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149    Faults and fractures at depth


                Although wellbore image data only provide information on the apparent aperture of
              faults where they are intersected by a wellbore, empirical relations have been proposed
              that attempt to relate fault length to aperture (e.g. Gudmundsson 2000) and enable one
              to develop ideas about fracture networks from wellbore image data. However, it should
              be pointed out that the aperture at the wellbore wall is not the actual width of the fault
              plane. As discussed by Barton, Tessler et al.(1991), image logs are basically measuring
              the smoothness of the wellbore wall, such that the logs are quite sensitive to any spalling
              at the wellbore wall that occurs as the bit penetrates the fault plane. Thus, the apparent
              aperture is always going to be larger than the actual aperture. Barton, Tessler et al.
              (1991) point out that it is sometimes useful to qualitatively distinguish large from small
              aperture faults during the analysis of image data.
                One obvious limitation of imaging tools is that they will undersample fractures and
              faultswhose planesarenearlyparalleltothewellboreaxis.Thisismosteasilyvisualized
              for a vertical well – the probability of intersecting horizontal fractures in the formation
              is one, but the probability of intersecting vertical fractures is essentially zero. Following
              Hudson and Priest (1983), it is straightforward to estimate the correction to apply to
              a fracture population of a given dip. If we have a set of fractures of constant dip, φ,
              with an average separation D (measured normal to the fracture planes), the number of
              fractures observed along a length of wellbore, L = D/cos φ, N obs (φ) must be corrected
              in order to obtain the true number of fractures that occur in the formation over a similar
              distance, N true (φ) via

              N true (φ) = (cos φ) −1  N obs (φ)                                  (5.6)

              This is illustrated for densely fractured granitic rock by Barton and Zoback (1992),
              who also discuss sampling problems associated with truncation, the inability to detect
              extremely small fractures, and censoring, the fact that when an extremely large fault
              zone is penetrated by a wellbore, it is often difficult to identify the fault plane because
              the wellbore is so strongly perturbed that data quality is extremely poor.




              Representation of fracture and fault data at depth


              Figure 5.5 illustrates the commonly used parameters that describe the orientation of
              faults and fractures in three dimensions. Fault strike refers to the azimuth of a horizontal
              line in the plane of the fracture and is measured from north. Unless otherwise noted,
              dip is measured from a horizontal plane and is positive to the right, when looking
              in the strike direction. Dip direction is often used instead of strike to define fracture
              orientation. Measured from north, dip direction is the azimuth of the projection of a
              vector in the plane of the fault that is normal to the strike direction and points down
              dip. Slip on the fault is also defined by a vector, which can be thought of as the
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