Early descriptive models of mountain-valley circulations indicated that the mountain flow (i.e., the along-valley axis component out of the valley) is a true three-dimensional phenomenon. According to these descriptions, at night shallow-down slope flows on the valley sidewalls directly driven by temperature deficits near the surface produce a pooling of cool air in the valley. This deep pool of cool air in the valley compared with a much shallower surface inversion over the plains produces a secondary flow (the mountain flow)) out of the valley driven by a deep hydrostatic pressure gradient. It is the purpose of this investigation to numerically simulate the above-mentioned secondary circulation using a three-dimensional numerical model. -from Authors
CITATION STYLE
McNider, R. T., & Pielke, R. A. (1984). Numerical simulation of slope and mountain flows. Journal of Climate & Applied Meteorology, 23(10), 1441–1453. https://doi.org/10.1175/0733-3021-23.10.1441
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