Professor at WKU in the 1990s, experimented with receiving Galactic radioĮmissions using dipole antennas at Bell for student education, in a forerunner Sandra Clemens, another UF graduate who was a visiting (0.6-m) Bell optical telescope, particularly for monitoring quasars and other WKU astronomy research focused on use of the 24-inch The radio observatory was shut down, and equipment on loanįrom UF was returned. The radio observatory was maintained at Bell Farm for over a decade.įollowing Frank Six's departure from WKU in 1983, local radio astronomyĪctivity waned. Land Bell donated in 1976, although construction was not completed until 1987. ![]() The foot of the hill where WKU's optical observatory would later be built on This was 10 miles west-southwest of Bowling Green, at ![]() The new facility was placed on a farm belonging to Warren County JudgeĮxecutive Charles Bell. The station was rebuilt in a different location the following year, and the This posed a significant setback for Roger Scott's M.S. Magnetic tape recorder the large polar-mounted Yagi antenna Rain storm in June 1969 ruined the building and equipment it housed, includingĪ Collins receiver, Texas Instruments paper chart recorder, and Magnavox Unfortunately, this site was in the flood plain of Drake's Creek, and a heavy The community of Alvaton, 10 miles south-southeast of Bowling Green. The first WKU radio observatory was on farm land owned by Rogers Lawson near (Although only briefly at WKU, Sky laterīecame a key member of the Radio Jove project.) If you know of other people who should be listed here, Students in the WKU program included Jesse Burd, Bill Allen, Bruce Allen, Ed Student first - one of several who went through Six's radio astronomy program, Karen Hackney in 1973, and Roger Scott in 1991. Other hires of UF alumni as WKU faculty included Richard Hackney in 1972, Although the Chile receiving station was subject to technicalĬhallenges and political uncertainties, valuable data were obtained and Operational, Flagg helped build the Chile receiving station, shortly after theĬommissioning of large optical observatories nearby at Cerro Tololo and La Member in physics and engineering, with additional assistance from WKU OgdenĬollege Machine Shop technician Alonzo Alexander. Robinson provided long-term support after being hired in 1968 as a WKU faculty UFĮngineers Dick Flagg and Max Robinson assisted with the initial WKU setup. Was first demonstrated coherently by Canadian astronomers in 1967). Times in the three locations in order to pinpoint the precise origins of theĮmissions within Jupiter's magnetosphere (an early application of VLBI, which Of 18 MHz Jupiter emissions in coordination with parallel observations runīy UF in Florida and Chile, with the intention of comparing the signal arrival Program became founders of the Radio Jove project inįrank Six established the WKU Radio Observatory to make high-speed recordings Waves from outside the Earth's atmosphere. Washington in 1955 - just two decades after Karl Jansky first detected radio ![]() Smith, and others at UF, including student (and later faculty member) ThomasĬarr, began studying Jupiter radio emissions immediately following theirĭiscovery by Bernard Burke and Kenneth Franklin at the Carnegie Institution of at the University of Florida inġ963 on bursts of low-frequency radiation from Jupiter and wished to extend The WKU radio astronomy program was initiated by Physics & Astronomyĭepartment Head Frank Six in 1967, the year after he was hired into the Project to foster education and public outreach in radio astronomy. Was recently revived on a more modest scale as part of NASA's Radio Jove Of the first very long baseline interferometry ever attempted. With particular focus on the planet Jupiter in the early days, including some Western Kentucky University has a long history of radio astronomy activity, History of Radio Astronomy at WKU History of Radio Astronomy at WKU
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