Infrared limit on the fine-scale anisotropy of the cosmic background radiation

Details Infrared limit on the fine-scale anisotropy of the cosmic background radiation Infrared limit on the fine-scale anisotropy of the cosmic background radiation

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phrvd..16.2424c&link_type=abstract

Physical Review D - Particles and Fields, 3rd Series, vol. 16, Oct. 15, 1977, p. 2424-2429.

Astronomy and Astrophysics

Astronomy

18

Anisotropic Media, Background Radiation, Galactic Evolution, Infrared Astronomy, Atmospheric Windows, Big Bang Cosmology, Hydrogen Ions, Microwave Emission, Perturbation Theory, Vorticity

Scientific paper

The cosmic-background anisotropy has been investigated at the angular scale of 25 arcmin by means of a special isotropometer at the alpine station of Testa Grigia (3500 m above sea level) through the atmospheric window 1.0-1.4 mm. An upper limit of 0.00012 at two standard deviations is found for the sky anisotropy. Some physical implications about the origin and rotation of superclusters and about the secondary ionization of plasma are discussed.

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