TY - JOUR
T1 - Low Froude number flow past three-dimensional obstacles. Part II
T2 - upwind flow reversal zone
AU - Smolarkiewicz, P. K.
AU - Rotunno, R.
PY - 1990
Y1 - 1990
N2 - The present paper contains a continuation of our study of the flow of a density-stratified fluid past three-dimensional obstacles for Froude number ~O(1). We have excluded the effects of friction, rotation, nonuniform ambient flow, and the complexity of realistic terrain. Herein we examine the zone of flow reversal on the windward side of the obstable, which is also a characteristic feature of the low-Froude number flow. We find that flow stagnation and a tendency for flow reversal upwind of a symmetric bell-shaped obstacle is well predicted by linear inviscid gravity-wave theory. This finding stands in contrast with "horseshoe-vortex' arguments often invoked in the literature. We also perform experiments on obstacles of varying aspect ratio, β (across-stream length/along-stream length). Here the utility of the linear theory is less clear: considering cases with Fr=0.33 and β→∞, we find that for β≤1 upstream-propagating columnar modes are essentially absent, however, for β increasing beyond unity, they appear with increasing strength. -from Authors
AB - The present paper contains a continuation of our study of the flow of a density-stratified fluid past three-dimensional obstacles for Froude number ~O(1). We have excluded the effects of friction, rotation, nonuniform ambient flow, and the complexity of realistic terrain. Herein we examine the zone of flow reversal on the windward side of the obstable, which is also a characteristic feature of the low-Froude number flow. We find that flow stagnation and a tendency for flow reversal upwind of a symmetric bell-shaped obstacle is well predicted by linear inviscid gravity-wave theory. This finding stands in contrast with "horseshoe-vortex' arguments often invoked in the literature. We also perform experiments on obstacles of varying aspect ratio, β (across-stream length/along-stream length). Here the utility of the linear theory is less clear: considering cases with Fr=0.33 and β→∞, we find that for β≤1 upstream-propagating columnar modes are essentially absent, however, for β increasing beyond unity, they appear with increasing strength. -from Authors
UR - https://www.scopus.com/pages/publications/0025659381
U2 - 10.1175/1520-0469(1990)047<1498:LFNFPT>2.0.CO;2
DO - 10.1175/1520-0469(1990)047<1498:LFNFPT>2.0.CO;2
M3 - Article
AN - SCOPUS:0025659381
SN - 0022-4928
VL - 47
SP - 1498
EP - 1511
JO - Journal of the Atmospheric Sciences
JF - Journal of the Atmospheric Sciences
IS - 12
ER -