4. Results: Dusty Case up previous next
4.b. Diurnal Change of Horizontal Mean Field

Figure 12a shows the diurnal variation of the vertical profiles of horizontal mean temperature and potential temperature for day 6, when the amount of atmospheric dust reaches an almost equilibrium state. The profiles of horizontal mean temperature and potential temperature show fairly regular diurnal change, while that of atmospheric dust shows little change (Figure 11b). The depth of the convection layer during daytime is about 5 km, which is roughly half that for the dust-free case (Figure 3e). One reason for this decrease in convection layer depth is an increase in stratospheric temperature, which is due to radiative heating caused by dust absorption of solar radiation (Figure 12e).

Figure 12a: Vertical profiles of horizontal mean temperature (left panel) and potential temperature (right panel) for the dusty case. Profiles are every 4 hours beginning at 8:00 LT on day 6.


The other results of diurnal changes in mean fields on day 6.


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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