Thermal tides in the Martian middle atmosphere as seen by the Mars Climate Sounder
Article first published online: 19 MAR 2009
DOI: 10.1029/2008JE003285
Copyright 2009 by the American Geophysical Union.
Additional Information
How to Cite
, et al. (2009), Thermal tides in the Martian middle atmosphere as seen by the Mars Climate Sounder, J. Geophys. Res., 114, E03005, doi:10.1029/2008JE003285.
Publication History
- Issue published online: 19 MAR 2009
- Article first published online: 19 MAR 2009
- Manuscript Accepted: 6 JAN 2009
- Manuscript Revised: 23 DEC 2008
- Manuscript Received: 23 OCT 2008
Keywords:
- MCS;
- Mars;
- tides
[1] The first systematic observations of the middle atmosphere of Mars (35–80km) with the Mars Climate Sounder (MCS) show dramatic patterns of diurnal thermal variation, evident in retrievals of temperature and water ice opacity. At the time of writing, the data set of MCS limb retrievals is sufficient for spectral analysis within a limited range of latitudes and seasons. This analysis shows that these thermal variations are almost exclusively associated with a diurnal thermal tide. Using a Martian general circulation model to extend our analysis, we show that the diurnal thermal tide dominates these patterns for all latitudes and all seasons.

2169-9100/asset/olbannerleft.jpg?v=1&s=214fb4f4c0e1408d296d9924aa555e5183c2161e)
2169-9100/asset/olbannerright.jpg?v=1&s=12881868082fda5139cf3855ea7f914a8a568e10)
2169-9100/asset/cover.gif?v=1&s=3e903c82115de9ec5800b65c840dcff674e71214)