Pryke searched for polarized waves with
the Degree Angular Scale Interferometer, a microwave telescope near the South Pole.
But the new results from
the Degree Angular Scale Interferometer (DASI) and the Balloon Observations of Millimetric Extragalactic Radiation and Geophysics (BOOMERANG) project reveal two peaks and strongly suggest the presence of a third one.
Detection of B - mode polarization at
degree angular scales by BICEP2.
BICEP2 I: Detection of B - mode polarization at
degree angular scales.
Not exact matches
Another result that we don't really understand is that we don't see any temperature fluctuations in the microwave background on
scales larger than 60
degrees [the
angular size in the sky of the fluctuations].
So we put these two ideas together, applying Asantha's mapping approach to new wavelengths, and decided that the best way to get at the extragalactic background was to measure spatial fluctuations on
angular scales around a
degree.
Another experiment carried out in 1990 at the South Pole by Phil Lubin of the University of California at Santa Barbara and his colleagues may have detected primordial ripples at
angular scales of 1.5
degrees, though they are not yet convinced that they can rule out a galactic origin for their signal.