1) The RL may exhibit significant turbulence reaching intensities comparable to those in the underlying stable boundary layer. Such observations alter the current picture of the RL from that of a quiescent region with predominantly laminar flow to one of a dynamic region with rapidly changing small-scaled variations of turbulence.
We hypothesize that enhanced turbulence is related to upward-propagating atmospheric gravity waves generated by stably stratified flow over the low-relief terrain. During one night a presence of critical layers in the RL, generated by wind turning with height, caused deposition of upward-propagating wave momentum resulting in generation of intermittent turbulence.
2) The well-accepted concept of turbulence generation below a critical value of the gradient Richardson number (Ri) is, in fact, scale dependent: Ri values typically decrease with decreasing vertical scale size, so that critical Ri values (»0.25) occur at vertical scales of only a few tens of meters. This poses a problem for incorporating experimentally determined Ri values in model closures on models that have poor vertical resolution.
3) There appears to be two distinct turbulence regimes' in the RL: a very weak but ever-present background turbulence level with minimal temporal and spatial structure, and a more intense, intermittent regime during which turbulent intensity levels can approach nighttime turbulent intensities near the surface.