Solar heating by the near-IR CO2 bands in the mesosphere

Physics

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Atmospheric Composition And Structure: Middle Atmosphere-Energy Deposition, Global Change: Atmosphere (0315, 0325), Meteorology And Atmospheric Dynamics: General Circulation, Meteorology And Atmospheric Dynamics: Numerical Modeling And Data Assimilation, Meteorology And Atmospheric Dynamics: Radiative Processes

Scientific paper

Absorption of solar energy by the near-infrared (NIR) CO2 bands provides an important source of heating in the mesosphere. At 60-85 km, this source exceeds 1 K day-1 and contributes up to 30% of the total solar heating. Calculation of the solar heating in the NIR CO2 bands requires consideration of complex non-local thermodynamic equilibrium (non-LTE) processes. The small energy effect, narrow region of importance, and the necessity to consider non-LTE effects, have accounted for the absence of an adequate parameterization for the NIR CO2 bands. Recently a parameterization has been developed and implemented into the Canadian Middle Atmosphere Model. Numerical experiments with this model have shown that inclusion of the NIR CO2 heating results in a significant warming of up to 8 K in the mesosphere for the current CO2 amount but does not significantly change the model thermal response induced by the doubling of CO2.

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