Abstract
Both radial errors with different spatial frequencies and local errors with different aperture sizes were fitted using Zernike polynomials. Householder transformation method was applied to work out Zernike coefficients, getting the RMS value of fitting errors. The limitation of Zernike polynomials was analyzed. The results showed that the maximum spatial frequency limits the fitting accuracy of radial errors, and the aperture size limits the fitting accuracy of local errors, generating extra ripples.
| Original language | English |
|---|---|
| Pages (from-to) | 675-678 |
| Number of pages | 4 |
| Journal | Guangxue Jishu/Optical Technique |
| Volume | 31 |
| Issue number | 5 |
| State | Published - Sep 2005 |
Keywords
- Local errors
- Radial errors
- Wavefront fitting
- Zernike polynomials
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