Abstract
We investigate the expression of non-Kolmogorov turbulence in terms of Zernike polynomials. Increasing the power-law exponent of the three-dimensional phase power spectrum from 2 to 4 results in a higher proportion of wave-front energy being contained in the tilt components. Closed-form expressions are given for the variances of the Zernike coefficients in this range. For exponents greater than 4 a von Kármán spectrum is used to compute the variances numerically as a function of exponent for different outer-scale lengths. We find in this range that the Zernike-coefficient variances depend more strongly on outer scale than on exponent and that longer outer-scale lengths lead to more energy in the tilt terms. The scaling of Zernike-coefficient variances with pupil diameter is an explicit function of the exponent.
| Original language | English |
|---|---|
| Pages (from-to) | 517-522 |
| Number of pages | 6 |
| Journal | Journal of the Optical Society of America A: Optics and Image Science, and Vision |
| Volume | 13 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - Mar 1996 |
| Externally published | Yes |
Keywords
- Adaptive optics
- Atmospheric turbulence
- Non-Kolmogorov
- Zernike polynomials
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