Abstract

Short gravity-capillary waves, the predominant radar scatterers under many oceanic and radar-viewing conditions, are modulated in amplitude, velocity and orientation by the larger-scale motions of the ocean surface. These modulations render the larger scales observable to microwave radar. The high data rate and advanced technology of modern radar systems make it possible to measure these modulations and, in some cases, to display them as images of the ocean surface. While the modulation of orientation and velocity are straightforward to understand, the amplitude modulation is a dynamic response of the equilibrium short gravity-capillary waves to larger scale driving forces including straining by orbital velocities of large waves. Microwave studies of the growth and equilibrium of short wind-generated waves are reviewed. It is shown that the response of these waves to straining can produce modulations in radar cross-section greater than those due to tilting but which are wind-speed dependent. The net modulation depends strongly on the direction as well as the magnitude of the wind speed. Quantitative determination of ocean wave-height spectra from measured modulations will therefore be a complicated procedure. Measurements of ocean waves with CW Doppler and Synthetic Aperture radars are discussed in the light of these findings.

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