Page 147 - Introduction to Mineral Exploration
P. 147

130   J. MILSOM



                  prove to be one of the most useful of the survey  every tenth of a second instead of every second
                  products (see section 9.2).                 or half second. Both cesium and proton instru-
                    The requirement for ever smaller ground   ments are (within limits) self-orienting and can
                  clearances and tighter grids is making demands  be mounted either on the aircraft or in a towed
                  on pilots that are increasingly difficult to meet.  bird. Sensors on aircraft are usually housed
                  In the future some airborne surveys, and espe-  in specially constructed nonmagnetic booms
                  cially aeromagnetic surveys, may be flown by  (stingers) placed as far from the main aircraft
                  pilotless drones.                           sources of magnetic field as possible (Fig. 7.2).
                                                              Aircraft fields vary slightly with heading and
                                                              must be compensated by systems of coils and
                  7.3  MAGNETIC SURVEYS                       permanent magnets. The magnitude of any
                                                              residual heading error must be monitored on a
                  Magnetic surveys are the quickest, and often  regular basis.
                  the cheapest, form of geophysics that can pro-  The Earth’s magnetic field is approximately
                  vide useful exploration information. A few  that of a dipole located at the Earth’s center
                  minerals, of which magnetite is by far the most  and inclined at about 10 degrees to the spin
                  common, produce easily detectable anomalies  axis. Distortions covering areas hundreds of
                  in the Earth’s magnetic field because the rocks  kilometers across can be regarded as due to
                  containing them become magnetized. The      a small number of subsidiary dipoles located
                  magnetization is either temporary (induced)  at the core–mantle boundary. The practical
                  and in the same direction as the Earth’s field,  unit of magnetic field for survey work is the
                  or permanent (remanent) and fixed in direction  nanotesla (nT, sometimes also known as the
                  with respect to the rock, regardless of folding or  gamma). At the magnetic poles the field is
                  rotation.                                   about 60,000 nT and vertical, whereas at the
                    Since magnetite is a very minor constituent  equator it is about 30,000 nT and horizontal
                  of sediments, a magnetic map generally records  (Fig. 7.3). Slow variations in both magnitude
                  the distribution of magnetic material in the un-  and direction, which must be taken into
                  derlying crystalline basement. Even sediments  account when comparing surveys made more
                  that do contain magnetite have little effect on  than a few months apart, are described, together
                  airborne sensors, partly because the fields from  with large-scale variations with latitude and
                  the randomly oriented magnetite grains typical  longitude, by a complicated experimentally
                  of sediments tend to cancel out and partly be-  determined formula, the International Geom-
                  cause the fields due to thin, flat-lying sources  agnetic Reference Field (IGRF). This is gener-
                  decrease rapidly with height. Because the small  ally a reasonable approximation to the regional
                  pieces of iron scrap that are ubiquitous in  field in well-surveyed areas where the control
                  populated areas strongly affect ground magnet-  on its formulation is good, but may be unsatis-
                  ometers, and also because ground coverage is  factory in remote areas.
                  slow, most magnetic work for mineral explora-  As well as long-term variations in field
                  tion is done from the air. Line separations have  strength, there are cyclical daily (diurnal)
                  decreased steadily over the years and may now  changes which are normally of the order of 20–
                  be as little as 100 m. Ground-clearance may  60 nT in amplitude. Variations are low at night
                  also be less than 100 m.                    but the field begins to increase at about dawn,
                    Magnetic surveys are not only amongst the  reaches a peak at about 10 a.m., declines rap-
                  most useful types of airborne geophysics but  idly to a minimum at about 4 p.m., then rises
                  are also, because of the low weight and sim-  more slowly to the overnight value. Although
                  plicity of the equipment, the cheapest. The  this pattern is repeated from day to day, the
                  standard instrument is now the high sensitiv-  changes are not predictable in detail and must
                  ity cesium vapor magnetometer. Proton mag-  be determined by actual measurement. Diurnal
                  netometers are still occasionally used but the  effects are especially important in airborne
                  cesium magnetometer is not only a hundred   surveys, which now typically use measuring
                  times more sensitive but provides readings  precisions of the order of 0.1 nT and contour
   142   143   144   145   146   147   148   149   150   151   152