature data into a general circulation model
publisher American Geophysical Union
publishDate 2001
url https://authors.library.caltech.edu/37499/
https://authors.library.caltech.edu/37499/1/2000JE001330.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411
geographic South Pole
North Pole
geographic_facet South Pole
North Pole
genre North Pole
South pole
genre_facet North Pole
South pole
op_relation https://authors.library.caltech.edu/37499/1/2000JE001330.pdf
Zhang, Kate Q. and Ingersoll, Andrew P. and Kass, David M. and Pearl, John C. and Smith, Michael D. and Conrath, Barney J. and Haberle, Robert M. (2001) Assimilation of Mars Global Surveyor atmospheric temperature data into a general circulation model. Journal of Geophysical Research E, 106 (E12). pp. 32863-32877. ISSN 0148-0227. doi:10.1029/2000JE001330. https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411 <https://resolver.caltech.edu/CaltechAUTHORS:20130313-131349411>
op_rights other
op_doi https://doi.org/10.1029/2000JE001330
container_title Journal of Geophysical Research: Planets
container_volume 106
container_issue E12
container_start_page 32863
op_container_end_page 32877
_version_ 1766140702337531904