Paper
22 April 1988 Laboratory Wavefront Sensor For Speckle Image Enhancement
Steven Krausman, Andy Jankevics, Larry Schmutz
Author Affiliations +
Proceedings Volume 0739, Phase Conjugation, Beam Combining, and Diagnostics; (1988) https://doi.org/10.1117/12.939714
Event: OE LASE'87 and EO Imaging Symposium, 1987, Los Angeles, CA, United States
Abstract
A small low speed wavefront sensor has been built for Harvard Smithsonian Observatory for astronomical observing. The sensor measures wavefronts using a small lenslet array to focus light as spots on a detector array. The position of these spots are used to measure the wavefront distortion. The detector array output is digitized and processed by a high speed image processor. The processor outputs the directional derivatives of the wavefront in the X and Y directions.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Steven Krausman, Andy Jankevics, and Larry Schmutz "Laboratory Wavefront Sensor For Speckle Image Enhancement", Proc. SPIE 0739, Phase Conjugation, Beam Combining, and Diagnostics, (22 April 1988); https://doi.org/10.1117/12.939714
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Wavefronts

Image processing

Telescopes

Wavefront sensors

Clocks

Detector arrays

Back to Top