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Black Bodies in the Extreme Infra-Red

C. Hawley Cartwright

  • California Institute, Pasadena

Phys. Rev. 35, 415 – Published 15 February, 1930

DOI: https://doi.org/10.1103/PhysRev.35.415

Abstract

Absorbing power of various materials of wave-lengths greater than 50μ—For blackening a receiver of a thermocouple for radiation for obtaining pure rotation band spectra, it is desirable to use a material that is an efficient absorber of the extreme infra-red but a poor absorber of radiation of shorter wave-lengths. The absorbing power of 25 materials were tested for radiation of wave-lengths near 4μ and greater than 50μ. Of all the materials tested, white lead, litharge, red phosphorus, powdered glass, copper sulphide, and celestite were found the best for covering a receiver to absorb the extreme infa-red radiation. The 25 materials were tested by painting them on a receiver of a thermocouple which was exposed to extreme infra-red radiation. The same receiver and thermocouple were used throughout the experiment. A D'Arsonval type galvanometer was improved by using a quartz suspension and replacing each conducting lead with silver leaf or gold plated silver ribbon 1μ thick wound in a spiral.

Glass as a source of extreme infra-red radiation.—Hot glass made a good source of extreme infra-red radiation when used with a cold thin glass shutter.

References (6)

  1. L. L. Holladay, J.O.S.A. 17, 333 (1928)
  2. G. Hettner, Zeits. f. Physik 47, 499 (1928)
  3. Paul S. Epstein, Zeits. f. Physik 54, 537 (1929)
  4. Edison Pettit, Astrophys. J. 61, 163 (1926)
  5. W. W. Coblentz, B. S. Bull. 2-3, 462 (1906)
  6. Badger and Cartwright, Phys. Rev. 33, 696 (1929)

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