Anisotropies in the cosmic microwave background (CMB) encode information ab
out the evolution and development of the universe. Quality observations of
CMB anisotropies can provide a very strong test of cosmological models and
provide high precision determination of major cosmological parameters. This
paper provides a review of the COBE DMR results, the current status of the
measurements of the CMB anisotropy power spectrum and then focuses current
and future programs including both suborbital observations and the two sel
ected satellite missions: the NASA MidEX mission MAP and the ESA M3 mission
Max Planck Surveyor. This review includes both a description of the experi
mental programs and the expected quality level of results. (C) 2000 Elsevie
r Science B.V. All rights reserved.