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dc.contributor.authorMontalvo, P.-
dc.contributor.authorKraenkel, R.-
dc.contributor.authorManna, M. A.-
dc.contributor.authorKharif, C.-
dc.date.accessioned2014-12-03T13:11:17Z-
dc.date.accessioned2016-10-25T20:13:45Z-
dc.date.available2014-12-03T13:11:17Z-
dc.date.available2016-10-25T20:13:45Z-
dc.date.issued2013-01-01-
dc.identifierhttp://dx.doi.org/10.5194/nhess-13-2805-2013-
dc.identifier.citationNatural Hazards And Earth System Sciences. Gottingen: Copernicus Gesellschaft Mbh, v. 13, n. 11, p. 2805-2813, 2013.-
dc.identifier.issn1561-8633-
dc.identifier.urihttp://hdl.handle.net/11449/113000-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/113000-
dc.description.abstractWe extend the Miles mechanism of wind-wave generation to finite depth. A beta-Miles linear growth rate depending on the depth and wind velocity is derived and allows the study of linear growth rates of surface waves from weak to moderate winds in finite depth h. The evolution of beta is plotted, for several values of the dispersion parameter kh with k the wave number. For constant depths we find that no matter what the values of wind velocities are, at small enough wave age the beta-Miles linear growth rates are in the known deep-water limit. However winds of moderate intensities prevent the waves from growing beyond a critical wave age, which is also constrained by the water depth and is less than the wave age limit of deep water. Depending on wave age and wind velocity, the Jeffreys and Miles mechanisms are compared to determine which of them dominates. A wind-forced nonlinear Schrodinger equation is derived and the Akhmediev, Peregrine and Kuznetsov-Ma breather solutions for weak wind inputs in finite depth h are obtained.en
dc.description.sponsorshipLabex NUMEV (Digital and Hardware Solutions, Modeling for the Environment and Life Sciences)-
dc.format.extent2805-2813-
dc.language.isoeng-
dc.publisherCopernicus Gesellschaft Mbh-
dc.sourceWeb of Science-
dc.titleWind-wave amplification mechanisms: possible models for steep wave events in finite depthen
dc.typeoutro-
dc.contributor.institutionUniv Montpellier 2-
dc.contributor.institutionCNRS-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionEcole Cent Marseille-
dc.contributor.institutionAMU-
dc.description.affiliationUniv Montpellier 2, Lab Charles Coulomb, UMR5221, F-34095 Montpellier, France-
dc.description.affiliationCNRS, UMR5221, Lab Charles Coulomb, F-34095 Montpellier, France-
dc.description.affiliationUNESP Univ Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil-
dc.description.affiliationEcole Cent Marseille, F-13451 Marseille 20, France-
dc.description.affiliationAMU, CNRS, UMR7342, Inst Rech Phenomenes Hors Equilibre, F-13384 Marseille 13, France-
dc.description.affiliationUnespUNESP Univ Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil-
dc.identifier.doi10.5194/nhess-13-2805-2013-
dc.identifier.wosWOS:000327800200009-
dc.rights.accessRightsAcesso aberto-
dc.identifier.fileWOS000327800200009.pdf-
dc.relation.ispartofNatural Hazards And Earth System Sciences-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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