The “Mad Sea” Phenomenon in the Strait of SicilySource: Journal of Physical Oceanography:;1999:;Volume( 029 ):;issue: 009::page 2210Author:Candela, Julio
,
Mazzola, Salvatore
,
Sammari, Chérif
,
Limeburner, Richard
,
Lozano, Carlos J.
,
Patti, Bernardo
,
Bonanno, Angelo
DOI: 10.1175/1520-0485(1999)029<2210:TMSPIT>2.0.CO;2Publisher: American Meteorological Society
Abstract: Sea 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.
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contributor author | Candela, Julio | |
contributor author | Mazzola, Salvatore | |
contributor author | Sammari, Chérif | |
contributor author | Limeburner, Richard | |
contributor author | Lozano, Carlos J. | |
contributor author | Patti, Bernardo | |
contributor author | Bonanno, Angelo | |
date accessioned | 2017-06-09T14:53:39Z | |
date available | 2017-06-09T14:53:39Z | |
date copyright | 1999/09/01 | |
date issued | 1999 | |
identifier issn | 0022-3670 | |
identifier other | ams-29108.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4166299 | |
description abstract | Sea 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. | |
publisher | American Meteorological Society | |
title | The “Mad Sea” Phenomenon in the Strait of Sicily | |
type | Journal Paper | |
journal volume | 29 | |
journal issue | 9 | |
journal title | Journal of Physical Oceanography | |
identifier doi | 10.1175/1520-0485(1999)029<2210:TMSPIT>2.0.CO;2 | |
journal fristpage | 2210 | |
journal lastpage | 2231 | |
tree | Journal of Physical Oceanography:;1999:;Volume( 029 ):;issue: 009 | |
contenttype | Fulltext |