Of interest for a transformation is the surroundings that can interact with the object of interest.
On Earth it's often the atmosphere.
Cases on Earth where a mean Universe temperature is meaningful are rare. For a space probe, the Sun would be one part of the environment, a planet if near enough, and the Universe the rest; even for Pioneer at its present distance, whether the Universe has 0K, 2.7K or a bit more makes no difference and the Sun is more important.
One difficulty with a mean temperature is that the Universe isn't uniform, so it radiates at varied wavelengths. A perfect black body would feel some mean Universe temperature which wouldn't be meaningful for a normal body, which (is designed to) has varied absorptivity at different wavelengths.
At very sensitive telescopes and antennas, designers try to decouple the receiver from the warm and noisy Earth. This includes directivity so the receiver senses heat only from the target direction, and possibly cold baffles in other directions.
See the home antennas for satellite TV? Apart from the paraboloid, they have a "primary source" (often a horn) which is well below the dish's axis, at least at mid-latitudes where I am. One important purpose is that this primary source looks to the sky, so that the secondary lobes in its sensitivity diagram which miss the dish look to the cold sky, not to the warm Earth.
Even with such tricks, an antenna temperature (=the noise it picks) would be 20K...150K depending on the wavelength and the design, so a "mean universe temperature" would be hard to define. But tables exist for the background temperature of the sky depending on the wavelength.