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Slow-scan television (SSTV) is used by amateur radio operators, to transmit and receive static pictures in monochrome (black & white) or colour.
Early originsSSTV was used extensively during the early years of the NASA Apollo program to transmit images to Earth, and the first images from Apollo 11 on the Moon were SSTV. (See also Apollo moon landing hoax accusations.) Narrow bandwidthBroadcast television requires huge 5, 6 or 8 MHz wide channels, because it transmits 25 or 30 pictures per second (in the NTSC, PAL or SECAM systems).
Hardware originsSSTV originally required quite a bit of specialized equipment. Usually there was a scanner or camera, a modem to create and receive the characteristic audio howl, and a cathode ray tube from a surplus radar set. The special cathode ray tube would have "long persistence" phosphors that would keep a picture visible for a minute or so. The modem would generate audio from pictures, and pictures from audio. The audio would be attached to a radio receiver and transmitter. The modern system uses a personal computer and special software in place of much of the custom equipment. The audio system of a PC, with special processing software, acts as a modem. The computer screen provides the output. A small digital camera or digital photos provide the input. Since SSTV produces and generates audio, amateurs use it on shortwave, Slow-scan television VHF and UHF radio. References
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The field of electronics is the study and use of systems that operate by controlling the flow of electrons or other electrically charged particles in devices such as thermionic valves and semiconductors. The design and construction of electronic circuits to solve practical problems is part of the fields of electronic engineering, and the hardware design side of computer engineering. The study of new semiconductor devices and their technology is sometimes considered as a branch of physics. # - A | B | Co - Cz | C - Cm | D Em - F | E - El | G - H | I - K | L - Ma |
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