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Interferometric Spectroscopy

  • H. A. Gebbie
Conference paper
Part of the Optical Physics and Engineering book series (OPEG)

Abstract

The far infrared region has benefited considerably from the introduction of Fourier Spectroscopy, a topic of which the generalities have now been treated by a number of authors. Basically its advantages come from the ability of a two beam interferometer like Michelson’s to pass a greater amount of information than any other “delay” instrument for a given size and spectral resolution. (1) This is of great importance in a spectral region where source brightness is low. It does, however, demand the additional process of Fourier Transformation to give spectra, but modern digital computers can do this very economically and rapidly to any required resolution.

Keywords

Source Brightness Index Spectrum Fourier Spectroscopy Spectral Background Verification Point 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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    H. A. Gebbie and R.Q. Twiss, Reports on Progress in Physics, 29 Part II. p. 729, 1966.ADSCrossRefGoogle Scholar
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    J. E. Chamberlain, F. D. Finlay and H. A. Gebbie, Applied Optics 4, 1302, 1965.CrossRefGoogle Scholar
  3. J.E. Chamberlain, A. E. Cosltey and H. A. Gebbie, Spectrochemica Alta, 25A, 9, 1969.ADSCrossRefGoogle Scholar
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    New Scientist, 17th October, 1968, Radar for Engineers.Google Scholar
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    J. Chamberlain and H. A. Gebbie; will be submitted to Applied Optics forthcoming issue on Interferometric Spectroscopy.Google Scholar
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    K. J. Button, B. Lax and C. C. Bradley, Phys. Rev. Letters 21, 350, 1968.ADSCrossRefGoogle Scholar

Copyright information

© Plenum Press, New York 1970

Authors and Affiliations

  • H. A. Gebbie
    • 1
    • 2
  1. 1.National Bureau of StandardsBoulderUSA
  2. 2.National Physical LaboratoryTeddingtonEngland

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