The Sunyaev--Zel'dovich (S--Z) effect (Sunyaev & Zel'dovich (1980)) is a secondary anisotropy in the Cosmic Microwave Background (CMB), due to inverse-Compton scattering of CMB photons by the hot electron atmosphere which exists in the potential well of clusters of galaxies. In the Rayleigh-Jeans region of the CMB spectrum, this results in a decrement in the CMB. This signal is small, only 1 mK even for the richest clusters, and is also diffuse.