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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 1, Iss. 4 — Jul. 1, 1962
  • pp: 465–471

Spectral Irradiance from Stars and Planets, above the Atmosphere, from 0.1 to 100.0 Microns

R. C. Ramsey  »View Author Affiliations


Applied Optics, Vol. 1, Issue 4, pp. 465-471 (1962)
http://dx.doi.org/10.1364/AO.1.000465


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Abstract

Using published data on star irradiances in the visible region and assuming a blackbody distribution of energy, irradiances from stars and planets are calculated over the spectral region of 0.1 to 100 microns. Results are presented in chart form for ready application in the design of viewing systems operating in space.

© 1962 Optical Society of America

History
Original Manuscript: October 1, 1961
Published: July 1, 1962

Citation
R. C. Ramsey, "Spectral Irradiance from Stars and Planets, above the Atmosphere, from 0.1 to 100.0 Microns," Appl. Opt. 1, 465-471 (1962)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-1-4-465


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References

  1. L. Larmore, “Infrared Radiation from Celestial Bodies,” U.S. Air Force Project, Rand Research Memorandum, 293-1 (17March1952).
  2. Smithsonian Physical Tables (Smithsonian Institution, Washington, D.C., 1954), 9th revised ed.
  3. H. N. Russell, R. S. Dugan, J. Q. Stewart, Astronomy (Ginn, New York, 1945), Vols. I and II.
  4. M. R. Krasno, private communication.
  5. Handbuch der Physik, S. Flügge, ed. (Springer-Verlag, Berlin, 1957), Vol. 48. [CrossRef]
  6. J. Stebbins, A. E. Whitford, Astrophys. J. 102, 318 (1945). [CrossRef]
  7. F. F. Hall, C. V. Stanley, Appl. Opt. 1, 97 (1962). [CrossRef]
  8. C. W. Allen, Astrophysical Quantities (Athlone Press, Univ. of London, 1955).

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