Open Access
31 October 2016 Deep-turbulence wavefront sensing using digital-holographic detection in the off-axis image plane recording geometry
Author Affiliations +
Abstract
This paper develops wave-optics simulations which explore the estimation accuracy of digital-holographic detection for wavefront sensing in the presence of distributed-volume or “deep” turbulence and detection noise. Specifically, the analysis models spherical-wave propagation through varying deep-turbulence conditions along a horizontal propagation path and formulates the field-estimated Strehl ratio as a function of the diffraction-limited sampling quotient and signal-to-noise ratio. Such results will allow the reader to assess the number of pixels, pixel field of view, pixel-well depth, and read-noise standard deviation needed from a focal-plane array when using digital-holographic detection in the off-axis image plane recording geometry for deep-turbulence wavefront sensing.
CC BY: © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
Mark F. Spencer, Robert A. Raynor, Matthias T. Banet, and Dan K. Marker "Deep-turbulence wavefront sensing using digital-holographic detection in the off-axis image plane recording geometry," Optical Engineering 56(3), 031213 (31 October 2016). https://doi.org/10.1117/1.OE.56.3.031213
Published: 31 October 2016
Lens.org Logo
CITATIONS
Cited by 59 scholarly publications and 3 patents.
Advertisement
Advertisement
KEYWORDS
Signal to noise ratio

Staring arrays

Wavefront sensors

Digital holography

Digital recording

Holograms

Optical engineering

RELATED CONTENT


Back to Top