4. Results: Dusty Case   a. Features of Dust Mixing up previous next
4.a.iii. Atmospheric heating profile (for days 1 and 2 of the dusty case)

The following four figures show the vertical profiles of the horizontal and temporal mean heating rates for potential temperature. Figure 11e and Figure 11g show such profiles for days 1 and 2 of the dusty case, and Figure 11f and Figure 11h show profiles for each component of radiative heating.

During the daytime after 16:00 LT on day 1, the radiative heating profile varies greatly in the vertical direction from 10 to 15 km. The main component of radiative heating, which causes this vertical variation, is the solar radiative heating associated with dust.

Figure 11e: Horizontal and temporal mean heating rates for potential temperature on day 1 of 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 the light purple line denotes heating due to turbulent dissipation. The lower panel shows a magnified view of the profiles at altitudes below 1 km. Figure 11f: Diurnal variation of horizontal and temporal mean radiative heating rates for potential temperature on day 1 of 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 the light blue line denotes solar radiative heating due to dust. The lower panel shows a magnified view of the profiles at altitudes below 1 km.
Figure 11g: Horizontal and temporal mean heating rates for potential temperature on day 2 of 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 the light purple line denotes heating due to turbulent dissipation. The lower panel shows a magnified view of the profiles at altitudes below 1 km. Figure 11h: Diurnal variation of horizontal and temporal mean radiative heating rates for potential temperature on day 2 of 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 the light blue line denotes solar radiative heating due to dust. The lower panel shows a magnified view of the profiles at altitudes below 1 km.


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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