Diurnal Kelvin wave in the atmosphere of Mars: Towards an understanding of 'stationary' density structures observed by the MGS accelerometer

Geophysical Research Letters

Volumn 27, Issue 21, 2000, Pages 3563-3566

  Forbes, Jeffrey M ^a   Hagan, Maura E ^b  

^a UCB 450   (United States)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

KELVIN WAVE; MARS; PLANETARY ATMOSPHERE;

ACCELEROMETERS; OSCILLATIONS; PERTURBATION TECHNIQUES;

DIURNAL KELVIN WAVES;

GEOPHYSICS;

EID: 0034352528     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL011850     Document Type: Article

References (13)

1. Thermal tides and stationary waves on Mars as revealed by Mars Global Surveyor thermal emission spectrometer
2. Possible effects of breaking gravity waves on the circulation of the middle atmosphere of Mars
3. The Mars thermosphere, II, general circulation with coupled dynamics and composition
4. Comparative terrestrial planet thermospheres 3. Solar cycle variation of global structure and winds at solstices
5. Influence of planetary-scale topography on the diurnal thermal tide during the 1971 Martian dust storm
6. Mars atmospheric dynamics as simulated by the NASA-Ames general circulation model I. The zonal-mean circulation
7. GSWM-98: Results for migrating solar tides
8. Forced stationary planetary waves in Mars winter atmosphere
9. An interpretation of Martian thermospheric waves based on analysis of a general circulation model
10. The structure of the upper atmosphere of Mars: In situ accelerometer measurements from Mars Global Surveyor
11. Effects of mean winds and horizontal temperature gradients on solar and lunar semidiurnal tides in the atmosphere
12. Comprehensive simulation of thermal tides in the Martian atmosphere
13. Free and forced modes in the Martian atmosphere