Noninvasive examinations of human patients and art objects share more than the important modus operandi of ‘do no harm.’ Soon after medical x-rays were discovered, they were applied to inspect the underlying layers of paintings. More recently, that extended to the newer modality of x-ray tomography. Now, optical coherence tomography (OCT), which acquires and processes optical signals to produce high-quality 3D images, has entered the picture. Medical OCT was first described in 1991,1 and reports of its use to examine artwork2–4 emerged in 2004. OCT uses low-coherence interferometry, a tool to study lightwave properties, to determine the distance to the scattering center in an object that moderately absorbs light. The light source’s spectral width determines the localization precision: IR broadband light sources spanning 200nm allow for better than 2μm axial resolution. While this is still less than in phase interferometry, the result is free of the phase-ambiguity disadvantages that limit the height difference between two adjacent data points. The most popular interferometer configuration is Michelson’s type (see Figure 1), in which scattering-center positions are recovered from interference-fringe frequencies superimposed on the light sources’ spectra. In our conservation experiment, we used a home-grown instrument5 with 4μm axial resolution at a central wavelength of λ = 850nm, shown in Figure 1. The results were obtained with two CCD linear cameras: an Action Research 2048-pixel, 12-bit resolution model and a Dalsa Corp. 1024-pixel, 8-bit resolution, high-transfer camera. The former is used when high sensitivity and imaging depth are required, and the latter for fast, real-time imaging (two frames of 400 lines per second) for monitoring conservation treatments. An interesting example of a process requiring online monitoring is laser ablation to remove varnish.6 If varnish is dull or Figure 1. Experimental laser/interferometer artwork-conservation treatment setup. The optical isolator (OI) is inserted between the light source (LS) and the fiber coupler (FC) to protect the former from reflected light. Light passes through the coupler and then propagates in the interferometer’s reference and object arms. In the reference arm (top right), it passes through the polarization controller (PC), a neutraldensity filter (NDF), the dispersion compensator (DC), and is then back-reflected by the stationary reference mirror (RM). In the object arm, comprised of transversal scanners (X-Y) and a lens, the light beam is scanned across the object and then backscatters. The returning light from both arms is collected and then analyzed using a spectrometer consisting of the spectrograph lens (SL), diffraction grating (DG), CCD linear camera, and a personal computer (COMP).
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