The high-resolution sea clutter is produced at high grazing angles by using the Neumann-Pierson sea surface model. The amplitude distribution and average Doppler frequency of the sea clutter produced are analyzed. The temporal and spatial auto-correlation functions are formulated, and then the correlation is analyzed. Some results are obtained with the beam in the Ku-band illuminating the sea surface in some sea state. The amplitude of the sea clutter obeys the χ2 distribution; the spectrum is widened at the shifted central frequency of 30Hz; the sea clutter has strong correlation in time and space, and the correlation time is about 20ms.