The following is from the February 1989 issue of QEX from an article written by H. Paul Shuch, N6TX, called A Low-Noise Preamp For Weather Satellite VISSR Reception. Geostationary weather satellites, from which radio amateurs have long delighted in recovering earth images, actually provide two distinct products. WEFAX, or weather facsimile is the more familiar of the two, and consists of preprocessed and enhanced frames, taken at visible or infrared wavelengths, relayed via a frequency modulated microwave carrier, in slow scan format (four lines per second). Because of its relatively narrow bandwidth (30 kHz per channel) and respectable output power (on the order of 5 watts), the WEFAX signal is commonly received with little effort using relatively simple equipment. But the data is secondhand. WEFAX images are analog retransmissions of raw satellite data that has been downlinked to a central datacollection facility for processing, then returned to the satellite for distribution. In WEFAX mode, the satellite is thus serving as a repeater. In its other operating mode, the familiar WEFAX satellite provides a wide-band digital signal variously called VISSR for Visible and Infrared Spin-Scan Radiometer, the image sensor on the satellites, VAS, for VISSR Atmospheric Sounder, or HRPT for High-Resolution Pictur Transmission, which highlights the signals advantage over WEFAX. throughout this article, I shall use the term VISSR. The ultimate microwave challenge is reception and display of raw satellite data prior to processing. this has until recently been an elusive goal, because in the digital mode, the satellite is transmitting at greater than 2 Mbits per second. Hence, a wide receiver bandwidth (on the order of 8 MHz) is required. Thus, though the VISSR transmitter power is on a par with that of the WEFAX transmission, the modulation sidebands are spread over a frequency spectrum about 300 times as wide. The resulting low spectral density makes it necessary to employ some rather sophisticated receiving equipment; government stations emply 60 foot dishes, parametric amplifiers and large mainframe computers for image processing.