Abstract
A number of puzzling features of the skewness of the vertical velocity field, Sw(z), are found in observations and large-eddy simulations (LES) of the buoyancy-driven planetary boundary layer (PBL). For example, observations of Sw(z) in cases where the air is heated from below indicate that Sw(z)>0 and remains relatively constant for z≥0.3zi, whereas all large-eddy simulations of these cases show a continuing increase of Sw(z) with height. In cases where the air is both heated from below and cooled from above, as in some of the stratus-topped PBL cases Sw is positive in the upper layer and negative in the lower layer. In the present paper we examine the skewness distribution from direct numerical simulations of several simple archetypes of buoyancy-driven turbulent flow. -from Authors
| Original language | English |
|---|---|
| Pages (from-to) | 1149-1162 |
| Number of pages | 14 |
| Journal | Journal of the Atmospheric Sciences |
| Volume | 47 |
| Issue number | 9 |
| DOIs | |
| State | Published - 1990 |
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