Abstract

Many error sources can affect the accuracy of displacement measuring interferometer systems. In heterodyne interferometry two laser source frequencies constitute the finally detected wavefront. When the wavefronts of these source frequencies are non-ideal and one of them walks off the detector, the shape of the detected wavefront will vary. This leads to a change in measured phase at the detector resulting in increased measurement uncertainty. A new wavefront measurement tool described in this publication measures the relative phase difference between the two wavefronts of the two source frequencies of a coaxial heterodyne laser source as used in commercial heterodyne interferometer systems. The proposed measurement method uses standard commercial optics and operates with the same phase measurement equipment that is normally used for heterodyne displacement interferometry. In the presented method a bare tip of a multimode fiber represents the receiving detection aperture and is used for locally sampling the wavefront during a line scan. The difference in phase between the beating frequency of the scanning fiber and a reference beating frequency that results from integration over the entire beam, is used for the reconstruction of the wavefront. The method shows to have a phase resolution in the order of ~25 pm or ~λ/25000 for λ 632.8 nm, and a spatial resolution of ~60 µm at a repeatability better than 1 nm over one week.

Highlights

  • Laser interferometry is applied for a wide range of measurement applications in the fields of high precision position sensing: measuring displacements of precision stages [1,2], gravitational wave detection in the LIGO [3] and LISA [4,5] projects, atomic force microscopy [6] and measuring orbital angular momentum of photons [7]

  • In this article we describe a new and easy to implement measurement tool that uses standard commercial optics and phase measurement equipment that is normally used for heterodyne displacement interferometry

  • The repeatability after 5 minutes is on the order of 0.8 nm and after a week 0.82 nm. These results show that the measurement method has a high repeatability and it shows that the laser source has a high relative wavefront stability between the wavefronts of frequency f1 and f2

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Summary

Introduction

Laser interferometry is applied for a wide range of measurement applications in the fields of high precision position sensing: measuring displacements of precision stages [1,2], gravitational wave detection in the LIGO [3] and LISA [4,5] projects, atomic force microscopy [6] and measuring orbital angular momentum of photons [7]. Wavefront deformations consist of phase differences throughout the cross-section of a laser beam and are caused by: a) the laser source, b) refractive index variations and c) reflective surfaces Such wavefront deformations can be multiple nanometers large and are potentially a problem when sub-nm displacement uncertainty is to be obtained. The main group of wavefront sensors is based upon the ‘Shack Hartmann’ principle, having a micro lens array that focuses onto a CCD This method is able to measure the absolute wavefront topology of the whole cross-section of a beam in a single measurement but is sensitive for tip/tilt alignment. In this group of sensors a trade-off is seen between high phase resolution versus high spatial resolution which is limited by the size of the lenslet-array and the number of lenses. Optimal choice in measurement concept will depend on more specific application needs

Wavefront measurement system
Relative wavefront measurements
Results
Measurement limitations and improvements
Conclusions
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