Space-time structure of long ocean swell fields

Type Publication
Date 2010-12
Language English
Copyright 2010 American Geophysical Union
Author(s) Delpey Matthias T.1, Ardhuin FabriceORCID1, Collard Fabrice3, Chapron Bertrand2
Affiliation(s) 1 : Serv Hydrog & Oceanog Marine, F-29200 Brest, France.
2 : IFREMER, ZI Ctr Brest, Lab Oceanog Spatiale, F-29280 Plouzane, France.
3 : Collecte Localisat Satellites, Div Radar, F-29280 Plouzane, France.
Source Journal Of Geophysical Research-oceans (0148-0227) (Amer Geophysical Union), 2010-12 , Vol. 115 , N. C12037 , P. 13 p.
DOI 10.1029/2009JC005885
WOS© Times Cited 26
Abstract The space-time structure of long-period ocean swell fields is investigated, with particular attention given to features in the direction orthogonal to the propagation direction. This study combines space-borne synthetic aperture radar (SAR) data with numerical model hindcasts and time series recorded by in situ instruments. In each data set the swell field is defined by a common storm source. The correlation of swell height time series is very high along a single great circle path with a time shift given by the deep water dispersion relation of the dominant swells. This correlation is also high for locations situated on different great circles in entire ocean basins. Given the Earth radius R, we define the distance from the source R alpha and the transversal angle beta so that alpha and beta would be equal the colatitude and longitude for a storm centered on the North Pole. Outside of land influence, the swell height field at time t, H-ss(alpha, beta, t) is well approximated by a function H-ss,H-0(t - R alpha/C-g)/root(alpha sin(alpha)) times another function r(2) (beta), where C-g is a representative group speed. Here r(2) (beta) derived from SAR data is very broad, with a width at half the maximum that is larger than 70 degrees, and varies significantly from storm to storm. Land shadows introduce further modifications so that in general r(2) is a function of beta and alpha. This separation of variables and the smoothness of the H-ss field, allows the estimation of the full field of H-ss from sparse measurements, such as wave mode SAR data, combined with one time series, such as that provided by a single buoy. A first crude estimation of a synthetic H-ss field based on this principle already shows that swell hindcasts and forecasts can be improved by assimilating such synthetic observations.
Full Text
File Pages Size Access
Publisher's official version 13 5 MB Open access
Top of the page