4. Results: dusty case   a. Feature of dust mixing up previous next
4.a.iii. Atmospheric heating profile

The following four figures show the vertical profiles of horizontal and temporal mean heating rate for potential temperature. Figure 11e and Figure 11g show the profiles of the first day and the second day of the dusty case, and Figure 11f and Figure 11h show the corresponding profiles of each component of radiative heating, respectively.

During the daytime after LT=16:00 of the first day, the profile of radiative heating varies greatly in the vertical direction of the height levels from 10 to 15 km. The main component of the radiative heating which causes this vertical variation is solar radiative heating associated with dust.

Figure 11e: Horizontal and time mean heating rates for potential temperature; profiles of the first day in the dusty case. Unit is K/day. Orange line denotes convective heating, red line denotes infrared radiative heating, blue line denotes solar radiative heating, green line denotes turbulent diffusion of potential temperature, and light purple line denotes heating due to turbulent dissipation, respectively. Lower panel shows the magnified profiles of the lower altitudes below 1 km height of upper panel. Figure 11f: Diurnal variation of horizontal and time mean radiative heating rates for potential temperature; profiles of the first day in the dusty case. Unit is K/day. Red line denotes infrared radiative heating due to CO2, purple line denotes infrared radiative heating due to dust, blue line denotes near infrared radiative heating due to CO2, and light blue line denotes solar radiative heating due to dust, respectively. Lower panel shows the magnified profiles of the lower altitudes below 1 km height of upper panel.
Figure 11g: Horizontal and time mean heating rates for potential temperature; profiles of the second day in the dusty case. Unit is K/day. Orange line denotes convective heating, red line denotes infrared radiative heating, blue line denotes solar radiative heating, green line denotes turbulent diffusion of potential temperature, and light purple line denotes heating due to turbulent dissipation, respectively. Lower panel shows the magnified profiles of the lower altitudes below 1 km height of upper panel. Figure 11h: Diurnal variation of horizontal and time mean radiative heating rates for potential temperature; profiles of the second day in the dusty case. Unit is K/day. Red line denotes infrared radiative heating due to CO2, purple line denotes infrared radiative heating due to dust, blue line denotes near infrared radiative heating due to CO2, and light blue line denotes solar radiative heating due to dust, respectively. Lower panel shows the magnified profiles of the lower altitudes below 1 km height of upper panel.


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