404 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 43, NO. 2, FEBRUARY 2005 for their given application. Obviously, “RMSE” is an important index for geometric accuracy. Therefore, it is suggested that the RMSE, area omission error, and area commission error should be used for the majority of applications. Level III: Shape similarity indexes (corner difference, perimeter difference, area difference, and moment-derived shape similarity). Some applications such as cadastral management may have shape similarity requirements. The first three indexes are easy to calculate and can be used to roughly estimate the shape similarity. The moment-derived index has a robust theoretical background and is more rigorous. Certain applications such as building visualization may require shape similarity assessments. For three-dimensional building evaluation, some of the indexes can be directly used (detect rate, correctness, corner difference). RMSE can be calculated using x, y, z coordinates. As well, a three-dimensional index can be defined to represent the volume difference between the extracted building and the reference. Similarly, the area omission and commission errors can be replaced by volume omission and commission errors. V. CONCLUSION A comprehensive building accuracy assessment approach has been presented. Unlike the more popular assessment approaches that only rely on building counts, this research provides ten quantitative indexes to add to the assessment of extraction completeness, correctness, geometric accuracy, and feature shape similarity. Using only count-based indexes may generate an overoptimistic performance evaluation. Also using too few indexes may allow biased assessment results to be perpetuated. Implementing the proposed ten indexes can evaluate the accuracy of the building extraction process more extensively. Accuracy assessment is a complex task, and different indexes should be combined to provide insight on the implications of inaccuracy from several different perspectives. REFERENCES [1] A. Gruen, E. P. Baltsavias, and O. Henricsson, Automatic Extraction of Man-Made Objects from Aerial and Space Images (II). Basel, Germany: Birkhauser Verlag, 1997. [2] H. Mayer, “Automatic object extraction from aerial imagery: A survey focusing on buildings,” Comput. Vis. Image Understanding, vol. 74, no. 2, pp. 138–149, May 1999. [3] R. Nevaita and A. Huertas, “Research in knowledtge-based automatic feature extraction,” Inst. Robotics Intell. Syst., Univ. Southern California, Los Angeles, Tech. Rep. 00–383, 1999. [Online]. Available: http://iris.usc.edu/Outlines/papers/2000/APGD-final.pdf. [4] T. Kim and J. P. Muller, “A technique for 3D building reconstruction,” Photogramm. Eng. Remote Sens., vol. 64, no. 9, pp. 923–930, Sep. 1998. [5] J. A. Shufelt, “Performance evaluation and analysis of monocular building extraction from aerial imagery,” IEEE Trans. Pattern Anal. Mach. Intell., vol. 21, no. 4, pp. 311–326, Apr. 1999. [6] O. Henricsson and E. Baltsavias, “3-D building reconstruction with ARUBA: A qualitative and quantitative evaluation,” in Proc. Conf. Automatic Extraction of Man-Made Objects from Aerial and Space Images (II), A. Gruen, E. Baltavias, and O. Henricsson, Eds., 1997, pp. 65–76. [7] A. Brunn and U. Weidner, “Hierarchical Bayesian nets for building extraction using dense digital surface models,” ISPRS J. Photogramm. Remote Sens., vol. 53, pp. 296–307, Oct. 1998. [8] S. Theodoridis and K. Koutroumbas, Pattern Recognition. San Diego, CA: Academic, 1999, pp. 245–249. [9] M. K. Hu, “Visual pattern recognition by moment invariants,” IRE Trans. Inf. Theory, vol. IT-8, no. 2, pp. 179–187, Feb. 1962. Accuracy, Reliability, and Depuration of SPOT HRV and Terra ASTER Digital Elevation Models Aurora Cuartero, A. M. Felicísimo, and F. J. Ariza Abstract—The aim of this communication is to study the accuracy and reliability of digital elevation models (DEMs) generated from two different satellite sources [the Terra Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER)] and [the Systeme P’our l’Observation de la Terre (SPOT) High Resolution Visible (HRV)] stereoscopic images), using three different photogrammetric softwares. The main reason of the study is the heterogeneity and absence of agreement found in previous research concerning several significant aspects of DEM generation methods. A set of 91 DEMs were generated from SPOT data and 55 DEMs from ASTER data. Error control was performed with 315 check points determined by differential global positioning systems. Results of Terra ASTER DEMs show that elevation RMSE (root mean square error) equals 13.0 m. The corresponding RMSE value for SPOT HRV DEM is 7.3 m. In both cases, the error is less than the pixel size. Furthermore, this communication proposes a technique to improve DEM structure, based on an objective criterion to cleanse redundancy in DEMs without a significant loss of accuracy. This criterion is based on removing all points with a correlation value below a threshold value. Index Terms—Accuracy, Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), digital elevation model (DEM), High Resolution Visible (HRV), reliability, Systeme P’our l’Observation de la Terre (SPOT), Terra. I. INTRODUCTION A digital elevation model (DEM) can be extracted automatically from stereo satellite images. Numerous applications are based on DEM, and their validity directly depends on the quality of the original elevation data. High-quality DEMs are seldom available, even though photogrammetric technology, the most common to work with DEMs, has been around for a few years. The possibility of using stereoscopic images from