In this paper an infrared single element two-dimensional acoustooptic processor using a crystal of tellurium will be described, that can process to return echos of each pulse to form the image of the terrain illuminated by the SAR in real-time. This highly compact processor is designed to maintain a range and azimuth resolution of 2 m, will operate with an acoustic bandwith of 200 MHz for an acoustic drive-power of only 1 watt at the optic wavelength of 5 jim and will reach a dynamic range of the order of 40dB determined by the Hg Cd Te CCD array. This processor will control range and azimuth sidelobes below 40 dB, in a minimum detector integration time of 200 ms to resolve a 5 Hz Doppler frequency.
INTRODUCTIONTo describe how synthetic aperture radar (SAR) works, let us take the example of Magellan's Venus orbiter. Any point in the radar map image can be located by using two measurements -the distance to the point (determined by the time it takes for the radar signals to return to Magellan), and the amount of Doppler shift in the signal (a shift in frequency caused by the spacecraft's motion along its orbit). However, two widely separated points (such as A and B shown in Fig 1 a) have the same delay and Doppler shift. Consequently, to avoid confusion between these two points, Magellan's SAR antenna will be pointed to the left of the orbital ground track to illuminate only one of these possible points (A as shown here, B will have already been mapped in a previous orbit's swath). The resulting radar map will therefore show only features to the left of the ground track. The portion of the Venusian surface shown here is a radar image form the Soviet Venera mission, and in Fig I b Nasa picture showing the stri king difference in resolution from a picture taken by the Arecibo radio-telescope and Magellan.With conventional radar, the resolution of an image depends on antenna size : the bigger the antenna, the better the resolution. A large antenna on a spacecraft, however, would be expensive and difficult to manipulate. To solve this problem, the signals from Magellan's synthetic aperture radar (SAR) are computer-processed on Earth so that they will imitate, or synthesize, the behavior of a large antenna on the spacecraft. Through this synthesis, the onboard radar sensor will operate as if it has a huge antenna and will produce high-resolution images, even though the antenna is only 3.7 meters (12 feet) in diameter. This computerized process of "aperture synthesis" is what gives SAR its resolving power as well as its name. As Magellan passes over the Venusian surface, its dish antenna will look downward and to the left side of the spacecraft's orbital path. For 37.2 minutes, the SAR antenna will emit several thousand radar pulses each second. Traveling at the speed of light, the pulses will strike and illuminate a 25-kilometer-wide (16-mile-wide) swath ot the planet's surface, and then will immediately bounce back and be received at the instrument. By recording the returned pulses, we can use two measurements on each ...