Page 31 - Special Topic Session (STS) - Volume 1
P. 31

STS346 A.H.M. Rahmatullah Imon
               This example gives a clear distinction between classical outlier and spatial
            outlier. In Figure 2(a) attribute values are plotted against their locations. For
            global outliers, traditional statistics will essentially look at the attribute values
            in the y axis and if we do that we observe that the points which are very high
            such as A or very low such as B. In contrast to that, the spatial outliers are like
            the spikes C, D, and E. They look like spatial outliers because they violate the
            law of geography that the nearby things should be very similar. When we take
            the first order difference of the attributes as shown in Figure 2(b) clearly C, D,
            and E look very different than their neighbors. It is also interesting to note that
            the  possible  global  outliers  A  and  B  do  not  look  like  outliers  anymore.  In
            general, we do not search for outliers along the x-axis. But when we carefully
            look at Figure 2(a), we observe that the point F has a marked difference from
            its neighbors. Points G and H look unusual too. This difference is visible more
            clearly when we look at the first order difference of the locations as shown in
            Figure 2(b). Point F now clearly looks like a high leverage point or an outlier
            along the x-space. Points G and H look more extreme as well.


















                     Figure 2: Scatter plot of the original and the first order differenced data.

                   Table 2: Residuals and leverages for Hadi and Imon (2018) spatial outlier data
                Index    Del St. Residual    Leverage         GSR              GP
                  1            *              *                *                *
                  2         0.45678        0.040885         1.09925          0.06658
                  3         0.11424        0.051079         0.20420          0.06290
                  4         2.15139        0.035779        5.31765 C         0.03590
                  5         -1.69711       0.037989        -4.20445 C        0.03835
                  6         0.47421        0.035612         1.13209          0.04571
                  7         0.32834        0.051079         0.72348          0.06290
                  8         0.06085        0.051079         0.07645          0.06290
                  9         -2.41622       0.045639        -6.03394 D        0.05185
                  10        2.61223        0.041275        6.49375 D         0.04367
                  11        0.07639        0.035779         0.07645          0.03590
                  12        0.89298        0.040885         0.13783          0.06658


                                                                20 | I S I   W S C   2 0 1 9
   26   27   28   29   30   31   32   33   34   35   36