4. Results: Dusty Case   c. Circulation Structure of Convection up previous next
4.c.i. Intensity of Convection

The depth of conduction layer and potential temperature difference in the layer can be estimated by using equation (2) and (4). Total amount of CO2 infrared radiative heating and sensible heat flux in day time is about 20 W m-2 which is responsible for driving convection (see Figure 12f). The value of turbulent diffusion coefficient is almost same as that in dust-free case (∼ 15 m2 sec-1, see Figure 12b). Substituting these values in Equation (2), the value of vertical gradient of potential temperature in conduction layer is -0.1 K m-1. It is consistent with the results of numerical simulation (Figure 14). In this case, Equation (4) which gives is as follows.


We obtain ∼ 60 m, ∼ 6 K (those of numerical simulation results are 50 m and 3 K, respectively). As compared to estimation in dust-free case, the value of is similar and is 2 K smaller.

The potential temperature deviation of a convective plume is estimated by using Equation (5). According to Figure 14, the depth of conduction layer is about 40 m, and temperature difference in the layer is 3 K. The depth of convection layer is 5000 m. The value of turbulent diffusion coefficient is almost same as that in dust-free case (∼ 15 m2 sec-1). Estimated value of potential temperature deviation of a convective plume by using Equation (5) is as follows.


Figure 14: Vertical profile of horizontal mean potential temperature below the height of 1 km at 14:00 LT on day 6 for the dusty case.


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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