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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 13, Iss. 11 — Nov. 1, 1974
  • pp: 2623–2628

Infrared Radiometer for the Pioneer 10 and 11 Missions to Jupiter

M. L. Bender, P. W. Callaway, S. C. Chase, G. F. Moore, and R. D. Ruiz  »View Author Affiliations


Applied Optics, Vol. 13, Issue 11, pp. 2623-2628 (1974)
http://dx.doi.org/10.1364/AO.13.002623


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Abstract

Pioneer 10 has successfully encountered Jupiter and several of its satellites. The two-channel infrared radiometer used to obtain data relating to thermal properties of the planet and its atmosphere is described. The instrument features a body-fixed, 7.62-cm diam aperture Cassegrainian telescope with reststrahlen filters defining the 14-μm to 25-μm and 30-μm to 56-μm bands. Detectors are 88-junction evaporated thin-film thermopiles. Stringent weight constraints of 2 kg dictated all-beryllium construction. Power consumption was 1.2 W.

© 1974 Optical Society of America

History
Original Manuscript: May 9, 1974
Published: November 1, 1974

Citation
M. L. Bender, P. W. Callaway, S. C. Chase, G. F. Moore, and R. D. Ruiz, "Infrared Radiometer for the Pioneer 10 and 11 Missions to Jupiter," Appl. Opt. 13, 2623-2628 (1974)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-13-11-2623


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References

  1. S. C. Chase et al., Science 183 (1974). [PubMed]
  2. K. R. Armstrong et al., Astrophysi. J. 178, L89 1 (1972).
  3. G. Münch, “Probing the Structure and Composition of the Jupiter Atmosphere from Pioneer 10/11,” AIAA/AGU Space Science Conference, Denver, Colo., Paper No. 73-561, 10–12 July 1973.
  4. W. Kaiser et al., Phys. Rev. 127 (1962). [CrossRef]
  5. G. Andermann, E. Duesler, J. Opt. Soc. Am. 60 (1970). [CrossRef]
  6. O. Stafsudd, N. B. Stevens, Appl. Opt. 7, 2320 (1968). [CrossRef] [PubMed]
  7. N. B. Stevens, in Semiconductors and Semimetals, Vol. 5, Infrared Detectors, R. K. Willardson, A. C. Beer, Eds. (Academic Press, New York, 1970), Chap. 7. [CrossRef]

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