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25 September 2017 Sensitivity analysis of phase diversity technique for high resolution earth observing telescopes
Ch. Latry, J. M. Delvit, C. Thiebaut
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Proceedings Volume 10562, International Conference on Space Optics — ICSO 2016; 105623X (2017) https://doi.org/10.1117/12.2296051
Event: International Conference on Space Optics — ICSO 2016, 2016, Biarritz, France
Abstract
Earth observing systems resolution is directly linked to the telescope diameter through the diffraction. Getting close to a diffraction limited telescope means low level aberrations, with a typical threshold value of ?/30 for the Wave Front Error (WFE) value.
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Ch. Latry, J. M. Delvit, and C. Thiebaut "Sensitivity analysis of phase diversity technique for high resolution earth observing telescopes", Proc. SPIE 10562, International Conference on Space Optics — ICSO 2016, 105623X (25 September 2017); https://doi.org/10.1117/12.2296051
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KEYWORDS
Telescopes
Active optics
Space telescopes
Satellites
Astronomical imaging
Mirrors
Modulation transfer functions
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