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Proceedings Paper

Laboratory Wavefront Sensor For Speckle Image Enhancement
Author(s): Steven Krausman; Andy Jankevics; Larry Schmutz
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Paper 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.

Paper Details

Date Published: 22 April 1988
PDF: 7 pages
Proc. SPIE 0739, Phase Conjugation, Beam Combining, and Diagnostics, (22 April 1988); doi: 10.1117/12.939714
Show Author Affiliations
Steven Krausman, Adaptive Optics Associates (United States)
Andy Jankevics, Adaptive Optics Associates (United States)
Larry Schmutz, Adaptive Optics Associates (United States)

Published in SPIE Proceedings Vol. 0739:
Phase Conjugation, Beam Combining, and Diagnostics
Ira Abramowitz; Robert A. Fisher, Editor(s)

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