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Reference interferometer

Figure 5.8. Interferometer, incorporating a separate reference interferometer for the laser and white channels. Figure 5.8. Interferometer, incorporating a separate reference interferometer for the laser and white channels.
The mirror position in the stepping mode, and the sampling point in the constant velocity mode, must be accurate to a small fraction of a wavelength. To achieve this accuracy it is customary to employ a second interferometer with a monochromatic source of a wavenumber considerably higher than that of the radiation to be measured. The reference interferometer shares part of the main infrared interferometer... [Pg.225]

Optical interferometry can be used to measure surface features without contact. Light reflected from the surface of interest interferes with light from an optically flat reference surface. Deviations in the fnnge pattern produced by the interference are related to differences in surface height. The interferometer can be moved to quantify the deviations. Lateral resolution is determined by the resolution of the magnification optics. If an imaging array is used, three-dimensional (3D) information can be provided. [Pg.700]

It is conceivable to detect amplitude and phase emitted by a celestial object at various observation sites and to correlate the results in order to create a huge interferometer (Fig. 3). Because laser can be very stable, the phase reference between lasers can be extracted at low data rate for example from the correlation of the interference signal of each laser with a high magnitude star. The main difference with communication case above is that the absolute phase of the thermal emission is meaningless only the phase correlation from site to site can be exploited. Emission of thermal source is governed by the Planck law. This law states that the probability of photon population of a mode is ... [Pg.370]

Er is becoming very small. Here, however, the effect will be masked by other effects contained in the data, such as the effect of small changes in source intensity, external interference or, in the case of FTIR, interferometer misalignment, or any of several other effects that change the actual values of reference and sample energy at the limits of the spectral range. [Pg.246]

Figure 2.50 Potential difference infrared (PDIR) spectra for adsorbed azide at the silver-aqueous interface in the asymmetric N-N-N stretch region. The reference (base) potential was -970 mV vs. SCE sample potentials as indicated. The solution contained 0.01 M NaNj/0.49 M NaCI04. The spectra are the average of 1024 interferometer scans at each potential. From Corrigan and Weaver (1986), Copyright 1986 American Chemical Society. Figure 2.50 Potential difference infrared (PDIR) spectra for adsorbed azide at the silver-aqueous interface in the asymmetric N-N-N stretch region. The reference (base) potential was -970 mV vs. SCE sample potentials as indicated. The solution contained 0.01 M NaNj/0.49 M NaCI04. The spectra are the average of 1024 interferometer scans at each potential. From Corrigan and Weaver (1986), Copyright 1986 American Chemical Society.
Figure 3. Mach-Zehnder interferometer One of the arms is covered by inert material (reference arm), the other arm exposes to the sample (measuring arm). Figure 3. Mach-Zehnder interferometer One of the arms is covered by inert material (reference arm), the other arm exposes to the sample (measuring arm).
The principle of operation of a typical MZI-CCMI sensor is illustrated in Fig. 7.17a, where two mode splitters/combiners (MSC) are created on a singlemode fiber. These two MSCs are separated by a distance of L, which is referred to as the length of the interferometer. The input light, originally guided inside the fiber... [Pg.161]

NaN3 + 0.1 M NaClO. Base (reference) potential was -0.97 V vs. SCE sample potentials (mV vs. SCE) are as indicated. Spectra were obtained by acquiring 1024 interferometer scans at the base and sample potentials, the potential being altered after every 32 scans (see references 7 and 10 for further details). [Pg.306]

Both the GC-MS and GC-IR instruments obviously require that the column effluent be fed into the spectrometer detection path. For the IR instrument, this means that the IR cell, often referred to as a light pipe, be situated just outside the interferometer (Chapter 8) in the path of the light, of course, but it must also have a connection to the GC column and an exit tube where the sample may possibly be collected. The infrared detector is nondestructive. With the mass spectrometer detector, we have the problem of the low pressure of the mass spectrometry unit coupled with the ambient pressure of the GC column outlet. A special method is used to eliminate carrier gas while retaining sufficient amounts of the mixture components so that they are measurable with the mass spectrometer. [Pg.352]

In a Mach-Zehnder interferometer (MZI) device the light from a laser beam is divided into two identical beams that travel the MZI arms (sensor and reference areas) and are recombined again into a monomode channel waveguide giving a signal which is dependent on the phase difference... [Pg.130]


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See also in sourсe #XX -- [ Pg.107 ]

See also in sourсe #XX -- [ Pg.225 , Pg.227 , Pg.294 ]




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Interferometer

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