First detection of wave interactions in the middle atmosphere of Mars

被引：7

作者：

Moudden, Y. ^{[1
]}

Forbes, J. M. ^{[1
]}

机构：

[1] Univ Colorado, Dept Aerosp Engn Sci, Boulder, CO 80309 USA

来源：

GEOPHYSICAL RESEARCH LETTERS | 2011年 / 38卷

关键词：

GENERAL-CIRCULATION MODEL; SEMIDIURNAL TIDES; TIDAL VARIABILITY; PLANETARY-WAVES; THERMOSPHERE; MESOSPHERE; TEMPERATURE;

D O I：

10.1029/2010GL045592

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Planetary wave-tide interactions are known to exist in Earth's atmosphere and to account for some of its diurnal variability, or put another way, for variations in its diurnal cycle over time scales from days to weeks. In this study, using an elaborate arrangement of temperature profiles at a single local time from MRO/Mars Climate Sounder, we show that planetary wave-tide interactions also occur in the middle atmosphere of Mars. These interactions excite secondary waves that amplify on average with altitude and appear to be an important source of tidal and longitudinal variability. Citation: Moudden, Y., and J. M. Forbes (2011), First detection of wave interactions in the middle atmosphere of Mars, Geophys. Res. Lett., 38, L04202, doi: 10.1029/2010GL045592.

引用

页数：5

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