Convective instability in the martian middle atmosphere
Dry convective instabilities in Mars’s middle atmosphere are detected and mapped using temperature retrievals from Mars Climate Sounder observations spanning 1.5 martian years. The instabilities are moderately frequent in the winter extratropics. The frequency and strength of middle atmospheric conv...
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Published in | Icarus (New York, N.Y. 1962) Vol. 208; no. 2; pp. 574 - 589 |
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01.08.2010
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Abstract | Dry convective instabilities in Mars’s middle atmosphere are detected and mapped using temperature retrievals from Mars Climate Sounder observations spanning 1.5 martian years. The instabilities are moderately frequent in the winter extratropics. The frequency and strength of middle atmospheric convective instability in the northern extratropics is significantly higher in MY 28 than in MY 29. This may have coupled with changes to the northern hemisphere mid-latitude and tropical middle atmospheric temperatures and contributed to the development of the 2007 global dust storm. We interpret these instabilities to be the result of gravity waves saturating within regions of low stability created by the thermal tides. Gravity wave saturation in the winter extratropics has been proposed to provide the momentum lacking in general circulation models to produce the strong dynamically-maintained temperature maximum at 1–2
Pa over the winter pole, so these observations could be a partial control on modeling experiments. |
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AbstractList | Dry convective instabilities in Mars's middle atmosphere are detected and mapped using temperature retrievals from Mars Climate Sounder observations spanning 1.5 martian years. The instabilities are moderately frequent in the winter extratropics. The frequency and strength of middle atmospheric convective instability in the northern extratropics is significantly higher in MY 28 than in MY 29. This may have coupled with changes to the northern hemisphere mid-latitude and tropical middle atmospheric temperatures and contributed to the development of the 2007 global dust storm. We interpret these instabilities to be the result of gravity waves saturating within regions of low stability created by the thermal tides. Gravity wave saturation in the winter extratropics has been proposed to provide the momentum lacking in general circulation models to produce the strong dynamically-maintained temperature maximum at 1-2Pa over the winter pole, so these observations could be a partial control on modeling experiments. Dry convective instabilities in Mars’s middle atmosphere are detected and mapped using temperature retrievals from Mars Climate Sounder observations spanning 1.5 martian years. The instabilities are moderately frequent in the winter extratropics. The frequency and strength of middle atmospheric convective instability in the northern extratropics is significantly higher in MY 28 than in MY 29. This may have coupled with changes to the northern hemisphere mid-latitude and tropical middle atmospheric temperatures and contributed to the development of the 2007 global dust storm. We interpret these instabilities to be the result of gravity waves saturating within regions of low stability created by the thermal tides. Gravity wave saturation in the winter extratropics has been proposed to provide the momentum lacking in general circulation models to produce the strong dynamically-maintained temperature maximum at 1–2 Pa over the winter pole, so these observations could be a partial control on modeling experiments. |
Author | Lawson, W.G. Schofield, J.T. Kleinböhl, A. Abdou, W.A. Heavens, N.G. Kass, D.M. Shirley, J.H. McCleese, D.J. Richardson, M.I. Lee, C. |
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Keywords | Atmospheres, Structure Atmospheres, Dynamics Mars, Atmosphere Meteorology Convective instabilities Atmospheres Northern hemisphere Saturation Atmospheric instability Mars Atmospheric temperature Dust storm Dynamics Atmosphere Models Modelling Solar system Structure Gravity waves |
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Snippet | Dry convective instabilities in Mars’s middle atmosphere are detected and mapped using temperature retrievals from Mars Climate Sounder observations spanning... Dry convective instabilities in Mars's middle atmosphere are detected and mapped using temperature retrievals from Mars Climate Sounder observations spanning... |
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SubjectTerms | Astronomy Atmospheres, Dynamics Atmospheres, Structure Atmospherics Circulation Earth, ocean, space Exact sciences and technology Gravity waves Instability Mars Mars, Atmosphere Meteorology Middle atmosphere Retrieval Solar system Stability Winter |
Title | Convective instability in the martian middle atmosphere |
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