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. Author manuscript; available in PMC: 2014 Jan 22.
Published in final edited form as: Proc SPIE Int Soc Opt Eng. 2010 Aug 27;7762:77621T. doi: 10.1117/12.862519

Figure 9.

Figure 9

The correction kinoform calculated from the sum of the individual Zernike polynomials. Encoding this into all subsequent kinoforms effectively removes any aberrations induced from the non-flat SLM or mis-aligned optical train.