4. Results: Dusty Case   a. Features of Dust Mixing up previous next
4.a.i. Horizontal mean dust mixing ratio

Figure 11a shows vertical profiles of horizontal mean dust mixing ratio for days 1 and 2. On day 1, as a result of dust injection and mixing, there is a large vertical gradient of dust mixing ratio from 10 to 13 km. By day 2, dust reaches the bottom of the stratosphere and is transported into higher altitudes. The vertical profile of horizontal mean dust mixing ratio does not significantly vary after day 4 (Figure 11b). Horizontal mean dust mixing ratio in the convection layer is vertically uniform and slightly increases as depth of the convection layer decreases. This indicates that the system is in a quasi equilibrium state where the total amount of dust in the atmosphere does not change significantly (Figure 9); the amount of dust injection is roughly in balance with the amount of dust sedimentation. In the region above the convection layer, dust mixing ratio slightly decreases as dust sedimentation progresses slowly.

Figure 11a: Vertical profiles of horizontal mean dust mixing ratio plotted for (left panel) every 1 hour from 13:00 to 18:00 LT on day 1, and (right panel) every 2 hours from 8:00 to 18:00 LT on day 2.

Figure 11b: Vertical profile of horizontal mean dust mixing ratio at 16:00 LT for days 1 through 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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