3. Results: Dust-Free Case up previous next
3.d. Intensity of Convection (1)

Figure 7: Vertical profile of horizontal mean potential temperature below the height of 1 km at 14:00 LT for the dust-free case.


As shown in Equation (1), wind velocity associated with convection is given by convection layer thickness and the temperature deviation of plumes. In this section, we consider how the potential temperature deviation of convective plumes can be estimated.

Referring to the features of convective plume generation, which can be interpreted from Figure 4 (upper left), it can be regarded that plumes are produced by thermal instability of the thermal boundary layer. This suggests that potential temperature deviation of a convective plume is roughly equal to that of the thermal boundary layer. Figure 7 is a magnified view of Figure. 3a (right) of the plot for potential temperature below 1 km. Careful observation of the profile indicates that the thermal boundary layer can be further divided into two regions according to the magnitude of the vertical gradient of potential temperature. One such region is the layer below the 50 m level, where the vertical gradient of potential temperature is quite large (conduction layer), and the other region is the layer between 50 m and approximately 400 m, where the vertical gradient of potential temperature is relatively moderate (transition layer).


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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