The 45m Radio Telescope: A 45m single-dish
radio telescope that operates in short-millimetre wavelengths. Its receivers operate at 1, 2, 3.75, 9.4, 17, 35, and 80 GHz in both left and right polarizations.
The Nobeyama Millimetre Array (NMA): An millimetre
interferometer consisting of six 10m diameter
telescopes.
The Nobeyama Radioheliograph (NoRH): An array of eighty-four, 80 cm antennas dedicated for
solar observations. Its receivers operate at 17–34 GHz in both left and right polarizations.[1]
The Nobeyama Radio Polarimeters: A set of radio telescopes that continuously observes the full Sun at the frequencies of 1, 2, 3.75, 9.4, 17, 35, and 80 GHz, at left and right circular polarization.[2]
The 45m Radio Telescope: A 45m single-dish
radio telescope that operates in short-millimetre wavelengths. Its receivers operate at 1, 2, 3.75, 9.4, 17, 35, and 80 GHz in both left and right polarizations.
The Nobeyama Millimetre Array (NMA): An millimetre
interferometer consisting of six 10m diameter
telescopes.
The Nobeyama Radioheliograph (NoRH): An array of eighty-four, 80 cm antennas dedicated for
solar observations. Its receivers operate at 17–34 GHz in both left and right polarizations.[1]
The Nobeyama Radio Polarimeters: A set of radio telescopes that continuously observes the full Sun at the frequencies of 1, 2, 3.75, 9.4, 17, 35, and 80 GHz, at left and right circular polarization.[2]