Physics
Scientific paper
Apr 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jgr...103.8587b&link_type=abstract
Journal of Geophysical Research, Volume 103, Issue E4, p. 8587-8602
Physics
9
Planetology: Solid Surface Planets: Atmospheres-Structure And Dynamics, Meteorology And Atmospheric Dynamics: Waves And Tides, Atmospheric Composition And Structure: Planetary Atmospheres, Meteorology And Atmospheric Dynamics: Planetary Meteorology
Scientific paper
Simulations of Mars' atmospheric tides with the NASA-Ames Mars general circulation model are presented and analyzed. In an annual simulation, diurnal and semidiurnal tides in the model's surface pressure field are shown to compare well with tides observed by the Viking landers throughout the Mars year. Focused simulations of global dust storms during the northern winter season show a semidiurnal tide that responds very strongly to the increased dust load during the storms, again matching well with observations. Analysis of the structure and behavior of this tide during global storms verifies that it is dominated by the gravest symmetric Hough mode (H22), as has been noted previously. However, it is shown here that additional symmetric and asymmetric modes play an important role in accounting for the structure of the tide and its variation during the dust storms. The phase advance observed between the Viking lander sites (earlier semidiurnal phase at the higher-latitude site) is explained by the presence of these higher-order modes. Finally, decomposition of the semidiurnal tide during a global dust storm into its component Hough modes shows that the amplitude of the H22 mode mirrors changes in the observed overhead visible dust opacity, while variations in higher-order modes are indicative of the zonal (and, possibly, longitudinal) distribution of airborne dust.
Bridger Alison F. C.
Murphy James R.
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