Abstract
This paper develops wave-optics simulations which explore the estimation accuracy of digital-holo- graphic 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.
Cite
CITATION STYLE
Spencer, M. F., Raynor, R. A., Banet, M. T., & Marker, D. K. (2016). Deep-turbulence wavefront sensing using digital-holographic detection in the off-axis image plane recording geometry. Optical Engineering, 56(3), 031213. https://doi.org/10.1117/1.oe.56.3.031213
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