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Exploring for Geothermal Systems                                            107


                           NW                Possible flow paths       SE
                               Mangakino                        Kaingaroa
                                caldera                          plateau    Ωm
                          0                                                 3000
                                                                            1000
                                                                            300
                        Depth (km)  10                                      100


                         20                                                 30
                                                                            10
                                                                            3
                                                                   km
                                              Possible magma body  0   10
            FIGUre 6.13  (See color insert following page 17.0..) A model based on a magnetotelluric survey conducted
            in the Wairakei Valley, New Zealand. The low resistivity region at a depth of about 20 km is interpreted to
            be a magma body. The white crosses indicate sites of microseismic events. The locations of possible fluid
            flow paths at depths of less than 10 km are indicated by the arrows. (Modified from Heise, W., Bibby, H. M.,
            Caldwell, T. G., Bannister, S. C., Ogawa, T., Takakura, S., and Uchida, T., Geophysical Research Letters, 34,
            L14313, 2007.)

              Although magnetotelluric surveys provide a powerful means for accessing information about the
            deep subsurface, heat sources, and regional fluid flow pathways, shallow level resistivity surveys are
            needed in order to identify specific drilling targets. In this way, they are admirable complements of
            an exploration program.


            GraviTy surveys
            If the Earth were a homogeneous perfect sphere, the resulting gravitational acceleration would be
            the same everywhere. The equation describing this phenomenon is the classic Newtonian represen-
            tation of gravitational force:

                                                           2
                                           F = (G × m  × m )/r .
                                                    1
                                                        2
                                              2
                                                  2
                                         −11
              The constant, G, equals 6.67 × 10  Nm /kg , m  and m  are the masses of the respective objects
                                                           2
                                                     1
            affected by the interaction and r is the distance between their respective centers of mass. At the
                                                                                          2
            surface of the Earth, the resulting nominal value for the acceleration due to gravity is 9.80665 m/s .
            But, topography, the oblate spheroidal form of the planet, and the complex geological structures that
            makeup the Earth result in a more complex gravitational field than a simple spherical, homogeneous
            body would provide. Two factors contribute to this situation. One factor reflects the density stratifi-
            cation and plastic nature of the deep, hot Earth. Since the crust of the Earth, whether it be oceanic
            crust or continental crust, literally floats on the mantle and, to a first approximation the mantle and
            core are homogeneous in density, they can be treated as a constant mass that underlies and supports
            the more heterogeneous crust. As a result, variations in the gravitational acceleration at the Earth’s
            surface can be interpreted in terms that include any differences in rock density in the crust. The sec-
            ond factor results from the effect of the r  term in the gravitational force equation. A small variation
                                            2
            in rock density near the surface of the Earth will have a much larger effect on the measured value
            of the acceleration of gravity than would the same sized density contrast at a greater distance. These
            variations in the gravitational field are called gravity anomalies, and can be either negative or posi-
            tive, depending upon whether they result in a local gravity feature that is, respectively, less than or
            greater than a locally derived baseline value. Sensitive gravimeters, capable of measuring variations
            in the earth’s gravitational field at a level of precision exceeding a fraction of a part per million, have
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