3. Results: dust-free case up previous next
3.d. Intensity of the convection (1)

Figure 7: Vertical profile of horizontal mean potential temperature below 1 km hight at LT=14:00 in dust-free case.


The wind velocity associated with the km-size convection can be estimated by using the equation (1). In this section, we consider how the potential temperature deviation of ascending convective plume () can be estimated.

The convective plume associated with the km-size thermal convection is generated by convective instability in the thermal boundary layer (see Figure 4 (upper left)). Therefore, it is considered that the potential temperature deviation of convective plume is corresponds to potential temperature difference in the thermal boundary layer. Figure 7 shows the vertical profile of horizontal mean potential temperature below 1 km hight in daytime. The thermal boundary layer where the vertical gradient of horizontal mean potential temperature is negative can be divided two regions. One is "conduction layer" which is located below about 50 m hight. In this region, the heating due to turbulent diffusion is comparable to radiative heating (Figure 3d) and the horizontal mean potential temperature increases linearly toward the grand surface. The other is "transition layer" which is located between the conduction layer and about 400 m hight where the vertical gradient of horizontal mean potential temperature is relatively moderate.


A numerical simulation of thermal convection in the Martian lower atmosphere.
Odaka, Nakajima, Ishiwatari, Hayashi,   Nagare Multimedia 2001
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