A case study of the evolution of a Kelvin-Helmholtz wave and turbulence in noctilucent clouds

Details A case study of the evolution of a Kelvin-Helmholtz wave and turbulence in noctilucent clouds A case study of the evolution of a Kelvin-Helmholtz wave and turbulence in noctilucent clouds

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jastp..72.1129d&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 72, Issue 14-15, p. 1129-1138.

Physics

2

Scientific paper

Bright and extensive noctilucent clouds (NLC) were observed in Århus (Denmark) on 3/4 July of 2008 with an automatic digital camera taking images every minute. This event was unique in the sense that bright NLC were seen at high elevation angles (more than 30°) that allowed observing the evolution of a Kelvin-Helmholtz (KH) wave, resulted in well-developed turbulence. In particular, coherent vortex structures of a horseshoe-shaped form were observed for the first time in noctilucent clouds. The turbulent diffusion coefficient and turbulent energy dissipation rate around the mesopause are estimated in the range 162-667 m2/s and 300-1235 mW/kg, respectively, representing a case of strong neutral air turbulence in noctilucent clouds. Turbulent structures were observed to be in the vicinity of breaking small-scale gravity waves that seems to be responsible for a high level of turbulence. At the same time, it has been demonstrated that it is of importance to take into account non-turbulent process such as the gravity wave motion that is always present in NLC layers. Unless non-turbulent process is taken into account, this certainly leads to overestimating of the value of the turbulent diffusion coefficient. More accurate characteristics of turbulence in NLC can be obtained by analyzing a sequence of high-resolution images with a high frame-rate high-resolution digital camera.

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