English

A generalized approach to compensate for low and high frequency errors in FFT based phase screen simulations

Instrumentation and Methods for Astrophysics 2021-06-03 v1 Atmospheric and Oceanic Physics

Abstract

Fast Fourier Transform based phase screen simulations give accurate results only when the screen size (GG) is much larger than the outer scale parameter (L0L_0). Otherwise, they fall short in correctly predicting both the low and high frequency behaviours of turbulence induced phase distortions. Sub-harmonic compensation is a commonly used technique that aids in low-frequency correction but does not solve the problem for all values of screen size to outer scale parameter ratios (G/L0(G/L_0). A subharmonics based approach will lead to unequal sampling or weights calculation for subharmonics addition at the low-frequency range and patch normalization factor. We have modified the subharmonics based approach by introducing a Gaussian phase autocorrelation matrix that compensates for these shortfalls. We show that the maximum relative error in structure function with respect to theoretical value is as small as 0.5-3% for (G/L0(G/L_0) ratio of 1/1000 even for screen sizes up to 100 m diameter.

Keywords

Cite

@article{arxiv.2106.01002,
  title  = {A generalized approach to compensate for low and high frequency errors in FFT based phase screen simulations},
  author = {Sorabh Chhabra and Jyotirmay Paul and Anamparambu N. Ramaprakash and Avinash Surendran},
  journal= {arXiv preprint arXiv:2106.01002},
  year   = {2021}
}

Comments

23 pages, 12 figures, 1 table, Accepted for Publication in JATIS (SPIE)

R2 v1 2026-06-24T02:44:29.442Z