Comparisons of simulated and actual synthetic aperture radar gravity wave images

The synthetic aperture radar (SAR) images obtained with the Jet Propulsion Laboratory's L band system in the Tower Ocean Wave and Radar Dependence (TOWARD) oceanographic experiment are compared with images generated by a simulation program implementing a SAR ocean imaging model based on two-scale hydrodynamic and electromagnetic scattering approximate models. A critically regarded test of a theory of SAR ocean imaging is its prediction of the best image focus dependence on surface motion. The primary means of comparison here is an estimate of the best focus parameter that uses a subimage cross-correlation technique. The focus parameter estimates for both the actual and simulated images show (1) a reversal in sign with reversal in dominant longwave direction relative to the SAR direction, (2) a magnitude increase with an increase in magnitude of the angle between the dominent long wave and SAR axes, and (3) an independence of the altitude and also the range-to-velocity ratio. All equivalent velocity estimates are of the order of the dominant longwave phase velocity, normalized by the SAR vehicle velocity, and agree well qualitatively though there are some quantitative differences. These behaviors are in agreement with a related analytical prediction. The “visibility” of the long waves' SAR image artifacts, for this TOWARD data set, increased with increased altitude and also with increased range-to-velocity ratio for both the actual and simulated images, as was predicted by a related analysis. Agreement of spectral density estimates of the actual and simulated SAR images generally required an order of magnitude increase in the strength of the hydrodynamic interaction of the long and short waves. This may indicate, as have surface measurements in TOWARD and other experiments, that the two-scale model does not fully describe this nonlinear interaction. With this interaction adjustment, a comparison of actual and simulated images using an alternative focus criterion showed very close agreement in some cases.

[1]  O. Shemdin,et al.  Synthetic aperture radar imaging of ocean waves during the marineland experiment , 1983 .

[2]  F. Bass,et al.  Wave scattering from statistically rough surfaces , 1979 .

[3]  Robert O. Harger,et al.  The side‐looking radar image of time‐variant scenes , 1980 .

[4]  Robert A. Shuchman,et al.  Processing of ocean wave data from a synthetic aperture radar , 1978 .

[5]  Owen M. Phillips,et al.  The dispersion of short wavelets in the presence of a dominant long wave , 1981, Journal of Fluid Mechanics.

[6]  I. Ostrovsky,et al.  Very high frequency radiowave scattering by a disturbed sea surface Part I: Scattering from a slightly disturbed boundary , 1968 .

[7]  O. H. Shemdin,et al.  Measurement of high frequency waves using a wave follower , 1983 .

[8]  R. Harger Synthetic aperture radar systems , 1970 .

[9]  Robert O. Harger,et al.  The SAR Image of Short Gravity Waves On a Long Gravity Wave , 1986 .

[10]  D. Ross,et al.  On the detectability of ocean surface waves by real and synthetic aperture radar , 1981 .

[11]  J. Wright,et al.  Backscattering from capillary waves with application to sea clutter , 1966 .

[12]  Fuk K. Li,et al.  Doppler Parameter Estimation for Spaceborne Synthetic-Aperture Radars , 1985, IEEE Transactions on Geoscience and Remote Sensing.

[13]  J. Wright A new model for sea clutter , 1968 .

[14]  G. Valenzuela,et al.  Scattering of Electromagnetic Waves From a Tilted Slightly Rough Surface , 1968 .

[15]  Robert C. Beal,et al.  Large‐and small‐scale spatial evolution of digitally processed ocean wave spectra from SEASAT synthetic aperture radar , 1983 .

[16]  O. H. Shemdin,et al.  L band SAR ocean wave observations during Marsen , 1983 .

[17]  The structure of short gravity waves on the ocean surface , 1981 .

[18]  M. Longuet-Higgins A stochastic model of sea-surface roughness. I. Wave crests , 1987, Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences.