The "Mad Sea" phenomenon in the strait of Sicily

Citation
J. Candela et al., The "Mad Sea" phenomenon in the strait of Sicily, J PHYS OCEA, 29(9), 1999, pp. 2210-2231
Citations number
22
Categorie Soggetti
Aquatic Sciences","Earth Sciences
Journal title
JOURNAL OF PHYSICAL OCEANOGRAPHY
ISSN journal
00223670 → ACNP
Volume
29
Issue
9
Year of publication
1999
Pages
2210 - 2231
Database
ISI
SICI code
0022-3670(199909)29:9<2210:T"SPIT>2.0.ZU;2-#
Abstract
Sea level observations at Cape Bon, Tunisia, and Mazara del Vallo, Sicily, show that large, coherent oscillations exist across the Strait of Sicily wi th 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 approxi mation to the gravitational barotropic normal modes with realistic topograp hy. It is observed that these oscillations are related to the passage of sy noptic weather systems over the region. An investigation on the configurati on, phase velocity, and direction of approach of atmospheric disturbances o ver the region suggests that the oscillations in the Strait of Sicily could be forced by instabilities that develop in large-scale, low pressure front s that propagate as pressure gravity waves with an approximate phase speed between 24 and 30 m s(-1).