satellites for a global digital elevation data production did not arise until the launch of the Systeme P’our l’Observation de la Terre (SPOT) series in 1986. Today, several satellites also offer the possibility for stereoscopic acquisition: SPOT [1], the Modular Optoelectronic Multispectral Stereo Scanner [2], the Indian Remote Sensing satellite, the Korea Multipurpose Satellite, the Advanced Visible and Near-Infrared Radiometer sensor [3], Terra [4], and more recently, the high-resolution pushbroom scanners IKONOS, EROS-A1, QUICKBIRD-2, SPOT 5, and ORBVIEW-3. Thus, some studies focus on constructing DEMs from stereoscopic images by means of high-resolution pushbroom scanners such as IKONOS [5], [6], EROS-A1 [7], and SPOT-5 [8]; furthermore, it is assumed that the automatic generation of a DEM from remotely sensed data with a Z subpixel accuracy is possible [9]. Automation allows the construction of DEMs with an almost randomly large point density. The selection of “very important points,” common in manual processing for the construction of triangulated irregular network (TIN) structures, is not applicable to automatic photogrammetric processes. The result often entails a very “hard” DEM Manuscript received February 26, 2004; revised November 8, 2004. This work was supported in part by the Junta de Extremadura (II Plan Regional de Investigación, Desarrollo Tecnológico e Innovación de Extremadura) and in part by the Fondo Europeo de Desarrollo Regional (FEDER) as part of Project 2PR03A105. A. Cuartero and A. M. Felicísimo are with the University of Extremadura, 10071 Caceres, Spain (e-mail: [email protected]). F. J. Ariza is with the University of Jaén, 23071 Jaén, Spain. Digital Object Identifier 10.1109/TGRS.2004.841356 0196-2892/$20.00 © 2005 IEEE IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 43, NO. 2, FEBRUARY 2005 TABLE I ANTECEDENTS ABOUT SPOT DEM ACCURACY DETERMINATION 405 For this reason, we have conducted a set of experiments that guarantee reliability in error control and analyze factors such as the influence of software, discarded in previous research. III. OBJECTIVES TABLE II ANTECEDENTS ABOUT ASTER DEM ACCURACY DETERMINATION This communication aims to do the following. • Verify the influence of pixel size and stereoscopic capture method (along/cross-track) in DEM accuracy generated from two different sources (Terra ASTER and SPOT HRV). In order to make results more consistent, we have used different photogrammetric software applications: Erdas Imagine with OrthoBase Pro (Leica Geosystems), Geomatica Ortho Engine (PCI Geomatics), and Socet Set (Leica Geosystems). • Propose a method of improvement for the structure of DEM without a loss in accuracy. This process of simplification enables the data structure to be better adapted for integration in a geographical information system (GIS). IV. MATERIAL AND METHODS A. Study Area, Data, and Software where a lot of redundant or unrelevant information can be removed. In a literature review, we could find no references to possible optimization strategies for this phase of the process. Accuracy estimation can be carried out by comparing the DEM data with a set of check points measured by high-precision methods. The basic conditions for a correct work flow are: 1) high accuracy of check points and 2) enough points to guarantee error control reliability. We have examined that most research does not satisfy those conditions. The common sources of check points are topographic contour maps, whose accuracy is not well known (e.g., see Table I). Also, the error control is frequently performed with a number of points that are clearly insufficient to guarantee the test reliability. II. BACKGROUND ON DEM GENERATED FROM SPOT HRV AND TERRA ASTER Deriving DEMs from stereoscopic satellite images is a well-known technique; however, the results of DEM accuracy and the method used to capture the check points and to calculate the reliability differ according to the literature revised. This variation may be due to the method used to estimate error in DEM as much in the number as in the source of check points used. Table I shows some significant examples about accuracy in SPOT DEM. We can see that root mean square error (RMSE) values are very different, varying from 3.3–33 m. The number of check points is also very different, from 6–40, but many authors do not provide information about this issue. Also, other aspects that may be crucial, such as the terrain topography, remain unknown. The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), onboard the National Aeronautics and Space Administration Terra satellite, provides along-track near-infrared stereoscopic images at 15-m resolution. Terra ASTER is a quite recent sensor; thus, there is little research that analyzes the accuracy of DEM generated, mostly on simulated ASTER data [4], [17]. There is little research focusing on possibilities in DEM generation with a variable elevation RMSE between 7–60 m. Table II shows results of research about accuracy in DEM derived from ASTER images. From previous work, we may conclude that the results for both SPOT High Resolution Visible (HRV) and Terra ASTER data are very different. Important questions such as the number of check points and the capture method are not standardized. Some authors do not even inform about control methods. The study area is a 23 km 2 28 km rectangle in Granada (southern Spain). It is an area with a complex topography: steep slopes in the south and flat surfaces in the north. Elevations are in the range 300–2800 m with an average of 1060 m. We have used a pair of panchromatic stereo images SPOT HRV (10-m