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SpectRx NIR Technology
                          apply Eq. (10.17) to the measurements of multiple blackbodies, we   513
                          get the following system of equations:
                                                                  σ
                                                         σ
                                                    σ
                                      L () =  S Measured ()/ K()−  M Stray ()
                                         σ
                                       1     1
                                                    σ
                                         σ
                                                         σ
                                                           −
                                                                  σ
                                                       K
                                      L () =  S 2 Measured ()/ () M Stray ()  (10.43)
                                       2
                                                     M
                                                         σ
                                                           −
                                                                  σ
                                           =
                                         σ
                                                    σ
                                                       K
                                      L  () S Measured ()/ ()− M Stray ()
                                       n      n
                             The preceding equations form a system of linear equations. The
                          general solution to such a system for n equations is as follows:
                                                         ⎛
                                          n∑  Measured () − ∑  Measured  σ  ⎞  2
                                                    σ
                                                      2
                                             S
                                              i          ⎜  i ⎝  S i  () ⎟ ⎠
                                   σ
                                            i
                                 K() =  n∑  Measured  σ  L ()−∑  Measured ()∑  σ  (10.44)
                                                                  σ
                                                     σ
                                          S
                                           i    ()  i      S i        L ()
                                                                       i
                                        i                i           i
                                                           (
                                                                     )
                                   n∑ S  Measured ()∑ S  Measured () L () − ∑ S Measured () ∑ L () ∑ L ()
                                                                      2
                                                        σ
                                                     σ
                                                                          σ
                                           σ
                                                                                  σ
                                                                    σ
                                      i         i      i       i          i      i
                               σ
                           M Stray () =  i    i              i         i     −  i
                                                         (
                                           n ∑ S  Measured () − ∑ S Meeasured () ) 2  n
                                                    σ
                                                                 σ
                                           2
                                                      2
                                                        n
                                               i            i
                                             i            i
                                                                              (10.45)
                             Eqs. (10.25) and (10.26) can be used to solve for systems of equa-
                          tions in the form of Eq. (10.24). In the case illustrated in Fig. 10.14, n
                          equals 5 and i runs from 1 to 5. The calibrated spectrum is then given
                          by Eq. (10.23) as before.
                          10.9.4  Nonlinear Multiple Point Calibrations
                          Nonlinear multiple point calibrations are used to correct for nonlinear-
                          ity in the response function of the FT spectroradiometer, Fig. 10.15.
                                    Scene Spectral Radiance  2  3  4  5  6
                                         1
                                             Spectral Power at Detector
                                            2 point calibration using 1 and 6
                                            Multiple point linear calibration
                                            Multiple point quadratic calibration
                     FIGURE 10.15  The nonlinear relationship between the object view radiance and the
                     detector response.
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