Paper
1 August 1992 Effects of predetection atmospheric compensation and post-detection image processing on imagery collected at a ground-based telescope
Marsha F. Bilmont, Michael C. Roggemann, David W. Tyler, Mark A. Von Bokern, John P. Albetski
Author Affiliations +
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.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Marsha F. Bilmont, Michael C. Roggemann, David W. Tyler, Mark A. Von Bokern, and John P. Albetski "Effects of predetection atmospheric compensation and post-detection image processing on imagery collected at a ground-based telescope", Proc. SPIE 1688, Atmospheric Propagation and Remote Sensing, (1 August 1992); https://doi.org/10.1117/12.137917
Lens.org Logo
CITATIONS
Cited by 5 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Telescopes

Spatial frequencies

Speckle

Wavefront sensors

Imaging systems

Atmospheric turbulence

Back to Top