Infrared radiative cooling in the mesosphere and lower thermosphere

Abstract

This paper discusses the current status of calculating infrared cooling by CO 2 in the mesosphere and lower thermosphere. It is desirable to have fast but accurate procedures for use in dynamic models. The most difficult region is from 70 to 90 km, where cooling rates are strongly influenced or, in the case of the summer mesopause region, dominated by the absorption of radiation emitted by underlying layers, with the hot bands and isotopic bands playing a significant role. A three-energy-level model is derived for the excited population levels of a CO 2 molecule. Vibrational-vibrational coupling between isotopes is also included as significant. Results from model calculations for cooling rates and NLTE source functions are presented. Global average infrared cooling rates appear to be in reasonable balance with solar heating rates, considering the uncertainties in calculating both these terms. Radiative cooling rates by CO 2 above 100 km are strongly dependent on atomic oxygen concentrations and on the rate of energy exchange between atomic oxygen and CO 2. Likewise, NO cooling, which is important above 120 km, is proportional to atomic oxygen concentrations. Since CO 2, NO and O concentrations can all vary with motions, these dependencies suggest interesting feedbacks to atmospheric dynamics.