Page 113 - Percolation Models for Transport in Porous Media With
P. 113

106                           CHAPTER 6.  PORE SIZE DISTRIBUTION

         ties  (such as  saturation) of such media are mainly determined by the volumes of
         the pores,  while  their conducting characteristics depend  primarily on  the capil-
         lary subsystem of the pore space.  Usage of the conventional parametric methods
         permits to study only the large-scale pore subsystem  (73].  To determine the pa-
         rameters of a capillary subsystem, it is necessary to gather information about the
         subsystem using a  quantity that does  not depend strongly on sizes of the pores.
         Electric conductivity is an example of such a  quantity.  Parameters can be found
         based on electric surface measurements using electro-parametric methods in a core
         partially saturated with a conducting electrolyte [74].  This method suggests that
         the measurements of the specific electric conductivities for  different  parts of the
         core saturated with a wetting electrolyte in the gravitational field  be taken instead
         of the measurements in the non-wetting mercury volume.  The described approach
         allows to get rid of the influence from  the subsystem of the site pores.  It is  also
         possible to determine the PDF for  capillaries based on direct  use of the percola-
         tional formula for electric conductivity.  This method suggests a combined scheme
         of mercury and standard porometry.


         6.1  Percolation Model for the Mercury Injection
                 Test


         During the mercury injection test the displacement of gas from the core by a non-
         wetting phase  (mercury)  takes  place.  As  it fills  the capillaries,  the non-wetting
         phase overcomes the capillary pressure

                              Pk  = !l.p = P1- P2  = 2xcos8/rk.              (6.1)
            For small pressure differences at the initial stage of the process, pores with radii
         greater than Tk  do not form  a  connected system.  They form  finite clusters, only
         those of which  can be reached  by mercury,  that are adjacent to the outer cross-
         section of the specimen.  When  the pressure difference reaches the breakthrough
         value,  large enough for  mercury to appear in  the outer cross-section of the core,
         the pores filled  with mercury form  a connected system, i.e., an infinite cluster.
            At  the intervening stage of the process,  as  !l.p increases further,  the density
         of the infinite cluster of the pores filled  with mercury goes  up.  When saturation
         S  reaches the second  threshold  value the connected system of the gas-saturated
         pores breaks.
            From this instant, during the final  stage of the process, the gas stops coming
         out of the core.  Trapped in the finite clusters, the gas compresses as the pressure
         in the non-wetting phase goes up.
            Take  a  periodic  network of cylindrical  capillaries  as  a  geometrical  model  of
         the  pore space and consider  the outlined  stages for  the  filling  of the  core  with
   108   109   110   111   112   113   114   115   116   117   118