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An observational and numerical modeling study of the evolving convective boundary layer and orographic circulation around the Santa Catalina Mountains in Arizona

Posted on:2010-03-15Degree:Ph.DType:Dissertation
University:University of WyomingCandidate:Demko, J. CoryFull Text:PDF
GTID:1440390002486529Subject:Meteorology
Abstract/Summary:
This research will show dynamical processes involved in convective, daytime flow behavior and subsequent moist convective development around an isolated, heated mountain. The observational component shows aircraft and surface measurements of mass and moisture transport in the boundary-layer towards the Santa Catalina Mountains (CM) in Arizona, 20-30 km in diameter, during the North American monsoon, on days with weak winds and cumulus congestus to cumulonimbus development over the mountain. Flights in the boundary-layer around the mountain and surface station data indicate that mountain-scale anabatic surface wind generally develops shortly after sunrise, peaking at ∼1 m s-1 in strength close to solar noon. There is some evidence for a toroidal heat-island circulation, with divergence in the upper boundary layer. The aircraft data and mainly the diurnal surface temperature and pressure patterns confirm that this circulation is driven by surface heating over the mountain. Three case studies suggest that growth spurts of orographic cumulus and cumulonimbus are not preceded by enhanced mountain-scale mass convergence near the surface, and that the decay of orographic deep convection is associated with divergence around the mountain.;The daytime evolution of the thermally-forced boundary-layer (BL) circulation over the CM is examined by means of numerical simulations validated with data collected in the Cumulus Photogrammetric, In situ and Doppler Observations (CuPIDO) field campaign. Three cases are presented, one remains cloud-free in the simulations, the second produces orographic convection just deep enough to yield a trace of precipitation, and the third produces numerous cumulonimbi (Cbs) over the CM. The Weather, Research and Forecasting v.3 simulations, at a resolution of 1 km, compare well with CuPIDO observations.;The simulations reveal a solenoidal circulation mostly contained within the convective BL, but this circulation and especially its upper-level return flow branch are not immediately apparent since they are overwhelmed by BL thermals. A warm anomaly forms over the high terrain during the day, but it is rather shallow and does not extend over the depth of the convective BL, which bulges over the mountain. Low-level mountain-scale convergence (MSC), driven by an anabatic pressure gradient, deepens during the day. Even relatively shallow and relatively small cumulus convection can temporarily disrupt the surface MSC by cloud shading and convective downdraft dynamics. Deeper and more widespread convection can shut down the MSC, and new convection tends to develop where outflow boundaries converge with each other or with the terrain.
Keywords/Search Tags:Convective, Circulation, Mountain, Orographic, MSC, Convection
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