High resolution millimeter reflector antennas

The foremost millimeter reflector antennas in use are surveyed. Antenna descriptions are written by personnel at the institutions operating the antennas. The antennas described are the following: 1) MIT 28-foot and 120-foot (U.S.A.), 2) Lebedev and Crimean RT 22-meter (USSR), 3) Aerospace 15-foot (U.S.A.), 4) University of Texas 16-foot (U.S.A.), 5) AFCRL 29-foot (U.S.A.), 6) Bonn University 10-meter (Germany), 7) (CRC (DRTE) 30-foot (Canada), 8) NRAO 36-foot (U.S.A.), 9) Berkeley 20-foot (U.S.A.), and 10) JPL 18-4oot (U.S.A.). Antenna system descriptions include information on antenna performance, pointing capabilities, limitations, and principal applications. The antennas are used in radio astronomy and communication research. The reference section covers the major results obtained with the antennas.

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[6]  F. Low Thermal detection radiometry at short millimeter wavelengths , 1966 .

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[37]  C. Tolbert Observed millimeter wavelength brightness temperatures of Mars, Jupiter, and Saturn , 1966 .

[38]  K. Takahashi AN INVESTIGATION OF SOLAR EMISSION AT FREQUENCIES OF 35, 70, AND 94 Gc WITH A 4.88-METER DIAMETER TELESCOPE. , 1967 .

[39]  E. Altshuler,et al.  A troposcatter propagation experiment at 15.7 GHz over a 500 km path , 1968 .