INTRODUCTION

The problem of statistical spatial analysis encompasses an expanding range of methods which address different spatial problems, from image enhancement and pattern recognition to spatial interpolation and socio-economic trend modeling. Each of these methods focuses on a particular aspect but what emerges is something that is clearly identifiable as spatial statistics, statistical methods like MG, CSS and GWR techniques which address geographical raw data that are spatially correlated.

According to Ferreira and Simoes (1993, 1994), the kernel of geography is to think geographically, that is, to study the spatial distribution of the phenomena and their correlations. Traditional statistics must be reformulated to properly account for spatial correlation and spatial heterogeneity within georeferenced data (Anselin, 1996, 1998). Spatial autocorrelation is a reality but also a requirement to carry out spatial interpolation and spatial regression modeling. For instance, if regression residuals reveal a medium-strong spatial autocorrelation then any missing variable within the initial regression model can be significant. Certainly, MG, CSS and GWR try to include this spatial autocorrelation issue within their spatial interpolation and simulation computation.

To re-examine these procedures becomes, hence, the goal of this research. Section two highlights Morphologic Geostatistics (MG) while sections three and four underline Conditional Gaussian Sequential Simulation (CGSS) and Conditional Categorical Sequential Simulation (CCSS), respectively. Direct Sequential Simulation (DSS) is also introduced while Geographical Weighted Regression (GWR) is presented in section five. Close relationships among these spatial issues are presented in present study.

It is vital to stress that the comprehension of this essay underlines the knowledge of variography and Kriging topics (Aguilar et al., 2008; Negreiros et al., 2010). Additionally, the input Pb spatial data, exploratory, variography and Kriging results that follow section two and three are presented in the Appendix (contamination data of Aljustrel, Portugal, within a global area of 4500 mx2950 m). The software used here was GeoMS⁸ from Instituto Superior Técnico, Lisbon.

MORPHOLOGIC GEOSTATISTICS

This section is dedicated to MG for categorical variables (body X and body X^C) such as the presence/absence of a particular type of pine tree in an open field, for example. The main idea is to analyze the spatial structure for problems closely related with qualitative variables which is useful to understand the degree of presence of a certain type of objects in space.

Fig. 1:	(a-d) Histogram, cumulative distribution functions, box-plot, descriptive statistics (top) and spatial location map (bottom) of the categorical variable (blue dots versus red ones) based on Eq. 1

Quite often, farmers do not want to measure the number of grasshoppers (quantitative variable) but wish to classify sub-regions according to a pre-define classification (categorical variable) such as lower, medium and high infestation.

For illustration purposes lets consider the Pb contamination dataset (Appendix). By considering an indicator variable whose cutoff value equals the median of the Pb values, a categorical variable can be created according to the next rule:

(1)

That is, a particular x location equals 1 if that particular site is classified as an X body (all x>40 ppm). Otherwise, it equals 0, which means that the location is classify as X^C (all x No. 40 ppm). It is central to highlight that this I_morf (x>40 ppm) condition (body X) used in this example works as a classification criteria for the present contamination dataset creating, thus, a two-phase structure: population X and population X^C (Fig. 1a-d).

As expected, the spatial continuity of both bodies can be measured by the indicator variogram based on the sill, anisotropy (range) and nugget-effect parameters. In this morphologic context, the range factor measures the average dimension of X and X^C bodies while the nugget-effect denotes the transition frequency between both bodies (1 and 0 states) at small scale (Fig. 2). The variogram that lies behind this spatial autocorrelation structure is a spherical one with a major and minor range of 2500 and 1000 m, respectively. The nugget-effect equals zero. The main direction of the geometric anisotropy is 901.

Fig. 2:	Probability estimation map for the X body obtained by Indicator Kriging of the IMorf variable (the highest probabilities of Pb to be greater than 40 ppm are located at the lower right corner)

Fig. 3:	The two-strata structure morphologic map (body X in red and body XC in blue)

Fig. 4:	The previous two-phase structure morphologic map including uncertainty regions

The probability map of Fig. 2 can be transformed into a morphologic binary map to reproduce the X and X^C bodies as described next (Soares, 1990):

In the Pb example, (m_X)* equals 0.605786 which means that the body X covers 60.6% of the region. Among the 34126 kriged blocks of Fig. 2, the 20673 locations (34126H0.605786) with the highest probabilities were assigned the value 1 and the remaining ones were set to 0. Mapping this new binary variable allows to produce the estimated morphologic map of the body X (Fig. 3).

