4. Results: dusty case   b. Horizontal mean fields up previous next
4.b.iii. Atmospheric heating profile

Figure 12d shows the horizontal and time mean vertical profiles of atmospheric heating rate for potential temperature of the 6th day in the dusty case. The major component of radiative heating above 2 km height during daytime is dust absorption of solar radiation. The magnitude of convective heating and the depth of convectively cooling layer near the surface are almost the same as those of the dust-free case. During the nighttime, the entire region of the calculated domain is subject to infrared radiative cooling due to CO2 and dust.

Each component of the heating profile shown in Figure 12d is presented in Figure 12e. The profile of near infrared radiative heating due to CO2 is vertically uniform over the calculated domain. In the convective layer, where dust mixing ratio is uniform, the profile of radiative heating due to dust is vertically uniform. These two components tend to suppress thermal convection, since they warm the convection layer uniformly in the vertical direction. The radiative component which contributes dominantly to driving thermal convection is the infrared heating due to CO2 which has a vertical profile concentrated near the surface.

Figure 12d: Diurnal change of the horizontal and time mean vertical profiles of atmospheric heating rate (K/day) for potential temperature in the 6th day of the dusty case. 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 12e: Diurnal change of the horizontal and time mean vertical profiles of radiative heating rate (K/day) in the 6th day of the dusty case. Red line and purple line denote infrared radiative heating due to CO2 and that of dust, blue line and light blue line denote solar radiative heating due to CO2 and that of dust.


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