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Active image restoration with a flexible mirrorThe 30 by 5 cm aperture telescope described uses six moveable mirrors to compensate for phase distortions induced by the atmosphere. A feedback system is used to adjust the mirrors in real time to maximize the intensity of light passing through a narrow slit in the image plane. Using the telescope, diffraction-limited images of objects were obtained, using both laser and white light, through 250 meters of turbulent atmosphere.
Document ID
19770041865
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Buffington, A.
(California Univ. Berkeley, CA, United States)
Crawford, F. S.
(California Univ. Berkeley, CA, United States)
Muller, R. A.
(California Univ. Berkeley, CA, United States)
Schwemin, A. J.
(California Univ. Berkeley, CA, United States)
Smits, R. G.
(California, University Berkeley, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1976
Subject Category
Astronomy
Meeting Information
Meeting: Seminar on Imaging through the atmosphere
Location: Reston, VA
Start Date: March 22, 1976
End Date: March 23, 1976
Accession Number
77A24717
Funding Number(s)
CONTRACT_GRANT: NGR-05-003-553
Distribution Limits
Public
Copyright
Other

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