Page 43 - Geochemical Remote Sensing of The Sub-Surface
P. 43

20                                                    O.F. Putikov and B.  Wen

                Pb, ~g/ml

              10                      /a
                                           c
                                                      50 m
               5


               0
                                   AB
                0  iiiili:~i~ii~i~ii!ii~i::~ii!::i~i~!::~ ilili ~ii~i:. ~iiiiiiiiii~iiiiiiiiii~iiiiii

              I00-


             200
                                                 \,, "x,
             300


                 ~il     [x~ w 14



           Fig. 2-2. Jet halo of lead, over a blind polymetallic ore body, overlain by allochthonous clays of
           thickness 30 to  100 m with different intervals between measurement points (a- 50 m, b- 20 m, c- 5
           m).  Schematic geological  section:  1- silts,  2-  clays, 3-  clay-siliceous siltstones,  4- quartzites,  5-
           mudstone  with  pyrite,  6-  mudstones,  siltstones,  7-  pyrite-polymetallic  ore  (reproduced  with
           permission from Ryss et al.,  1987b).


            9  the  shape  of anomalies  in profile  is more variable
            9  anomaly  amplitude,  Cm~x, and  width,  b,  are  only  loosely  related  to  the  depth  of  the
              source, h
            9  the  halo  extends  nearly  vertically  from  the  source,  so  that  the  halo  width,  b,
              corresponds  to the vertical projection  of the source to the surface

               These  features  of  the  jet  halo  enhance  the  prospecting  depth  of  the
           geoelectrochemical  methods.  A  number  of  field  experiments  have  verified  that  the
           prospecting  depth  for  an  ore  body  attains  some  hundred  metres  and  for  oil  and  gas
           reservoirs  several kilometres.  Similar results have been obtained with data for relatively-
           confined  forms  of metals,  although  the widths  of halos  are  greater than those  for mobile
           and weakly-conf'med forms of metals.
              Detailed  studies  of  the  distributions  of  concentrations  of  metals  in jet  halos  reveal
           apparent  non-uniformity  of  anomaly  structure  (Fig.  2-2).  Maximum  concentrations  of
           anomalies  on  the  diumal  surface  correspond  to  the  zones  of enhanced  concentrations  of
           mobile  fo~ms of metals  at depth,  which  extend almost vertically and have  a  complicated
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