Measurements of CMB by the
COBE gave the Nobel Prize in Physics in 2006 to Georg Smooth and John Mather for discovering CMB. Similarly, measurements of DLR are presented as evidence of DLR supporting CO2 alarmism.
The existence of both CMB and DLR is thus manifested by certain instrument readings and to understand the nature of CMB and DLR, we have to ask what in fact the instrument or detector, is recording.
The detector of CMB is a radio-telescope, which like a radio tuner tunes in different resonance frequencies of an antenna which produces an electrical signal, which is amplified into a recording over frequency or a spectrum.
The recorded spectrum is matched with a black-body spectrum according to Planck's law,
where the peak of the recorded spectrum determines the temperature (3 K) from which a radiance can be computed by Planck's law. The recorded spectrum is thus translated by using Planck's law into a radiance measured in W/m2, which is perceived as a "faint glow".