Concerning the uncertainty assessment of the morphologic map, which is higher on the border between different bodies, the following four steps were computed (Fig. 4):

In the example:

CONDITIONAL GAUSSIAN AND DIRECT SEQUENTIAL SIMULATION

Interpolation methods, such as Ordinary Kriging (OK), typically overestimate small values and underestimate large ones. As with the traditional regression, the final estimates are less variable than the true values. Although a kriged map shows the best estimates of a variable, it does not represent the variability in a proper way, that is, this loss of variance could lead to wrong decisions. To estimate a surface that retains the original samples variability, we need other techniques such as geostatistical stochastic simulation (Webster and Olivier, 2007).

Within spatial analysis, the stochastic simulation is a tool to evaluate the spatial uncertainty based on the generation of N sets of equiprobable values (Soares, 2000). Each simulated image should hold the statistical properties of the original observations, such as the mean, variance, histogram and covariance. Additionally, simulated values honor, at their locations, the measured data values. Based on the N realizations, it is possible to compute uncertainty measures and to assess the extreme spatial behavior of any particular phenomenon. For instance, from a set of maps, it is possible to assess all sub-regions with values above a certain threshold and the probability of that to happen. Even more important for pollution studies, it is possible to generate scenarios yielding the smallest (best scenario) and the largest (worst scenario) contaminations costs.

Broadly, there are three classes of simulation algorithms B sequential, p-field and annealing-although only the first one will be covered in this study. The Conditional Gaussian Sequential Simulation (CGSS) technique is based on the assumption that the spatial distribution of a continuous random variable can be modeled by a multivariate Gaussian model. Through the sequential simulation algorithms, instead of modeling the N-points conditional cumulative distribution function (ccdf), a one-point ccdf is modeled and sampled at each of the N nodes visited along a random sequence. To ensure the reproduction of the variable covariance model, each one-point ccdf is made conditional not only to the original data but also to all values simulated at previously visited locations (Goovaerts, 1997).

With CGSS, each variable is simulated sequentially according to its Normal ccdf, which is fully characterized through a Simple Kriging (SK) system. The conditioning data consist of all original data and all previously simulated values found within a neighborhood of the location being simulated.

Fig. 5:	Random path example of the sequential simulation technique (Soares et al., 2010)

Fig. 6:	Diagram of step 5 (Soares et al., 2010)

The conditional simulation of a continuous variable Z(u) modeled by CGSS proceeds, then, as follows:

Journel (1994) showed that for this conditional sequential simulation algorithm to reproduce a specific covariance model it suffices that the simulated values are drawn from the local distributions centered at the Simple Kriging estimates with a variance corresponding to the Simple Kriging estimation variance. This result guarantees that the spatial covariance and the global sample mean and variance, of the original variable are reproduced but not the histogram. To overcome this limitation, Soares (2001) proposed a Direct Sequential Simulation (DSS) algorithm that uses the local Simple Kriging estimates of the mean and variance, not to define the local cumulative distribution function (cdf) but to sample from the global cdf.

Recently, Costa et al. (2008a) and Costa and Soares (2009) proposed a new method for the homogenization of climate data using the DSS algorithm. The DSS procedure is used to calculate the local probability density function (pdf) at a candidate station's location. The algorithm generates realizations of the climate variable through the resampling of the global pdf using the local mean and variance of the candidate station, which are estimated through a spatiotemporal model.

