The development of a 1.4-mm heterodyne radiometric system and the initial measurements taken with it are described. The

of the system at the antenna terminals was approximately

K for a 0.25-Hz post-correlation noise bandwidth. Measurements show that the attenuation through the atmosphere at this wavelength is primarily due to water vapor, and an estimate of the zenith attenuation is given by

, where

is the precipitable water in centimeters. Measurements of the antenna half-power beamwidths using the sun as a source show that at 1.4 mm the atmospheric turbulence effects are not appreciable for observations through the atmosphere at zenith angles less than

with a 15-foot antenna.