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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 34, Iss. 24 — Aug. 20, 1995
  • pp: 5268–5277

Multiplex Fabry–Perot interferometer: II. Laboratory prototype

Hilary E. Snell, William B. Cook, and Paul B. Hays  »View Author Affiliations


Applied Optics, Vol. 34, Issue 24, pp. 5268-5277 (1995)
http://dx.doi.org/10.1364/AO.34.005268


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Abstract

The Multiplex Fabry–Perot interferometer (MFPI) consists of a Fabry–Perot interferometer in which the étalon plate separation is changed over a large optical distance. Fourier transformation of the resultant interferogram allows one to treat the multiple reflections within the étalon cavity in a manner analogous to an array of Michelson-type interferometers. However, the scan distance required by the MFPI is much less than for a comparable Michelson. The design and construction of the MFPI are described. Solar absorption spectra measured with this instrument are compared with results from the FASCODE atmospheric model.

© 1995 Optical Society of America

History
Original Manuscript: August 10, 1994
Revised Manuscript: March 29, 1995
Published: August 20, 1995

Citation
Hilary E. Snell, William B. Cook, and Paul B. Hays, "Multiplex Fabry–Perot interferometer: II. Laboratory prototype," Appl. Opt. 34, 5268-5277 (1995)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-34-24-5268


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References

  1. W. B. Cook, H. E. Snell, P. B. Hays, “Multiplex Fabry–Perot interferometer: I. Theory,” Appl. Opt. 34, 5263–5267 (1995). [CrossRef] [PubMed]
  2. H. E. Snell, “Development of a multiplex Fabry–Perot interferometer and measurement of atmospheric HF and HCl,” Ph.D. dissertation (University of Michigan, Ann Arbor, Michigan, 1994).
  3. The mention of brand names in this paper is for information purposes only and does not constitute an endorsement of the products by the authors or their institutions.
  4. J. V. Ramsay, “Automatic control of the spacing of Fabry–Perot interferometers,” Appl. Opt. 5, 1297–1301 (1966). [CrossRef] [PubMed]
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  6. P. B. Hays, V. J. Abreu, M. E. Dobbs, D. A. Gell, H. J. Grassl, W. R. Skinner, “The high-resolution Doppler imager on the upper atmosphere research satellite,” J. Geophys. Res. 98, 10713–10723 (1993). [CrossRef]
  7. G. Guelachvili, “Distortions in Fourier spectra and diagnosis,” in Spectrophotometric Techniques, G. A. Vanasse, ed. (Academic, New York, 1981), Chap. 1, pp. 1–10.
  8. S. A. Clough, F. X. Kneizys, L. S. Rothman, W. O. Gallery, “Atmospheric spectral transmittance and radiance: FASCOD1B,” in Atmospheric Transmission, R. W. Fenn, Proc. Soc. Photo-Opt. Instrum. Eng.277, 152–166 (1981).
  9. S. A. Clough, F. X. Kneizys, E. P. Shettle, G. P. Anderson, “Atmospheric spectral transmittance and radiance: FASCOD2,” in Proceedings of the Sixth Conference on Atmospheric Radiation (American Meteorological Society, Boston, Mass., 1986) pp. 141–144.
  10. R. J. Bell, Introductory Fourier Transform Spectroscopy (Academic, New York, 1972), Chap. 12, pp. 159–166.

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