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Simulation of anisoplanatic lucky look imaging and statistics through optical turbulence using numerical wave propagation
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This paper investigates anisoplanatic numerical wave simulation in the
context of lucky look imaging. We demonstrate that numerical wave
propagation can produce root mean square (RMS) wavefront distributions
and probability of lucky look (PLL) statistics that are consistent
with Kolmogorov theory. However, the simulated RMS statistics are
sensitive to the sampling parameters used in the propagation window.
To address this, we propose and validate a new sample spacing rule
based on the point source bandwidth used in the propagation and the
level of atmospheric turbulence. We use the tuned simulator to
parameterize the wavefront RMS probability density function as a
function of turbulence strength. The fully parameterized RMS
distribution model is used to provide a way to accurately predict the
PLL for a range of turbulence strengths. We also propose and validate
a new parametric average lucky look optical transfer function (OTF)
model that could be used to aid in image restoration. Our OTF model
blends the theoretical diffraction-limited OTF and the average
turbulence short exposure OTF. Finally, we show simulated images for
several anisoplanatic imaging scenarios that reveal the spatially
varying nature of the RMS values impacting local image quality.
Title: Simulation of anisoplanatic lucky look imaging and statistics through optical turbulence using numerical wave propagation
Description:
This paper investigates anisoplanatic numerical wave simulation in the
context of lucky look imaging.
We demonstrate that numerical wave
propagation can produce root mean square (RMS) wavefront distributions
and probability of lucky look (PLL) statistics that are consistent
with Kolmogorov theory.
However, the simulated RMS statistics are
sensitive to the sampling parameters used in the propagation window.
To address this, we propose and validate a new sample spacing rule
based on the point source bandwidth used in the propagation and the
level of atmospheric turbulence.
We use the tuned simulator to
parameterize the wavefront RMS probability density function as a
function of turbulence strength.
The fully parameterized RMS
distribution model is used to provide a way to accurately predict the
PLL for a range of turbulence strengths.
We also propose and validate
a new parametric average lucky look optical transfer function (OTF)
model that could be used to aid in image restoration.
Our OTF model
blends the theoretical diffraction-limited OTF and the average
turbulence short exposure OTF.
Finally, we show simulated images for
several anisoplanatic imaging scenarios that reveal the spatially
varying nature of the RMS values impacting local image quality.
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