Precise radiometric tracking is of key importance during operations of interplanetary missions and for advanced radio science applications. Radio science research performed on deep space missions like Cassini, Juno, BepiColombo, and the upcoming JUICE mission, rely on a combination of X and K a band radio links to mitigate the dispersive effects of propagation through interplanetary plasma, solar corona, and Earth ionosphere, leaving tropospheric delay as one of the main error contributors to Doppler and ranging measurements.To meet the demanding requirements of BepiColombo's Mercury Orbiter Radio science Experiment (MORE) (Iess et al., 2021) and JUICE's Geodesy and Geophysics of Jupiter and the Galilean Moons (3 GM) radio science experiment (Cappuccio et al., 2020), in terms of radiometric tracking accuracy and end-toend stability of the Doppler signals, ground-based microwave radiometers (MWR) are deemed as the most appropriate instruments for tropospheric delay calibration (Iess et al., 2009).Microwave radiometers have been extensively used in the past decades for the correction of tropospheric induced delay in astrometric and geodetic observations using very large base interferometry (VLBI) (Nikolic et al., 2013;Roy et al., 2007). However, their application to deep space radiometric tracking was originally introduced by the Jet Propulsion Laboratory (JPL) to support the Cassini radio science experiments, with the development and installation of two dedicated high-stability water vapor radiometers at the Goldstone deep space communication complex in California (