White Light Interferometers are devices that use interference effects between light beams. The interference occurs when the light reflected from a sample is superimposed with the light reflected by a high-precision reference mirror. The basic principle behind this method is Michelson interferometry. A broadband white light source is used to illuminate the sample in white light interferometry. The collimated light beam from a coherent light source is split into two beams, a measurement beam and a reference beam using a beam splitter. The measurement beam will hit the sample and the reference beam is the beam that hits the reference mirror. Light reflected from the sample and reference mirror is recombined at the beam splitter and is focused onto a CCD camera. Figure 1 shows the optical setup for white light interferometry.
Figure 1: Setup for White Light Interferometry
If there is any difference in the optical path length (distance travelled by light) between the light reflected from the sample and the reference beam to the camera, interference occurs at the camera. The formed interference pattern is then studied. If the optical path length is same, constructive interference takes place and the camera pixel shows high intensity at those points. For different path lengths, destructive interference occurs and low intensity is shown on camera pixels. The white light interferometers are used for high-precision distance and thickness measurements. Surface roughness can be measured using this method. Color cameras that can split light into red, blue, and green are preferred for this technique. Complex optics are involved in this method.
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