Preliminary DMR measurements of the CMB isotropy

The COBE Differential Microwave Radiometers (DMR) instrument has produced preliminary full-sky maps at frequencies 31.5, 53, and 90 GHz. The redundant channels and matched beams at three frequencies distinguish the DMR from previous large-scale surveys. Galactic emission is seen unambiguously at all three frequencies. The only large-scale anisotropy detected in the cosmic microwave background is the dipole anisotropy. There is no clear evidence for any other large-angular-scale feature in the maps. Without correcting for any systematic effects, we are able to place limits {Delta}T/T{sub 0}{lt}3{times}10{sup {minus}5} for the rms quadrupole amplitude, {Delta}T/T{sub 0}{lt}4{times}10{sup {minus}5} for monochromatic fluctuations, and {Delta}T/T{sub 0}{lt}4{times}10{sup {minus}5} for Gaussian fluctuations (all limits are 95% C.L. with T{sub 0}=2.735 K). The data limit {Delta}T/T{sub 0}{lt}10{sup {minus}4} for any feature larger than 7{degree}. We briefly review the DMR and discuss some implications of these results for cosmology.