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Image Geometric Rectification      195

                   The accuracy of determining the position and orientation of the
               sensor using direct georeferencing lies typically between 10 and
               20 cm (RMS), and 15 and 30 arc seconds (RMS), respectively (Litho-
               poulos et al., 1999). This level of accuracy has been confirmed by Kinn
               (2002). Evaluated against 24 GCPs, a ground positioning accuracy of
               around 1 m was achieved in both easting and northing (Mostafa and
               Schwarz, 2000). The accuracy for height is lower, at a range from 1.5 to
               about 3 m. Horizontal coordinates and height have a standard devia-
               tion of 0.9 and 1.8 m, respectively. The ground positioning accuracy
               was further improved to 0.5 m in planimetry (1s) and 1.6 m in height
               from stereopairs at an average image scale of 1:12,000 (Mostafa and
               Schwarz, 2001). The highest ground positioning accuracy is achieved
               at 0.2 m of planimetric accuracy and 0.3 m in height using GPS/INS-
               aided block triangulation of both nadir and oblique images. This
               accuracy level is sufficiently accurate for mappings at scales <1:5000.

               5.8.2  Comparison with Polynomial Model
               As shown in Eqs. (5.13) and (5.14), polynomial-based image transfor-
               mation handles only the horizontal position of pixels. It is unable to
               deal with the third dimension of pixels (i.e., height). Therefore, any
               positional shift caused by topographic relief on the ground cannot be
               removed via the application of the two transformation models. The
               polynomial method is suitable for georeferencing satellite images
               obtained at a very small scale. If ground control is available, this
               method is preferable in transforming images from the local coordi-
               nate system to the global system. In this way it is feasible not only to
               coregister multiple images but also to correct geometric distortions
               inherent in the input image. Very easy to implement, polynomial
               image rectification is advantageous over direct georeferencing in that
               it does not require information on satellite orbit and sensor calibra-
               tion (El-Manadili and Novak, 1996). However, it has the following
               three disadvantages:
                    •  First, it requires maintaining a large number of well-distributed
                      GCPs.
                    •  Second, it lacks physical interpretation of the model beyond
                      the second order.
                    •  Third, it is unable to handle the positional shift caused by
                      topographic relief displacement. Of the two sources of
                      geometric distortions in remote sensing images, those caused
                      by orbital parameters exert a global impact on all pixels in an
                      image. With the polynomial model, such distortions can be
                      effectively dealt with. However, those caused by variation in
                      topography are impossible to address.

                   The influence of topographic relief is local and random in nature.
               This influence can be effectively tackled by a stochastic approach of
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