4. Results: Dusty Case   b. Diurnal Changes of Horizontal Mean Fields up previous next
4.b.iv. Heat budget of the atmosphere and surface

Figure 12f shows the diurnal changes of the horizontal mean heat budgets at the ground surface and atmosphere for the dusty case. In each panel, the amount of net heating is almost equal to that of cooling.

  • The amount of net solar radiative heating in the ground layer is smaller than that of the dust-free case (Figure 3e). This is caused by the absorption of solar radiation due to atmospheric dust.
  • The amount of net infrared radiative heating due to CO2 and sensible heating, which are the dominant contributors in driving convection, are smaller than those of the dust-free case (Figure 3e). The sum of these differences reaches 20 W m-2 during the daytime.
  • For the atmosphere, the dominant component of net solar heating is the absorption of solar radiation due to dust. The amount of this absorption is similar to the decrease of net solar radiative flux in the ground layer for the dust-free case.

The reason for the decrease in CO2 infrared heating is a decrease in ground temperature. This decrease is approximately on the same order of magnitude of the decrease of the 15 μm-band infrared emission from the ground surface (i.e., several W m-2). Sensible heating decreases due to a decrease in the wind velocity associated with convection.

Figure 12f: Diurnal changes of the horizontal mean heat budgets for day 6 of the dusty case. Unit of the vertical axis is W m-2. (Left panel) Heat budget for the ground layer. Blue line shows net solar radiative flux ( ), red line shows net infrared radiative flux (, green line shows sensible heat flux (), and the orange line shows the total flux. Positive sign indicate heating of the ground surface. (Right panel) Heat budget for the atmosphere. Blue line shows net solar radiative heating (), red line shows net infrared radiative heating (), green line shows sensible heating (), purple line shows heating due to turbulent dissipation, and the orange line shows the sum of net infrared radiative heating and sensible heating. Positive sign indicate heating of the atmosphere.


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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