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article · Optics Letters · 1995

Strehl ratio and visibility in long-baseline stellar interferometry

Theo A. ten Brummelaar, Stephen T. Ridgway, W. G. Bagnuolo

Cited by 14Abstract and details only

Abstract

The relationship between Strehl ratio (S), the parameter most often used by those in the adaptive optics field, and visibility (V), the parameter of most interest to those working in interferometry, is investigated. It is found that if the atmospheric turbulence is assumed to be Kolmogorov, V approximately S for high Strehl ratios. At low Strehl ratios, both simulations and an analytical formulation show that the Strehl ratio underestimates the visibility.

Cite this paper

APA 7

ten Brummelaar, T. A., Ridgway, S. T., & Bagnuolo, W. G. (1995). Strehl ratio and visibility in long-baseline stellar interferometry. Optics Letters, 20(6), 521. https://doi.org/10.1364/ol.20.000521

MLA 9

ten Brummelaar, Theo A., et al. “Strehl ratio and visibility in long-baseline stellar interferometry.” Optics Letters, vol. 20, no. 6, 1995, p. 521, https://doi.org/10.1364/ol.20.000521.

Chicago

ten Brummelaar, Theo A., Stephen T. Ridgway, and W. G. Bagnuolo. 1995. “Strehl ratio and visibility in long-baseline stellar interferometry.” Optics Letters 20 (6): 521. https://doi.org/10.1364/ol.20.000521.

Harvard

ten Brummelaar, T.A., Ridgway, S.T. and Bagnuolo, W.G. (1995) ‘Strehl ratio and visibility in long-baseline stellar interferometry’, Optics Letters, 20(6), p. 521. Available at: https://doi.org/10.1364/ol.20.000521.

BibTeX
@article{tenbrummelaar1995strehl,
  title = {{Strehl ratio and visibility in long-baseline stellar interferometry}},
  author = {ten Brummelaar, Theo A. and Ridgway, Stephen T. and Bagnuolo, W. G.},
  journal = {Optics Letters},
  volume = {20},
  number = {6},
  pages = {521},
  year = {1995},
  doi = {10.1364/ol.20.000521}
}

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