Fig. 7:

With conditional simulation, the number of realizations used to produce the final estimates can strongly affect the outcome of the interpolation. The upper six images correspond to 80 mx80 m grid interpolated maps (density of 0.5 m) with different numbers of simulations: (a) block Kriged data; (b) the same data interpolated for n = 1 conditional simulation; (c) n = 10 simulations; (d) n = 100 simulations; (e) n = 1000 simulations; (f) n = 10000 simulations (Robertson, 2008)

The local pdf from each instant in time is used to verify the existence of irregularities: a breakpoint is identified whenever the interval of a specified probability p, centered in the local pdf, does not contain the observed (real) value of the candidate station. If irregularities are detected in a candidate series, the time series can be adjusted by replacing the inhomogeneous records with the mean of the pdf(s) calculated at the candidate station's location for the inhomogeneous period(s).

Recently, Costa et al. (2008b) used the direct sequential cosimulation (coDSS) algorithm to map a flood indicator and extreme precipitation frequency in Southern Portugal using elevation as auxiliary information. The methods incorporate space-time models that account for long-term trends of extreme precipitation and local changes in the relationship between elevation and extreme precipitation through time.

SEQUENTIAL SIMULATION FOR CATEGORICAL VARIABLES

Variables, such as the concentration of a metal in the soil, may appear to change abruptly in space. In this case, the phenomenon should be modeled as a mixture of two populations each of them may have different patterns of spatial continuity (Goovaerts, 1997). To deal with this type of variables, Sequential Indicator Simulation (SIS) is presented in this section as it allows modeling the relative geometry of each population (strata) in order to create an exhaustive categorical map.

Analogous to the CGSS, seven major steps are involved in the SIS algorithm:

Sequential simulation will be exemplified for non-continuum variables using the input dataset detailed in Appendix. First, a new categorical variable with four classes (Fig. 8a-d), named CI (u), is computed using the Pb contamination data and Eq. 2:

(2)

u stands for a particular spatial location

Several experimental variograms for the four phase variable were computed according to two main directions (geometric anisotropy): 0° (N/S direction) and 901 (E/W direction). Notice that this multiphase variogram equals:

that is, each variogram lag corresponds to a global average of four individual covariances (Fig. 9a, b).

Fig. 8:	(a-d) Histogram, cumulative distribution function, box-plot and univariate statistics (top) spatial layout (bottom) of the categorical variable CI(u)

Fig. 9:	(a, b) Average variogram for the multiphase CI(u) variable adjusted by a spherical model with the sill equal to 1.24, the major range equal to 2000 m (E/W direction, bottom) and the minor one equal to 1200 m (N/S direction, top)

Regarding the simulated data of Fig. 10, it is curious to confirm that the histogram of these 34126 values estimated by the Sequential Indicator Simulation (SIS) is similar to the original distribution histogram (Fig. 11a-c).

Fig. 10:	Example of an indicator realization map of CI(u) generated by SIS

Fig. 11:	(a-c) Histogram, cumulative distribution function, box-plot and univariate statistics of the simulated values

It is also important to highlight that all simulated data honors the experimental data.

In average, the simulated spatial images hold the same statistical features of the original observations. In fact, the variograms of the simulated map hold a similar shape (Fig. 12a, b). In this case, a spherical model with a major range of 2000 m (E-W direction) and a minor one of 1200 m (N-S direction) was fitted. The fluctuations between both models are known as ergodic fluctuations (Goovaerts, 1997). In fact, Gaussian and Indicator simulation algorithms only reproduce the original observations variogram in the presence of an average simulated map that results over many realizations. The ergodic fluctuations of the realizations' variograms are generally important when the range of the variogram model is larger with respect to the size of the simulated area (particularly if the relative nugget-effect is small).

As already stated before, Indicator Kriging (IK) allows to estimate the conditional cumulative distribution function (ccdf) for a particular spatial location. By defining L cutoff values, it is then possible to infer about the uncertainty probability of each class (ccdf difference of any adjacent cutoffs).

Fig. 12:	(a, b) Comparison of the SSI multiphase experimental variogram with the one fitted to the original data in Fig. 9.

Fig. 13:	Local entropy map generated by the 100 indicator simulation maps

Using these partial probabilities, the Shannon entropy procedure allows inferring the local uncertainty of the interpolation at unknown sites. Given L sets of IK probabilities at any u location P_i(u), with i = 1...L, the Shannon entropy (a disorder measure closely connected to the spatial organization of an attribute) equals BSUM(P_i(u)H LN(P_i(u))), where LN() denotes the Neperian logarithm, P_i() is the IK estimation probability for each class while BSUM() denotes the negative sum of all classes' probabilities at that u location. As expected, red color signifies high lack of estimation confidence while dark blue denotes low uncertainty (Fig. 13). Unsurprisingly, uncertainty is smaller near the samples locations.

