http://www.cnr.it/ontology/cnr/individuo/prodotto/ID6467
The 'Mad Sea' phenomenon in the Strait of Sicily (Articolo in rivista)
- Type
- Label
- The 'Mad Sea' phenomenon in the Strait of Sicily (Articolo in rivista) (literal)
- Anno
- 1999-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1175/1520-0485(1999)029<2210:TMSPIT>2.0.CO;2 (literal)
- Alternative label
Candela J., Mazzola S., Sammari C., Limeburner R., Lozano C. J., Patti B., Bonanno A. (1999)
The 'Mad Sea' phenomenon in the Strait of Sicily
in Journal of physical oceanography
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Candela J., Mazzola S., Sammari C., Limeburner R., Lozano C. J., Patti B., Bonanno A. (literal)
- Pagina inizio
- Pagina fine
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
- http://apps.webofknowledge.com/full_record.do?product=WOS&search_mode=GeneralSearch&qid=1&SID=V1D6@Lkjb5jOO7MjGol&page=4&doc=39 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
- Rivista
- Note
- ISI Web of Science (WOS) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- IAMC-CNR U.O. DI MAZARA DEL VALLO (ITALY)
INSTM DI TUNISI (TUNISIA)
WHOI DI WOODSHOLE (USA) (literal)
- Titolo
- The 'Mad Sea' phenomenon in the Strait of Sicily (literal)
- 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. (literal)
- Prodotto di
- Autore CNR
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