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NASA NTRS · 20150005915

Phase-Shifting Zernike Interferometer Wavefront Sensor

Abstract

The canonical Zernike phase-contrast technique transforms a phase object in one plane into an intensity object in the conjugate plane. This is done by applying a static pi/2 phase shift to the central core (approx. lambda/diameter) of the PSF which is intermediate between the input and output plane. Here we present a new architecture for this sensor. First, the optical system is simple and all reflective, and second the phase shift in the central core of the PSF is dynamic and can be made arbitrarily large. This common-path, all-reflective design makes it minimally sensitive to vibration, polarization and wavelength. We review the theory of operation, describe the optical system, summarize numerical simulations and sensitivities and review results from a laboratory demonstration of this novel instrument.

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BibTeXRIS

Wallace, J. Kent, Rao, Shanti, Jensen-Clem, Rebecca M.. 2011-08-01. Phase-Shifting Zernike Interferometer Wavefront Sensor. https://ntrs.nasa.gov/citations/20150005915

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