npsm 새물리 New Physics : Sae Mulli

pISSN 0374-4914 eISSN 2289-0041
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Research Paper

New Phys.: Sae Mulli 2018; 68: 1378-1383

Published online December 31, 2018 https://doi.org/10.3938/NPSM.68.1378

Copyright © New Physics: Sae Mulli.

A Phase Unwrapping Algorithm in Three-Wavelength Digital Holographic Microscopy

Sanghoon SHIN1, Younghun YU*2

1 Kanghae Precision System, Hwaseong 18487, Korea
2 Department of Physics and Research Institute for Basic Sciences, Jeju National University, Jeju 63243, Korea

Correspondence to:yyhyoung@jejunu.ac.kr

Received: September 11, 2018; Revised: October 29, 2018; Accepted: October 30, 2018

This is an open-access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/3.0/) which permits unrestricted non-commercial use, distribution, and reproduction in any medium, provided the original work is properly cited.

Multi-wavelength holography has a better axial range than single-wavelength holography, thus allowing unambiguous phase imaging. Noise amplification is the limiting factor in multi-wavelength holography as noise is amplified by a factor equivalent to the magnification of the wavelengths. Here, we propose a new algorithm to remove noise amplification in multi-wavelength holography. The proposed method does not use phase unwrapping and removes 2$\pi$ ambiguities. Experiments and numerical simulations indicated that the proposed method is fast, has low noise, and is useful for measuring samples with arbitrary step heights.

Keywords: Digital holography, Three-wavelength holography, Noise reduction

Fig. 1. The phase maps of beat wavelengths and profiles. (a), (b) Phase map of λ12 and λ23, (c) phase map of λ123, (d) the unwrapped phase map with ϕ12, and (e) profiles of dotted lines in Figs. 5(c) and (d).

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