Paper
1 October 1990 Self-imaging technique for focusing an IR telescope
Paul Jennison, Loris G. Gregoris, Edward J. Kristufek
Author Affiliations +
Abstract
A method has been developed, whereby the optimum focus of an IR telescope may be determined utilizing self imaging. A set of gold-bars, located adjacent to an array of detectors within a cooled focal plane, are reimaged and scanned across the detector array. The respective spatial and temporal frequencies of the gold bars and external scan mirror are selected to maximize the response of the sensor electronics. The resulting response to this cooled periodic stimulus is Fourier transformed and stored in memory for each location of the focal plane. The optimum focus is determined to be the position where maximum power at the stimulating frequency was obtained.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paul Jennison, Loris G. Gregoris, and Edward J. Kristufek "Self-imaging technique for focusing an IR telescope", Proc. SPIE 1309, Infrared Imaging Systems: Design, Analysis, Modeling, and Testing, (1 October 1990); https://doi.org/10.1117/12.21777
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Sensors

Mirrors

Spatial frequencies

Telescopes

Gold

Modulation transfer functions

Systems modeling

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