GEOGRAPHICALLY WEIGHTED REGRESSION (GWR)

Statistically, Ordinary Least Squares (OLS) regression is a technique that allows to relate k-1 independent variables (X₁YX_k-1) to a dependent one (Y) in the following form: Y = X₀+X₁β₁+X₂β₂+Y+X_k-1β_k-1+∈. Denoting by n the number of sub-regions considered in the spatial problem, Y is a (nH1) vector, X is a (nHk) matrix, β is a (kH1) regression coefficients vector concerning each independent variable and X is a (nx1) residuals vector (Fig. 14). The regression errors should follow a Gaussian distribution with zero mean and constant variance σ² (Druck et al., 2004).

The major aim of regression analysis is to uncover which variables contribute in a significant way for the linear relationship of the dependent variable. Still, it is expected, among other factors, that regression errors are independent. According to Anselin (1992, 1994), this OLS model fails quite often due to the occurrence of spatial autocorrelation. The global spatial lag model (SAR) for stationary processes overcomes this drawback. It is defined by Y = ρWY+Xβ+ε where, W represents the neighborhood matrix and ñ is the spatial autoregressive coefficient. Another possibility is to use different spatial regimes (i.e., an individual regression for each region) in SpaceStat⁸. Polynomial trends is another option to work with the region overall tendency and non-stationary phenomenon. Another possibility is the local continuous variation framework computed by the Geographically Weighted Regression (GWR) system. The idea is to adjust a regression model by weighting the neighborhood observations. In this way, the estimation computation will reflect automatic adjustments according to the distance of the available samples.

GWR is a specific model which allows representing non-stationary local phenomena by generating a separate regression equation for every feature analyzed as a means to address spatial variation (Fotheringham et al., 2002). Thus, GWR allows the modeling of processes that vary over space. Since, it usually works with aggregation data, this inferential model considers that spatial data may change abruptly (or not) at region boundaries only (Fig. 15).

Another example of this method is presented by Legg and Bowe (2009) regarding the analysis of the listed sales price for single family houses in Marquette, Michigan and it is based on location and three other variables: number of bedrooms and bathrooms, house square footage and lot size (Fig. 16). According to these authors, the OLS model was found to be significant and had a high R² = 0.782. Yet, the GWR model improved on this statistic and increased the model’s goodness of fit to an R² = 0.865. In addition, the range of the residual error decreased by $160,000 when using the GWR model instead of the Ordinary Least Square (OLS) model. The coefficients surface was also helpful for identifying the spatial patterns apparent in the study area.

Fig. 14:	The Ordinary Least Squares (OLS) regression system in matrix notation

Fig. 15:	The number of murders per ward in Rio de Janeiro between 1908 and 1992 (Druck et al., 2004). Values do not vary within each ward because of the polygon spatial structure

Fig. 16:	Listing price map of a typical house modeled using spatially varying regression coefficients generated using GWR tools of ArcGIS© (Legg and Bowe, 2009)

Fig. 17:	W(ui) is an n by n matrix representing the geographical weights around location ui. This weighting system is known as kernel

For example, the lot coefficient indicates that located groups nearer the urban core and farther from the rural townships increases its price. In contrast, coefficients suggest that the larger the house, the less it contributes to the listing price.

For Lloyd (2007), one key decision emerges from this inferential spatial approach: the choice of a weighting function (kernel shape and kernel bandwidth). Given two independent variables, y₁ and y₂, the local estimation of GWR parameters equals z (u_i) = β₀(u_i)+β₁(u_i)Hy₁+β₂(u_i)Hy₂, where z is the dependent variable while (u_i) is the (x,y) location at which the parameters are estimated. By solving the system, the parameters can be estimated by β (u_i) = (Y^THW(u_i)HY)^-1HY^THW(u_i)Hz, where, W (u) is a weight square matrix closely related to the position of u towards the available samples (Fig. 17), Y^THW (u_i) HY represents the geographically weighted variance-covariance matrix (the estimation requires its inverse) while z corresponds to the vector of values of the dependent variable (original observations).

