Second, we re-examine data from the Hudson Valley Ambient Meteorology Study (HVAMS) during September and October 2003. The HVAMS surface network included nine integrated surface flux system stations from the National Science Foundation's Lower Atmosphere Observing Facilities and five conventional meteorological stations encompassing the Hudson Valley for 100 km from Albany southward. Additional Albany radiosondes along with data from radar wind profilers at Schenectady and Kingston airports provided additional wind information through the depth of the planetary boundary layer. At dawn and dusk, an the University of Wyoming's King Air made detailed soundings of the stable boundary layer by making close approaches' at small airports.
After very briefly recounting our efforts of a decade ago, analysis proceeds by estimating the momentum balance in the afternoon convective boundary layer (CBL); we use the suite of HVAMS observations to infer vetrical momentum exchanges in the decaying CBL seen during the early-evening transition. After this transition, the wind at ≈150 m (the top of the eventual stable boundary layer SBL) often presents the direction earlier seen above zi ≈ 1200m. We re-examine the idea that decaying turbulence in the CBL, even while weaking rapidly, may still be sufficient to mix momentum and other scalar quantities down to the top of the ensuing SBL, the hodograph indicating the remnant CBL winds spiraling toward geostrophic balance. During this period, and after the establishment of the shallow (100-200 m) SBL, we estimate momentum balances using a simple bulk model that includes a tilted mixed' layer to counter the Coriolis acceleration. This model treats the effects of the cold pool' in the valley and its modulation of the nocturnal along-valley jet'.