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56      Modern  Spatiotemporal  Geostatistics —  Chapter  2

        of  ds,  we can write the  space/time  metric  as in  Equation 2.28.  Equation 2.28
        attributes  a  physical meaning to  the  quantity  \dp\,  even  if  the  points  are so
        chosen  that  the  corresponding  \dp\  does  not  vanish  (Einstein,  1994  [1954]).
         In  particular,  we say that  the  space/time  distance is  "space-like"  when  \dp\  is
        real,  "time-like"  when \dp\  is imaginary, and  "light-like"  or  "null"  when \dp\ is
        zero.  Space-like distances occur  between events with  a spatial separation less
        than the distance the  light  pulse travels between the times of their occurrence;
        time-like  distances occur between events with a spatial separation that exceeds
        the  distance  that  the  light  pulse can  travel  in  the  time  between  them;  null
        distances  represent events  in  space/time  that  could just  be  connected  by a
        light  pulse.  Mathematically,  the  distance (Eq.  2.28)  is the  Minkowski  metric
                                                    2
        determined  from  Equation 2.27 by letting g 00 = —c ,  gu  =  1 (i  =  1,... ,n),
         and

         Restrictions  on  spatiotemporal    geometry    imposed
        by  physical laws
        We  have  seen  that  we can  learn  about  the  nature of  space/time  by  studying
        the  characteristics of  the  physical system.  Nature  does  not,  of  course,  allow
        the  natural  processes  to  vary  in  an arbitrary manner,  but  imposes constraints
        in the  form of  physical laws.  Consider a physical law governing the  distribution
        of  a natural field  X(p)  that  is generally expressed as



        where v =  (v\,... ,Vk)  are known physical coefficients, BC  and 1C  are given
        boundary  and initial conditions,  and L[-\  is a known mathematical functional.
        Typically,  Equation  2.33  is  regarded as  determining  the  values  of  the  field
        X(p]  from  the  known coefficients v,  the  BC  and 1C,  and the  space/time
        coordinates.  When it  comes to  the spatiotemporal metrical structure, however,
        there are several ways in which the  physical law (Eq.  2.33) can help one's effort
        to  determine  the  appropriate metric  form.  Some  of  these ways  are reviewed
        next.
            In  certain  applications,  Equation  2.33  leads  to  the  following  explicit  ex-
        pression for  the  metric



        where  x  ar| d  x'  are  ^-values  at  points  p  and p',  respectively;  and g [•] has
        a  functional  form  associated  with  -£•[•].  As  far  as  the  metrical  structure  is
        concerned,  the  interpretation  of  Equation  2.34  can  be different  from  that  of
        Equation  2.33.  Given  any  metric  \dp\,  Equation  2.34 will  not  be satisfied
        automatically.  In fact,  Equation  2.34 will  serve  to  cut  down  the  number  of
        possible  metric  models.  Equation  2.34  is  thus  regarded  as  determining  the
        metric  \dp\  of  the  space/time  geometry  from  the  natural  field  values  at  p
        and  p',  the  coefficients  v,  the  BC,  and  the  1C.  Here,  then,  is  a  sense  in
        which  Equation  2.34 restricts the space/time  geometry.  On imposing  Equation
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