Local mean state changes due to gravity wave breaking modulated by the diurnal tide

During gravity wave breaking, heating rates are determined by wave advectio n, turbulent diffusion, and turbulence dissipative heating. A series of num erical experiments show that the total heating rates can be larg (similar t o +/-10 Kh(-1)) and can cause large local temperature changes. The wave adv ection causes dynamical cooling in most of the wave breaking region, consis tent with previous studies. Nonuniform vertical turbulent diffusion causes strong transient heating in the lower part of the wave breaking region and cooling above. The dissipative heating rate is relatively small compared wi th those due to the dynamical cooling and turbulent diffusion. In these num erical experiments, zonal wind and temperature perturbations of the diurnal tide and the zonal mean zonal wind and temperature compose the background state for the computation. This is used to examine the idea that temperatur e inversions, often observed in the mesosphere, are related to the gravity wave and tidal wave interactions. The simulation results show that the larg e temperature changes in this process can form temperature inversion layers that progress downward with a speed similar to that of a diurnal tide phas e speed, which clearly suggests the tidal modulation of the gravity wave an d mean flow interactions. Such a process is dependent on season and latitud e, because the background state stability varies with season and latitude. The development of the temperature inversion is also affected by the gravit y wave characteristics. It is also shown that the local mean wind, wind she ar, and chemical species can undergo large changes accompanying the tempera ture inversion.