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5. Discussion

Based on the results of our numerical simulations presented so far, we now discuss the following issues. Because the Viking Lander 1 observed wind and temperature at a height of 1.6 m, it may be informative to compare its results with data obtained at the lowest level of our numerical model (approximately 1.5 m). Our numerical simulations show that surface wind associated with the kilometer-size thermal convection of the dust-free case can lift dust from the surface. Therefore, we suggest that it is necessary to incorporate the effect of kilometer-size thermal convection into Martian GCMs in order to better simulate the weather conditions of Mars, i.e., the emergence of dust storms.

  1. Comparison with Observation Results
  2. Treatment of Convection in a GCM


A Numerical Simulation of Thermal Convection in the Martian Lower Atmosphere with a Two-Dimensional Anelastic Model
Odaka, Nakajima, Ishiwatari, Hayashi,   Nagare Multimedia 2001
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