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Journal of the Optical Society of America

Journal of the Optical Society of America

  • Vol. 67, Iss. 12 — Dec. 1, 1977
  • pp: 1680–1685

Measurement of the atmospheric correlation scale

M. G. Miller and P. L. Zieske  »View Author Affiliations


JOSA, Vol. 67, Issue 12, pp. 1680-1685 (1977)
http://dx.doi.org/10.1364/JOSA.67.001680


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Abstract

A variable-frequency, spinning reticle photometer has been used to measure the spatial-frequency modulation of stellar images in the Cassegrain focal plane of a 1.22 m telescope at the AMOS observatory atop Haleakala on the island Maui, Hawaii. This data, processed in real time, provides information on the statistical properties of the image size which, in turn, yields an estimate of the atmospheric correlation scale ro. Data was collected on 24 nights over a period of eight months. Values of ro ranged from 5.3 to 17.8 cm with a mean value of 9.6 cm at 5000 Å. A variety of temporal behavior was also observed.

© 1978 Optical Society of America

Citation
M. G. Miller and P. L. Zieske, "Measurement of the atmospheric correlation scale," J. Opt. Soc. Am. 67, 1680-1685 (1977)
http://www.opticsinfobase.org/josa/abstract.cfm?URI=josa-67-12-1680


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References

  1. R. E. Hufnagel and N. R. Stanley, "Modulation transfer function associated with image transmission through turbulent media, " J. Opt. Soc. Am. 54, 52–61 (1964).
  2. D. L. Fried, "Optical Resolution through a randomly inhomogeneous medium for very long and very short exposures," J. Opt. Soc. Am. 56, 1372–1379 (1966).
  3. D. Korff, "Analysis of a method for obtaining near-diffraction- limited information in the presence of atmospheric turbulence," J. Opt. Soc. Am. 63, 971–980 (1973).
  4. See, for example, R. A. Muller, and A. Buffington, "Realtime correction of atmospherically degraded telescope images through image sharpening, " J. Opt. Soc. Am. 64, 1200–1210 (1974).
  5. C. R. Giuliano, J. A. Jenney, L. Miller, M. E. Pedinoff, D. Y. Tseng, and S. M. Wandzura, "Space Object Imaging," Technical Report No. RADC-TR-76-54 (Rome Air Development Center, Griffiss AFB, New York, 1976), p. 21.
  6. M. Miller, P. Zieske and D. Hanson, "Characterization of Atmospheric Turbulence, " Proc. Soc. Photo-Opt. Instrum. Eng. 75, 30 (1976).
  7. D. P. Karo and A. M. Schneiderman, "Speckle interferometry lens-atmosphere MTF measurements, " J. Opt. Soc. Am. 66, 1252 (1976), and private communication.
  8. A. Papoulis, Probability, Random Variables and Stochastic Processes (McGraw-Hill, New York, 1965), p. 245.
  9. M. G. Miller and P. L. Zieske, "Turbulence Characterization and Control, " Technical Report No. RADC-TR-77-70 (Rome Air Development Center, Griffiss AFB, New York, 1977), p. 18.
  10. The data taken during the period 11 November 1975 to 8 December 1975 have been reported previously (Ref. 6). They are included here in order to provide a better estimate of the long-term statistics.
  11. M. G. Miller and P. Kellen, "Astronomical Differential Angle of Arrival Measurements, " Proceedings of the AAS/SAO/OSA/SPIE Topical Meeting on Imaging in Astronomy, Cambridge, Mass., 1975, Paper WB-3.
  12. D. Kelsall, "Optical seeing through the atmosphere by an interferometric technique," J. Opt. Soc. Am. 63, 1472 (1973).
  13. J. C. Dainty and R. J. Scadden, "Measurements of the Atmospheric Transfer Function at Mauna Kea, Hawaii," Mon. Not. R. Astr. Soc. 170, 519 (1975).
  14. D. L. Fried and G. E. Mevers, "Evaluation of ro for Propagation Down through the Atmosphere, " Appl. Opt. 13, 2620 (1974). Several numerical corrections to these results are given by D. L. Fried, Appl. Opt. 14, 2567 (1975); ibid. 16, 549 (1977).
  15. D. Korff, G. Dryden, and M. G. Miller, "Information Retrieval from Atmospheric Induced Speckle Patterns, " Opt. Commun. 5, 187 (1972).
  16. D. Karo and A. Schneiderman, "Nonstationarity of the atmospheric transfer function, " J. Opt. Soc. Am. 66, 1065A (1976).

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