4. Results: dusty case   a. Feature of dust mixing up previous next
4.a.i. Horizontal mean dust mixing ratio

Figure 11a shows the vertical profile of horizontal mean dust mixing ratio of the first and the second days. As a result of dust injection and mixing of the first day, a region with a large vertical gradient of dust mixing ratio forms at the altitudes of from 11 km to 13 km. On the second day, dust, which has reached the bottom of the stratosphere, is transported slowly into the higher altitudes.

The vertical profile of horizontal mean dust mixing ratio does not change greatly after the 4th day (Figure 11b). Horizontal mean dust mixing ratio in the convection layer is vertically uniform and slightly increasing as the depth of 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 every 1 hour from LT = 13:00 to 18:00 on the first day (left panel), and plotted every 2 hours from LT = 8:00 to 18:00 on the second day (right panel).

Figure 11b: Vertical profile of horizontal mean dust mixing ratio at LT = 16:00 from the first day to the 6th day.


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