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Spatiotemporal  Geometry                    61

        where  g(-)  is some known  function.  [Notice the  difference  between  fir(x map),
        which  is  a  function  of  the  realization  values,  and  its  expectation  ~g(p map),
        which  is a function  of  the  space/time  points.]  There  is, generally,  no  need  to
        specify  limits  of  integration  in  Equation  2.44,  since  if  certain  ranges  of  Xma P
        are  impossible,  the  pdf will  be zero,  removing  contributions from these ranges.

        EXAMPLE   2.27:  If we let g(xi)  =  Xi<  Equation  2.44  provides the mean




        of  the S/TRF. If we let g(xi,X2)  =  (Xi  -  zi)(X2 -  x 2),  the (centered)
        covariance function




        between the points p1 and p2 is obtained; etc.



        COMMENT 2.11 : S/TRF   characterization   i n terms   o f Equation   2.44   w

         considered "incomplete"   (or   general   or   vague),   in   the   sense   that   several
        random fields exist  that share the same space/time  moments.   Also,   statisti-
         cal moments  can  be defined  for   more  than  one  random  field  simultaneously,

        in which   case   Equation   2.44   should   involve   data   or   map   vectors   for  all


        these  field s (see,   e.g.,  th e multivariable   o r vector  formulation  o f  BM E  i n

         Chapter 9).

         Correlation  analysis  and spatiotemporal      geometry
        In  geostatistical  applications,  spatiotemporal  correlation  functions  are usually
        part  of  the  available physical  knowledge  bases.  These functions  could  be de-
        rived  from  a  physical  law  or  fitted  to  the  data.  Commonly  used  correlation
        functions  include the ordinary covariance, the variogram (sometimes also called
        semivariogram),  and the  generalized covariance. Ordinary covariance  analysis,
         e.g.,  can  be  helpful  in  determining  the  physically  appropriate  spatiotemporal
        geometry.  Let  us suppose that the form  of a finite metric  A is sought  such that




        Taking the derivatives of this equation, we find dc x/dhi  =  (dc x/dX)  (dX/dhi)
        and  dc x/dr  =  (dc x/dX)  (dX/dr).  The  last  two  equations  imply  that  the
        metric  A is related  to  the  covariance of the  natural  field  through the following
        set of  equations







        where i, j  = 1,... ,n.
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