Measurement of wave-front aberration in a small telescope remote imaging system using scene-based wave-front sensing
Abstract
Reference-free compensated imaging makes an estimation of the Fourier phase of a series of images of a target. The Fourier magnitude of the series of images is obtained by dividing the power spectral density of the series of images by an estimate of the power spectral density of atmospheric turbulence from a series of scene based wave front sensor (SBWFS) measurements of the target. A high-resolution image of the target is recovered from the Fourier phase and the Fourier magnitude.
- Inventors:
- Issue Date:
- Research Org.:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1177024
- Patent Number(s):
- 8995787
- Application Number:
- 13/828,963
- Assignee:
- Lawrence Livermore National Security, LLC (Livermore, CA)
- Patent Classifications (CPCs):
-
G - PHYSICS G06 - COMPUTING G06T - IMAGE DATA PROCESSING OR GENERATION, IN GENERAL
- DOE Contract Number:
- AC52-07NA27344
- Resource Type:
- Patent
- Resource Relation:
- Patent File Date: 2013 Mar 14
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 47 OTHER INSTRUMENTATION
Citation Formats
Poyneer, Lisa A, and Bauman, Brian J. Measurement of wave-front aberration in a small telescope remote imaging system using scene-based wave-front sensing. United States: N. p., 2015.
Web.
Poyneer, Lisa A, & Bauman, Brian J. Measurement of wave-front aberration in a small telescope remote imaging system using scene-based wave-front sensing. United States.
Poyneer, Lisa A, and Bauman, Brian J. Tue .
"Measurement of wave-front aberration in a small telescope remote imaging system using scene-based wave-front sensing". United States. https://www.osti.gov/servlets/purl/1177024.
@article{osti_1177024,
title = {Measurement of wave-front aberration in a small telescope remote imaging system using scene-based wave-front sensing},
author = {Poyneer, Lisa A and Bauman, Brian J},
abstractNote = {Reference-free compensated imaging makes an estimation of the Fourier phase of a series of images of a target. The Fourier magnitude of the series of images is obtained by dividing the power spectral density of the series of images by an estimate of the power spectral density of atmospheric turbulence from a series of scene based wave front sensor (SBWFS) measurements of the target. A high-resolution image of the target is recovered from the Fourier phase and the Fourier magnitude.},
doi = {},
journal = {},
number = ,
volume = ,
place = {United States},
year = {2015},
month = {3}
}
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