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358   Chapter Eleven


               according to the inversion algorithm they employ for reconstructing
               the ensemble statistics from the measured experimental trace. Phase-
               space techniques estimate either the Wigner function or the ambiguity
               function. There are two classes of phase-space techniques, spectro-
               graphic and tomographic. Methods from which the inversion returns
               either the two-time or two-frequency correlation function may be clas-
               sified as direct techniques: these are interferometric.

               11.3.2 Pulse Characterization Apparatuses
                        as Linear Systems
               Although currently most methods for pulse characterization are based
               on nonlinear optical processes, it is informative to consider a general
               framework for analyzing measurement methods based on a linear
               filter analysis. This approach has two benefits. First, it proves that
               nonlinearities are not necessary for determining the pulse field and
               shows why they are often used. Second, it specifies the necessary and
               sufficient conditions that must be fulfilled by any apparatus that is ca-
               pable of determining the field. This leads to a convenient classification
               scheme for most methods.
                 Consider the general interferometer shown in Fig. 11.6. It consists
               of four causal filters and a square-law, integrating detector. Therefore,
               we may consider a two-beam interferometer for the analysis with-
               out loss of generality because a multibeam interferometer can always
               be decomposed into a linear combination of two-beam interferome-
               ters. Each filter is characterized by a time-domain response function
                H k (t, t ). We take the filters, and therefore the interferometer, to be

               linear systems in the broad sense that the output field E out (t) after the
               filters can be expressed as a function of the input field E in (t)as




                                E out (t) =  dt H k (t, t )E in (t )  (11.56)
               for the kth filter in the sequence. For measurement schemes in which
               no interference of the filtered versions of the input pulse is required,
                H 3 and H 4 may be set to zero.


                               H (t;t′)        H (t;t′)
                                                2
                                1

                               H (t;t′)        H (t;t′)
                                3
                                                4
               FIGURE 11.6 General interferometer for optical pulse characterization
               where H k (k = 1 to 4) represents the action of linear filters on the electric field
               of the input pulse before a square-law time-integrating detector.
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