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             1991; Reddy et al., 1992; Chinn and Ascough, 1997; Chinn, 2006). GES- and AI-based
             techniques for mineral  prospectivity mapping are  beyond the scope  of this  volume.
             Readers are referred,  nonetheless, to  Yatabe and Fabbri (1988,  1989) for review of
             geoscience applications of AI methods and to Pan and Harris (2000, pp. 422-438) for a
             review of expert systems and AI methods applicable to mineral exploration.


             DISCUSSION AND CONCLUSIONS
                There are various  bivariate and multivariate  methods  of GIS-based data-driven
             modeling of mineral prospectivity and these methods are now mostly well-established.
             This chapter  has  demonstrated two methods for GIS-based  data-driven modeling  of
             mineral prospectivity (one bivariate method, data-driven evidential belief modeling, and
             one multivariate  method, linear  discriminant  analysis) and two techniques supporting
             these methods in order to properly create and integrate predictor maps in determining
             new targets for further exploration of undiscovered occurrences of mineral deposit of the
             type sought in a study area. These two latter techniques each address the issues of (a)
             objective selection  of a  suitable unit cell size for  data-driven modeling  of mineral
             prospectivity and  (b) selection of coherent  deposit-type locations  for data-driven
             modeling of  mineral prospectivity. In addition, a brief  review of cross-validation
             strategies in data-driven modeling of mineral prospectivity has been provided here.
                Until now, the choice  of a suitable unit cell (or  pixel) size [denoted as  N(•)] for
             raster-based-GIS data-driven  modeling  of  mineral prospectivity has been subjective.
             Point pattern analysis  (Boots  and Getis, 1988;  Rowlingson and  Diggle, 1993)  of the
             range  of distances in  which there is zero probability of  one neighbour deposit-type
             location situated next to another deposit-type location is useful in deriving a preliminary
             set of choices for a suitable N(•). Then, using this range of distances, the analysis of the
             rate of increase in the ratio [N(D)] : [N(T)–N(D)] as function of equal-interval change in
             N(•) is robust, regardless of the number of deposit-type locations and the size of a study
             area, in determining the most suitable N(•). Although these propositions have not been
             demonstrated through formal testing, the empirical spatial associations between deposit-
             type locations and indicative geological features in the case study area as quantified via
             data-driven estimation of EBFs (this chapter) and as  quantified via the  distance
             distribution method and distance correlation method (Chapter 6) are very similar. On the
             one hand, the pixel size used in the spatial association analyses in Chapter 6 is, in fact,
             10 m. This small pixel size was necessary in the analysis in Chapter 6 because we know
             (or have learned from Chapter 4) that spatial measurements (e.g., distances) are fractals
             so that an infinitesimally small pixel or unit cell  is  necessary for  accurate spatial
             measurements. On the  other  hand, the  pixel size used in all the experiments of data-
             driven modeling of mineral prospectivity presented in this chapter is 100 m, as
             determined objectively via the proposed techniques. A pixel size of 100 m is a practical
             spatial representation of the epithermal Au deposit occurrences in the case study area,
             whilst a pixel size of 10 m is not. Nevertheless, the proposed techniques for objective
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