The paper is focused on investigation of microwave backscattering from wind waves on a clean water surface. Field experiments were carried out in the coastal zone of the Black Sea using dual co-polarized Doppler X-band scatterometer and a three-band Doppler dual co-polarized radar (X-, С-, S-bands). The radar incidence angles were about 50 - 60 degrees, the wind changed in a wide range of speeds. We assumed that microwave backscattering at VV and HH polarizations is composed by a Bragg (polarized) component associated with Bragg waves and a non-polarized component (NBR). Analysis of Doppler spectra of NBR allowed us to remove the effect of strong wave breaking (overturning wave crests) from the time series and to study the backscatter associated only with dm-scale waves. Measurements of wind waves with a wire gauge were carried out simultaneously with the radar monitoring. It is shown that the velocities of non-Bragg scatterers not associated with strong wave breaking in X-, С-, S-bands correspond to the velocities of short dm waves and weakly depend on radar wavelength. The speeds of the scatterers in X-, С-, S-bands associated with overturning wave crests are also close to each other (within the measurement error). The intensity of NBR in X-, С-, S-bands grows with wind speed as well as with the intensity of dm-waves measured by the wire gauge. Strong suppression of NBR and simultaneously measured decrease of short dm-wave intensity are demonstrated, thus confirming the assumption that the intensity of the NBR in X-, С-, S-bands is determined by dm waves.
The role of wave breaking in microwave backscattering from the sea surface is a problem of great importance for development of theories and methods of the ocean remote sensing. Recently it has been shown that the microwave radar return is determined by both Bragg and non Bragg scattering components, and some evidences have been given that the latter is associated with wave breaking. However, our understanding of different mechanisms of the role of wave breaking on small-scale wind waves (ripples) and thus on the radar return is still insufficient. This paper presents results of laboratory experiments on the influence of wave breaking on Ka-band radar signals. An effect of the radar return suppression after wave breaking has been revealed and attributed with wind ripples suppression by breaking waves. The experiments were carried out in an oval wind wave tank where intense m/dm-scale surface wave trains were generated by a mechanical wave maker, in particular using a method of dispersive wave focusing. Wind waves were independently generated in the wave tank. A Ka-band radar was mounted at a height of about 1 m above the water level the incidence angle of microwave radiation was about 50 degrees. The experiments were performed both for a clean water surface and in the presence of an oleic acid monomolecular film. It has been obtained that the radar return before the wave train was determined by wind ripples, the radar Doppler spectrum was centered close to the Bragg wave frequencies. The radar signal intensity was strongly enhanced in a wide frequency range when the train was passing by the study area. After the intense wave train the radar return dropped and then slowly recovered to the initial level. We believe that the attenuation of radar backscattering after the wave train is due to suppression of wind ripples by turbulence and surfactants associated with wave breaking.
Analysis of possibilities of identification and characterization of marine processes using their signatures in radar and optical imagery of the sea surface is a very important problem of the ocean remote sensing which has not been solved yet completely by now. Marine slicks which are the areas of suppressed wind waves can be recorded by different sensors and can be indicators of internal waves, non uniform currents, atmospheric convective cells, etc. Field studies including those simultaneous and co-located with remote observations is the most perspective way to the problem solution. An expedition of the Institute of Applied Physics RAS was organized to study the nature of slick bands and its dynamics in the field of various subsurface processes. Field experiments were carried out in the coastal zone of the Black sea from the Oceanographic Platform of Marine Hydrophysical Institute RAS and from the shore. The structure of the currents in the studied area is characterized by significant heterogeneity, so we were able to register different slick structures in the flow field and wind and the slick dynamics. In some experiments, marine slicks were recorded simultaneously in satellite Sentinel images. Observations of surface manifestations of internal waves were carried out using a digital radar station MRS-1000 and multi-frequency radar complex of IAP RAS. At the same time the measurements of currents in the water column were carried out using the ADCP WH Monitor 1200 kHz, wind speed and direction at a height of 30 meters using WindSonic acoustic anemometer. During the passage of internal waves a system of slick bands with a reduced intensity of small-scale waves were observed. Slick bands were observed mainly over the rear slopes of the internal waves; the data from the accompanying measurements showed that the phase velocity was close to the surface current velocity. Theoretical analysis has shown that in this case the convergent zones, where surfactants are accumulated were formed at the rear slopes of the internal waves. This mechanism of slick formation was predicted earlier theoretically and then was modeled in laboratory experiment.
Recent studies of microwave radar return at moderate and large incidence angles have shown the backscattering is determined by resonance (Bragg) surface waves of cm-scale wavelength range, and by non polarized (non Bragg) component which is associated with wave breaking and quasi specular reflection. This paper is focused on results of field studies of non-Bragg backscattering from the clean water surface and from the water surface covered with surfactant films. The study was carried out using dual polarized X-band radars in the coastal zone of the Black Sea in 2017-2019 at an incidence angle of about 60 degrees. It was found that the radar return contains a Non Bragg component not related to the breaking crests and specular tilt areas at wind speeds from a threshold of the wind wave generation up to wind velocities of the order of 10 m/s. The part of the non-Bragg component not related to the wave breaking crests decreases strongly in the areas of film slicks. At high wind velocities the non-Bragg component out of the spikes is strongly modulated (several times larger than the Bragg component) in the long-wave field, in film slicks the modulation of the non-Bragg component increases. Analysis of the Doppler shifts showed that the velocities of the non-Bragg scatterers correspond to the dm-scale free surface waves and vary slightly in the areas of film slicks. Thus, we concluded that nonlinear features associated with the dm-scale wind waves cause the non-Bragg scattering.
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