The NASA Deep Space Network (DSN) has a long history of providing larg
e parabolic dish antennas with precision surfaces, low-loss feeds, and
ultra-low noise amplifiers for deep-space telecommunications. To real
ize the benefits of high sensitivity, it is important that receiving s
ystems are accurately calibrated and monitored to maintain peak perfor
mance. A method is described to measure system performance and to cali
brate the receiving system using procedures, software, and commercial
instruments that are easy to implement and efficient to use. The utili
ty of the measurement procedures and the precision of the receiver cal
ibration technique were demonstrated by performing tests at K(a)-band
(32 and 33.68 GHz) frequencies at Goldstone on a 34-m beam-waveguide a
ntenna. Observations of multiple calibration radio sources are used to
measure the dependence of antenna gain and system noise temperature o
n source elevation and derive the performance parameters. Receiving sy
stem nonlinearities are frequently overlooked as an error source in th
e calibration of microwave radiometers. The experimental results descr
ibed in this paper illustrate some of the ways that receiving system n
onlinearity can negatively impact system performance. A simple radiome
ter calibration technique and analysis provide quantitative informatio
n that enables the system engineer to adjust and linearize the receivi
ng system. When that is not practical, the experimenter or the operato
r can apply correction coefficients to the measured values of system n
oise temperature and thereby compensate for the receiving system nonli
nearity. The high-performance antennas and the sensitive receiving sys
tems of the DSN are valuable resources for scientific research in addi
tion to the primary telecommunication tasks that support space mission
s. The antenna gain and system noise temperature measurements and the
radiometer calibration method described in this paper are also useful
to perform precision research experiments.