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Large-angular-scale anisotropy in the cosmic background radiation

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/158714· OSTI ID:6335863
We report the results of an extended series of airborne measurements of large-angular-scale anisotropy in the 3 K cosmic background radiation. Observations were carried out with a dual-antenna microwave radiometer operating at 33 GHz (0.89 cm wavelength) flown on board a U-2 aircraft to 20 km altitude. In 11 flights, between 1976 December and 1978 May, the radiometer measured differential intensity between pairs of directions distributed over most of the northern hemisphere. The measurements show clear evidence of anisotropy that is readily interpreted as due to the solar motion relative to the sources of the radiation. The anisotropy is well fitted by a first order spherical harmonic of amplitude 3.6 +- 0.5 mK, corresponding to a velocity of 360 +- 50 km s/sup -1/ toward the direction 11.2 +- 0.5 hours of right ascension and 19/sup 0/ +- 8/sup 0/ declination. A simultaneous fit to a combined hypothesis of dipole and quadrupole angular distributions places a 1 mK limit on the amplitude of most components of quadrupole anisotropy with 90% confidence. Additional analysis places a 0.5 mK limit on uncorrelated fluctuations (sky-roughness) in the 3 K background on an angular scale of the antenna beam width, about 7/sup 0/.
Research Organization:
Space Sciences Laboratory and Lawrence Berkeley Laboratory, University of California, Berkeley
OSTI ID:
6335863
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 244:2; ISSN ASJOA
Country of Publication:
United States
Language:
English