Page 274 - Modern Spatiotemporal Geostatistics
P. 274

Popular  Methods in  the  Light  of  Modern Geostatistics  255

        and time that  are due to  the  mean of the  increment;  if  the  mean of the  incre-
        ment  is zero, the  mean of X(p)  is constant).  This  class of  models can handle
        complicated  space/time  variabilities  of  any  size in  a  mathematically  rigorous
        and  physically  meaningful  manner,  and is considerably  more  general  than  the
        restricted  class  of  homogeneous/stationary  S/TRF  (by  standard  convention,
        the index values v =  JJL =  — 1 correspond to spatially  homogeneous/temporally
        stationary  fields with  no trends).
            There  are various useful representations of the S/TRF-^//x X(p)  (Chris-
        takos and Hristopulos,  1998).  An interesting representation is derived by choos-
        ing the following test  function




        where the superscript (i/+/i+2) denotes the space/time differentiation  operator
                                           with                  In light of
         Equation  12.38,  Equation  12.34 leads  to  a  continuous-domain  S/TRF-f//z
         representation  as follows




        where  X[q](p)  = Y(p) is a zero-mean  homogeneous/stationary field.  A dis-
        crete domain representation  is possible by means of  the summation




        where  q(p, pj  are local  weights  and the X(p i)  represent the  values  of the
         random  field  at  space/time  points p t.  Several  other  S/TRF-z///x representa-
        tions  (continuous  and discrete)  involving test  functions  different  than that  of
         Equation  12.38 can be found  in the  literature.
             The  space/time  covariance of X(p)  satisfies the  decomposition  relation-
        ship


        where k x(r, T)  is the  generalized spatiotemporal covariance that depends only
        on the spatial and temporal  lags r  =  s — s'  and T =  t  — t';  the ©,,/ M(p,  p')
        denotes  polynomials of  degrees v  in  space and n in time.
             The  generalized  covariance k x  can  be  viewed  as a  generalized  function
        defined  on  the  spaces 2? or  *D'  by  means of  a  linear  functional  as follows




        with  p  =  (r,  T).  The generalized  Fourier  transform  k x(w),  w  =  (K, cu),  of
         ^(p)  is defined as (k x,q}  =  (k x,q);  the functional  (k x,q)  =  f wq(w)k x(w)
         is  a  frequency  space integral,  where  q(w)  is  the  ordinary  Fourier  transform
        of  the  test  function.  Various examples  of  generalized space/time covariances
   269   270   271   272   273   274   275   276   277   278   279