
Laboratory study of the fine structure of short surface waves due to breaking: Two‐directional wave propagation
Author(s) -
Rozenberg A.,
Ritter M.
Publication year - 2005
Publication title -
journal of geophysical research: oceans
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2004jc002396
Subject(s) - breaking wave , physics , gravity wave , mechanical wave , optics , surface wave , wavelength , capillary wave , scattering , wave propagation , longitudinal wave , computational physics
This study was stimulated by the need to identify the influence of breaking on the evolution of the short surface wave field responsible for microwave scattering. Laboratory measurements of the fine space‐time structure of short gravity‐capillary waves and Ku band scattering at grazing and moderate incidence from spilling and plunging breaking waves in a laboratory wave channel are presented. Unsteady breaking waves are generated by focusing wave groups in space‐time domains. A scanning laser slope gauge was used for measuring capillary‐gravity waves with wavelengths of 2 mm to 10 cm and frequency ranges of up to 150 Hz. A dual polarized (VV, HH) coherent pulsed Ku band scatterometer with a 3 ns temporal resolution was used to simultaneously obtain Doppler spectra of the scattered signals from the breaking area for grazing angles from 6° to 25°. Two‐dimensional filtering in the wave number‐frequency plane as well as plus/minus Doppler spectra were used to separate the direction of propagation of the surface waves within the breaking region. It was found that the breaking splash is the main source of the surface wave generation. The short surface wave slope field produced by breaking could be separated into short (4–8 mm wavelength), fast waves and free gravity‐capillary waves. Both types of waves were found to be co‐ and counterpropagate relative to the dominant wave propagation direction. The Doppler spectrograms reveal the presence of high‐frequency waves at the moment of breaking that can be associated with short, fast waves. The low‐frequency part of the Doppler spectrogram is consistent with the appearance of free waves.