Polarization of the microwave background radiation. II. An infrared survey of the sky

The linear polarization degree of the cosmological background has been investigated at angular scales ranging between 0.5/sup 0/ and 40/sup 0/ by means of a balloon-borne far-infrared polarimeter. An upper limit has been found of 8 x 10/sup -/4 at 40/sup 0/ (at one standard deviation). Some cosmological implications are discussed.