For the last several years, there has been increasing interest in obtaining high-resolution (sub-kilometer) marine wind speed measurements from SAR imagery. The need for higher resolution wind fields in coastal areas, in frontal systems and tropical storms cannot be obtained with wind fields measured onboard conventional space-based satellites such as scatterometers (e.g., QuikSCAT) or passive microwave radiometers (e.g., SSM/I and the recently launched WindSat). These sensors are best suited for global measurements, because with 25-km spatial resolution many important high-resolution spatial phenomena are missed.
The normalized radar cross-section (NRCS) at the incidence angles in the range of 20° to 70° is dominated by Bragg resonant scattering from centimetric waves traveling in the direction of the incident microwave energy. Consequently the radar reflectivity is strongly dependent on direction of propagation of these short waves with respect to that of the radar energy. These short waves are known to propagate centered on the wind direction. The SAR images can be used to determine a spatial average of the instantaneous backscatter, i.e. the roughness of the ocean surface. Thus the accurate retrieval of wind speed and direction are linked. First, the estimation of wind direction from SAR images is determined from surface features like wind streaks. The calibrated NRCS is then taken together with this direction to determine wind speed by applying a CMOD-type algorithm originally developed for the ERS scatterometer.
The spatial resolution of the derived wind fields from the different SAR systems is about 500 m. The results will be compared with in-situ measurements such as buoys which provide a temporal average at a location from anemometers or sonic measurements at a specific height.