An examination of structure and parameterization of turbulence in the stably-stratified atmospheric boundary layer

Graduation date: 1988The very stable boundary layer is a region of the atmosphere typified by large\ud vertical gradients of temperature and momentum. Analysis of very stable atmospheric\ud flows is complicated by the presence of nonlinear interactions among gravity waves, shear-driven\ud overturning circulations, two-dimensional vortical modes and intermittent turbulence\ud in various stages of development. This study examines the horizontal structure of a very\ud stable atmospheric boundary layer, using data obtained primarily from terrain-following\ud aircraft flights over central Oklahoma.\ud Several diagnostic procedures are applied to the aircraft data, including classical and\ud rotary spectral analysis, principal component analysis, and structure functions. Coherent\ud structures with sharp boundaries are examined with a new conditional sampling technique\ud which requires little a priori specification of sampling criteria. Because the flows involve\ud sharp boundaries, spectral techniques do not provide as much useful information as other\ud more localized procedures. The edges of the coherent structures are regions of significant\ud vertical heat transport, a feature not often emphasized in studies of gravity waves and\ud vortical modes in the stable boundary layer.\ud The presence of significant turbulence even for large stability has implications for\ud modelling of the very stable boundary layer. Forecasts of minimum temperature, boundary\ud layer height, inversion characteristics, and pollutant dispersal are all significantly affected\ud by turbulent mixing. Many models of the stable boundary layer artificially arrest the\ud mixing under stable conditions, resulting in, for example, overestimates of nocturnal\ud cooling. A new parameterization of the stable boundary layer is studied here by\ud incorporating it into an existing model of the planetary boundary layer. The model is then\ud run with one-dimensional sensitivity tests for an idealized atmosphere and with data from\ud Wangara day 33. A simulation over snow cover is also examined. The tests substantiate\ud the role of vertical mixing in ameliorating nocturnal cooling. An additional improvement is\ud a more realistic boundary layer height for moderate wind speeds