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Proceedings Paper

Effects of predetection atmospheric compensation and postdetection image processing on imagery collected at a ground-based telescope
Author(s): Marsha F. Bilmont; Michael C. Roggemann; David W. Tyler; Mark A. Von Bokern; John P. Albetski
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Paper Abstract

Short exposure imagery of single and binary stars was collected at the 1.6-m Air Force Maui Optical Station (AMOS) telescope, using a low-noise CCD camera. Atmospheric turbulence effects were partially mitigated using the Compensated Imaging System (CIS), a predetection wavefront sensor and deformable mirror adaptive optical system. We present images and power spectra from both partially compensated and uncompensated short exposure simulations and field data. Our results illustrate that the use of lower-cost partially compensating adaptive optical systems combined with post-detection processing provides a viable alternative to expensive, fully compensated adaptive imaging systems for achieving high-resolution imagery through the atmosphere.

Paper Details

Date Published: 1 August 1992
PDF: 12 pages
Proc. SPIE 1688, Atmospheric Propagation and Remote Sensing, (1 August 1992); doi: 10.1117/12.137917
Show Author Affiliations
Marsha F. Bilmont, Air Force Phillips Lab. (United States)
Michael C. Roggemann, Air Force Phillips Lab. (United States)
David W. Tyler, Air Force Phillips Lab. (United States)
Mark A. Von Bokern, Air Force Phillips Lab. (United States)
John P. Albetski, Thermo Electron Technologies Corp. (United States)


Published in SPIE Proceedings Vol. 1688:
Atmospheric Propagation and Remote Sensing
Anton Kohnle; Walter B. Miller, Editor(s)

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