Abstract

Non-contact optical detection of ultrasound critically depends on the amount of light collected from the detection surface. Although it can be optimized in multiple ways for an ideal flat polished surface, industrial non-destructive testing and evaluation (NDT&E) usually requires optical detectors to be robust for unpolished material surfaces that are usually rough and curved. Confocal detectors provide the best light collection but must trade off sensitivity with depth of field. Specifically, detection efficiency increases with the numerical aperture (NA) of the detector, but the depth of field drops. Therefore, fast realignment of the detector focal point is critical for in-field applications. Here, we propose an optical distance and angle correction system (DACS) and demonstrate it in a kHz-rate laser-ultrasound inspection system. It incorporates a Sagnac interferometer on receive for the fast scanning of aircraft composites, which minimizes the required initial alignment. We show that DACS performs stably for different composite surfaces while providing ±2° angular and ±2 mm axial automatic correction with a maximum 100 ms realignment time.

Highlights

  • Non-contact interferometric methods of ultrasound (US) detection exploit either birefringence induced by US displacement in one of the interferometer arms [1,2] or record the Doppler frequency shift introduced by the surface motion due to the US wave

  • Echo-signals scattered by internal heterogeneities can be recorded at the same spot or at a distance from the pump with the fiber-optic Sagnac interferometer powered by a tiny, low-coherent super-luminescent diode (SLD) source (30 mW power) at 1550 nm wavelength

  • Confocal optical detection trades off sensitivity with depth of field, we have shown here

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Summary

Introduction

Non-contact interferometric methods of ultrasound (US) detection exploit either birefringence induced by US displacement in one of the interferometer arms [1,2] or record the Doppler frequency shift introduced by the surface motion due to the US wave. Interferometers can achieve high sensitivity for optically ideal (polished) surfaces under low-noise laboratory conditions, US signal reception from unpolished material surfaces in noisy industrial facilities remains a challenge. Rough material surfaces create speckle noise and strongly reduce the light collected compared to mirror surfaces. The most efficient way to improve light collection is confocal detection. Speckle limitations can be resolved with speckle inversion using multiple photodetectors [6], photo-refractive crystals [7], or confocal Fabry-Perot [8,9] or Sagnac-type interferometers [10,11,12]

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