Page 275 - Chalcogenide Glasses for Infrared Optics
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250    Cha pte r  T e n

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              Spitzer and Fan fall almost exactly on the TI measured values. These
              measurements were made using the TI Perkin Elmer 301 grating
              spectrophotometer, standard with a Golay cell detector or using the
              TI liquid helium cooled, gallium doped germanium bolometer.  A
              study was run by TI and PE to compare the sensitivity of the Golay
                                6
              cell to the TI bolometer  that demonstrated the TI bolometer improved
              S/N by a factor of 3. For every wavelength point, k values may be
              calculated. In application of the scan technique, change in intensity of
              the peaks is not the main concern. Only the wavelength location of
              each peak is important.
                 Optical interference occurs, and as the infrared spectrophotometer
              scans from a short wavelength to a longer one, a pattern of maxima
              and minima occurs with the amplitudes depending in part upon the
              ratio of the resistivity of layer to substrate. Often the resistivity ratio
              of layer to substrate was 10 to 20. The scans were generated using the
              double-beam infrared instruments available at that time. Most were
              optical null instruments where the reference beam was matched to
              the intensity of the sample beam by moving a wedge-shaped object
              into the reference beam until the two beams were equal. The wedge
              was linked to the recorder to read 1 to 100 percent For this applica-
              tion, a reflectance attachment was mounted in the sample beam. The
              angle of incidence was fixed at 20° to 30°. An example of such a scan
              is shown in Fig. 10.3. The wavelength of the scan covers from 12 to
              over 30 µm. Notice the spacing of patterns is closer together in the
              shorter wavelengths than in the longer because the order of interfer-
              ence (integer  m) is decreasing as  λ approaches the same order of
              magnitude as d. Many of these instruments made by Beckman Instru-
              ments were purchased by TI and put in service in the production



                 100

                  80
                % reflectivity (relative)  60




                  40


                  20



                    0     4     8    12    16    20    24   28    32
                                       Wavelength (µm)
              FIGURE 10.3  Typical infrared scan epitaxial layer interference pattern.
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