To improve the measuring accuracy of optical interferometry
the filtering methods to eliminate the noise in interference fringe patterns were researched. The results of different filtering methods were discussed in different wavefronts and different noises of the interferometer. By taking the effects of interferometric noise on fringe patterns and different wavefronts into account
four kinds of fringe patterns for defocus
astigmatism
coma
spherical aberration were established based on zernike polynomials by matlab simulation. The differences of PV and GRMS values before and after filtering were calculated for different wavefronts. The results on four kinds of wavefronts for defocus
astigmatism
coma
spherical aberration show that under the same kind of noise and filtering
the PV difference of the spherical aberration is largest
up to 0.11λ
which shows a poor filtering effect as compared with the 0.08λ from other wavefront differences under the multiplicative noise. Furthermore
the PV difference of the astigmatism wavefront is smallest
and it is down to 0.05λ excepting median filtering in the multiplicative noise
showing a better filter effect. Moreover
the result of coma wavefront filtering is slightly better than that of the defocus wavefront filtering. For the filter methods
low-pass filters offer high-stability and the differences of the PV is from 0.01λ to 0.04λ
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