Stratospheric fluctuations in the FIR

Details Stratospheric fluctuations in the FIR Stratospheric fluctuations in the FIR

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984infph..24....7d&link_type=abstract

Infrared Physics (ISSN 0020-0891), vol. 24, Jan. 1984, p. 7-10. Research supported by the Consiglio Nazionale delle Ricerche.

Computer Science

Sound

Background Noise, Far Infrared Radiation, Infrared Astronomy, Millimeter Waves, Stratosphere Radiation, Atmospheric Sounding, Balloon Sounding, Cassegrain Optics, Emissivity, Infrared Detectors, Low Noise

Scientific paper

The fluctuations in the stratospheric emission in the 800-2000-micron wavelength range have been studied by means of a special correlator operating at 0.3 K. The observed noise is about three times larger than expected from a grey body at a temperature of 250 K and an emissivity of 0.0005. This fact has been interpreted as proof that about 2 percent of the stratospheric lines were saturated.

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