2016
DOI: 10.1117/1.oe.55.9.094108
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Technique for measuring the three-dimensional shapes of telescope mirrors

Abstract: Abstract. Telescope mirrors determine the imaging quality and the observation ability of the telescopes. Unfortunately, manufacturing highly accurate mirrors remains a bottleneck problem in space optics. One primary cause is the lack of a technique to robustly measure the three-dimensional (3-D) shapes of mirrors for inverse engineering. After centuries of study, researchers developed different techniques for testing the quality of telescope mirrors and proposed different methods for measuring the 3-D shapes o… Show more

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Cited by 4 publications
(2 citation statements)
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References 23 publications
(29 reference statements)
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“…Since the distance D between the projection center and the orthogonal interception plane is unknown, the following algorithm is used to compute it [23][24].…”
Section: Pattern Registrationmentioning
confidence: 99%
“…Since the distance D between the projection center and the orthogonal interception plane is unknown, the following algorithm is used to compute it [23][24].…”
Section: Pattern Registrationmentioning
confidence: 99%
“…The top ten downloaded papers addressed laser space debris removal, 1 hyperspectral camera design, 2 satellite optical downlinks, 3 freeform optics, 4 ultrasonic nondestructive evaluation, 5,6 microwave photonics, 7 optical-wireless networking, 8 and telescope mirror metrology. 9 The tenth on the list was actually my July editorial on performing excellent peer reviews. I am still not certain anyone actually reads my editorials, but this confirms that at least some are downloaded.…”
mentioning
confidence: 99%