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contributor authorCandela, Julio
contributor authorMazzola, Salvatore
contributor authorSammari, Chérif
contributor authorLimeburner, Richard
contributor authorLozano, Carlos J.
contributor authorPatti, Bernardo
contributor authorBonanno, Angelo
date accessioned2017-06-09T14:53:39Z
date available2017-06-09T14:53:39Z
date copyright1999/09/01
date issued1999
identifier issn0022-3670
identifier otherams-29108.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4166299
description abstractSea level observations at Cape Bon, Tunisia, and Mazara del Vallo, Sicily, show that large, coherent oscillations exist across the Strait of Sicily with significant energy bands centered at periods of 35.3, 41.6, 50.6, 75.8, and 134.5 min, whose possible structure is confirmed by a numerical approximation to the gravitational barotropic normal modes with realistic topography. It is observed that these oscillations are related to the passage of synoptic weather systems over the region. An investigation on the configuration, phase velocity, and direction of approach of atmospheric disturbances over the region suggests that the oscillations in the Strait of Sicily could be forced by instabilities that develop in large-scale, low pressure fronts that propagate as pressure gravity waves with an approximate phase speed between 24 and 30 m s?1.
publisherAmerican Meteorological Society
titleThe “Mad Sea” Phenomenon in the Strait of Sicily
typeJournal Paper
journal volume29
journal issue9
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(1999)029<2210:TMSPIT>2.0.CO;2
journal fristpage2210
journal lastpage2231
treeJournal of Physical Oceanography:;1999:;Volume( 029 ):;issue: 009
contenttypeFulltext


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