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contributor authorGallée, Hubert
contributor authorSchayes, Guy
date accessioned2017-06-09T16:09:50Z
date available2017-06-09T16:09:50Z
date copyright1994/04/01
date issued1994
identifier issn0027-0644
identifier otherams-62361.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4203244
description abstractThe spatial evolution of Antarctic katabatic winds in the area of Terra Nova Bay is examined using the three-dimensional version of the Université Catholique de Louvain-Modèle Atmosphérique Régional (UCL-MAR) mesoscale primitive equation models. The ability of the model to replicate classical linear mountain wave simulations is verified. Then, three-dimensional experiments are performed for the terrain configuration of Terra Nova (Ross Sea coastal zone) using different horizontal resolutions (5, 10, and 20 km). The model converges for resolutions lower than 10 km. Results are in qualitative agreement with available observations and previous modeling work. Strong katabatic winds are simulated with a jet over Terra Nova Bay. The model seems able to initiate the mesocyclonic activity in the Ross Sea due to the katabatic circulation.
publisherAmerican Meteorological Society
titleDevelopment of a Three-Dimensional Meso-γ Primitive Equation Model: Katabatic Winds Simulation in the Area of Terra Nova Bay, Antarctica
typeJournal Paper
journal volume122
journal issue4
journal titleMonthly Weather Review
identifier doi10.1175/1520-0493(1994)122<0671:DOATDM>2.0.CO;2
journal fristpage671
journal lastpage685
treeMonthly Weather Review:;1994:;volume( 122 ):;issue: 004
contenttypeFulltext


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