Typically, these weights follow the Gaussian weighting function: W(u_i) = exp (B0.5(d/b)²) if d_i≤b, where d is the Euclidean distance between the location of the neighborhood observations and the location u_i to be estimated, while b represents the bandwidth of the kernel. As the bandwidth gets larger, the weights approach one and the local GWR model approaches the global OLS model. As expected, if d_i>b, a zero value should be produced.

Overall, GWR extends the traditional regression framework by allowing local rather than global parameters to be estimated. Regarding the choice of the weighting system W(u_i), the majority of software follows an adaptative kernel decoded in Eq. 3 (Bocci et al., 2007). A fixed kernel may be another option where b is a fixed vicinity distance.

(3)

where, b is the distance between i and the Nth nearest neighbor (between 8 and 16 neighbors is a good start). Hence, this kernel function distance varies in space and presents an adaptive bandwidth depending on the data points' density: b is relatively small in areas where the data points are densely distributed and the bandwidth is relatively large where the data points are sparsely distributed.

Charlton and Fotheringham (2009) use the corrected Akaike Information Criterion (Eq. 4) in the GWR as a measure of goodness of fit. Two separate models being compared are held to be equivalent if the difference between the two AICc values is less than 3. The AICc value can also be used to determine the optimal value of the kernel bandwidth (the lowest, the better).

(4)

where, n is the number of observations in the dataset; is the estimate of the standard deviation of the residuals; and tr(S) is the trace of the hat matrix.

As stated by Lloyd (2007), the goodness-of-fit of a GWR model can also be assessed using the geographically weighted coefficient of determination: R_i² = (TSS^w-RSS^w)/TSS^w where TSS^w denotes the geographically weighted total sum of squares:

and RSS represents the geographically weighted residual sum of squares:

FINAL THOUGHTS

Spatial autocorrelation and statistical heterogeneity hold the ability to compare two regions and to characterize texture differences. Quite often, distant pairs are less similar (competitive spatial processes) than closer ones (cooperative spatial processes). Probably, some landscapes can exhibit extremely irregular shapes. As a consequence, indices of spatial autocorrelation calculated globally and locally are valuable for descriptive purposes because they provide a measure of how similar objects are to their spatial neighbors. This spatial dependence impact is also crucial on spatial inference interpolation such as Kriging, spatial simulation and geographical regression.

The word Kriging is synonymous with the optimal prediction of unknown values from observed data at known locations (Journel and Huijbregts, 1978; Aunon and Hernandez, 2000). After the variogram has been defined, the algebraic relationship between values at different distances is used to estimate Kriging weights. Mostly, four factors are taken into account in assigning weights to the spatial observations: closeness to the location being estimated, redundancy between data values (clustering), anisotropy (direction) and magnitude of continuity.

Generally, the estimation of missing spatial data when undertaking GWR for discrete data, Kriging and spatial autocorrelation lead to a close linkage among them: the missing data issue (Griffith and Layne, 1999). Spatial autocorrelation can also be used with spatial prediction. For instance, a high degree of spatial autocorrelation suggests an equally likely chance of predicting neighboring values. Also, a low value reveals a low level of spatial data redundancy.

Eight relationships emerge among these concepts (Griffith and Layne, 1999):

APPENDIX

Table A1:	The Pb dataset (99 samples): Contamination data of Aljustrel, Portugal, within a global area of 4500 mx2950 m

Fig. A1:	Histogram, cumulative distribution functions, box-plot and descriptive statistics of the Pb dataset. Clearly, it follows a positive asymmetric distribution

Fig. A2:	Spatial distribution of the Pb contamination dataset. The attribute has a more continuous spatial pattern from East to West, thus it is anisotropic

Fig. A3:	Experimental variograms according to four directions plus the omnidirectional one with spherical models fitted

Fig. A4:	Ordinary Kriging estimation (a) and Kriging variance (b) maps. As an uncertainty measure, OK variance reflects the geometry of the observations but not the variability among them