Page 243 - Geochemical Remote Sensing of The Sub-Surface
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216                                                       T. Ruan and Q. Fei

           Indicator  gases

              Microseeps  comprise  a  number  of different  gases  that  are  evolved  as  a  product  or
           by-product  of  the  generation,  migration,  accumulation,  dispersion  and  destruction  of
           petroleum,  along with  other gases that follow the  same  migration  route.  Methane  (C~) is
           by  far  the  most  abundant  indicator  gas  in  microseeps  by  virtue  of  its  correspondingly
           high  relative  abundance  in  petroleum,  its  low  molecular  weight  and  its  chemical
           stability.  However, as an  indicator of oil and gas  it suffers  interference  from  methane  of
           near-surface  biological origin (Philp and Crisp,  1982).  Thus care must be exercised  when
           interpreting  the  C~  patterns  of  gas  geochemical  surveys.  Discrimination  between
           thermogenic  methane  (from  oil  and  gas)  and  near-surface  biogenic  methane  is  possible
           by  means  of  carbon  isotope  determinations,  but  the  method  is  relatively  expensive.
           Ethane  (C2), propane  (C3) butane  (C4) and  pentane  (C5) are  useful  for characterising  the
           thermogenic origin of microseeps because they are  less  likely to form  in the  near surface
           by biological  processes.  Some  higher molecular-weight  hydrocarbons (C5 up to  C22) are
           found  in microseeps either because they possess appreciable  vapour pressures or because
           they  occur  in  the  form  of  an  aerosol,  which  essentially  behaves  as  a  gas.  Data  for  a
           combination  of  the  foregoing  gases  provide  a  fingerprint  from  which  the  origin  and
           significance  of  surface  anomalies  can  be  deduced  with  greater  confidence  than  is
           possible using only data for a single gas (Klusman and Voorhees,  1983).
              In  addition  to  hydrocarbons,  a  number  of  inorganic  gases  that  follow  similar
           migration  pathways  are  useful  in  gas  geochemical  surveys  for  petroleum,  ltelium
           produced  by  the  radiodecay  of  U  and  Th  in  rocks  may  accumulate  in  gas  traps  to
           thousands  of  times  of  its  average  concentration  of  5.24  ppm  in  atmospheric  air,  and
           being  light  and  inert,  may  escape  to  the  surface.  Mercury  is  absorbed  from  water  by
           phytoplankton,  the  very  raw  material  of petroleum"  therefore  Hg  is  intrinsically  related
           to the  generation  of oil  and  gas.  In remote  sedimentary  basins  where  Hg of igneous  and
           anthropogenic origins  is rare,  Hg detection can  prove useful  in gas geochemistry surveys
           for  petroleum  exploration.  Since  uranium  seems  to  concentrate  in  the  low  Eh  oil-water
           contact zone  in oil fields, radon and  its daughters find applications  in surface prospecting
           tbr  oil  fields.  Some  natural  gas  contains  H2S and  SO2, which  are  produced  by  bacteria
           attacking sulphates  or by thermal  alteration  of amines (Hunt,  1979).  These  sulphur gases
           are therefore  possible surface  indicators of natural gas fields,  but their ready solubility  in
           groundwater  leads  to  weak  and  unstable  anomalies.  Nitrogen  is  evolved  during  thermal
           maturation  of organic  matter,  but N2 anomalies  are  difficult  to detect  in the  near-surface
           because of the high background concentration  of N2 in the atmosphere.
              Thus  oil  and  gas  fields  are  associated  with  many  types  of gases.  During  migration
           many  of these  gases,  especially  the  hydrocarbons,  react  with  their  surroundings  to  alter
           the  environment,  usually  by  consuming  free  oxygen  and  producing  more  reducing
           conditions.  The  formation  of pyrite,  magnetite,  siderite  and  other  carbonates,  as  well  as
           the  proliferation  of  certain  bacteria,  are  amongst  the  near-surface  consequences  of
           hydrocarbon  gas migration.  Whilst this  chapter  is concerned  with  the  direct  detection  of
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