pixel) and two pairs of Terra ASTER scenes (15-m pixel). The SPOT images were taken on November 2, 1991 and January 2, 1992, and the Terra ASTER images were taken on August 22, 2000. ASTER data were processed with Erdas Imagine and Ortho Engine. Erdas Imagine and Socet Set were used for processing SPOT data. B. DEM Generation The automatic extraction of DEM is facilitated if the specific sensor model information is available. In order to guarantee the most accurate DEM that can provide SPOT HRV and Terra ASTER images, we have analyzed the influence of aspects such as number and spatial distribution of ground control points, the data structure [TIN or uniform regular grid (URG)], and the sample interval. With some applications, the algorithms and correlation coefficient threshold can also be tested. We have conducted several experiments to determine the optimal value of influential variable. We constructed ninety SPOT-derived DEM and 60 ASTER-derived DEM (see the Section V). C. Accuracy and Reliability DEM accuracy is estimated by a comparison with DEM Z values and by contrasting many check points with “true” elevations. The pairwise comparisons allow the calculation of the mean error (ME), RMSE, standard deviation (SD), or similar statistics. The number of check points is an important factor in reliability influencing the range of stochastic variations on the SD values [18]. Another factor is obvious: the accuracy of check points must be sufficient for the control objectives. The estimate of errors in DEM is usually made by following the U.S. Geological Survey recommendation of a minimum of 28 check points [19]. Li [18] showed, however, that many more points are needed to achieve a reliability closer to what is accepted in most statistical tests. The expression that relates reliability to number of check points is R(e) = () 1 2(n 0 1) 2 100% (1) where R e represents the confidence value in percent, and n is the number of check points used in the accuracy test. As an inverse example, if we wish to obtain a SD confidence value of 5%, we need 406 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 43, NO. 2, FEBRUARY 2005 about 100 check points. If we used 28 check points, we would reach a 20% confidence value. Therefore, the number of check points must guarantee stability in error estimates. Revised research is rather heterogeneous regarding number and accuracy of check points, and no author has verified reliability in of these results. Most research used a number of check points that proved clearly insufficient for guaranteeing the validity of error results [14], [16]. One article explained the use of check points from preexisting cartography [10], [11]; this procedure is not recommended, as there tends to be no knowledge about the control map quality itself. Methods based on global position systems (GPS) constitute the ideal source to obtain these points, since they yield the coordinates with great accuracy and also allow to plan a spatially well-distributed sample covering the whole area under analysis. To ensure error reliability, we used a set of 315 randomly distributed check points whose coordinates were determined by differential GPS techniques. We were able to calculate the difference between these points and the elevation values of the DEM, and estimate the ME, SD, and RMSE. The confidence interval (CI) of the standard deviation was also calculated (see Table IV). DEPURATION OF TABLE III DEM SPOT BY CHANGE IN CORRELATION VALUES THE THRESHOLD TABLE IV ERROR STATISTICS FOR DEMS D. DEM Depuration Procedure Due to they very high density of points, digital photogrammetric workstation-generated DEM may attain massive computational sizes. Their integration into a GIS may lead to conflict between these huge data sizes and the analysis, mapping algebra, and simulation operations. Therefore, it would clearly be advisable to avoid a blind inclusion of all of the data deriving from the photogrammetric process and only to take those points that show both good quality and significance in representing the relief. By eliminating poor-quality data, model accuracy can be improved. By eliminating unnecessary data, will be redundancy reduced. Obviously, this process can be applied over TIN structures. Due to fixed cell size, the procedure is not applicable over gridded DEMs. Effectiveness in the characteristic operations of the GIS can be increased by both effects. By use of GIS, the DEM is just one more of the layered variables to be considered. The working hypothesis is that the correlation coefficient associated with each elevation value may be interpreted as a reliability index. If this assumption is correct, we can eliminate the data with a poor correlation value without a significant loss of accuracy. All the accuracy tests were carried out with the set of 315 check points. V. RESULTS A. Accuracy and Reliability Results We constructed 146 DEM, 91 from SPOT images and 55 from ASTER images serving as numerous combinations of variables until reaching the most accurate DEM. A synthesis of the most accurate DEM is given in Table IV, which lists the values of the ME, SD, its , : ), and RMSE. In our case, confidence interval (CI the availability of 315 check points enabled the error control to have a reliability of 96%. Optimal findings include the following. • Erdas Imagine generates the most accurate ASTER-DEM (34.8-m RMSE) using 12 ground control points; and SPOT DEM (7.7-m RMSE) using 14 ground control points. Both are TIN structures. • Geomatica OrthoEngine obtains the best ASTER-DEM (12.6-m RMSE) as a URG structure (30-m cell size), using 15 ground control points. • Socet Set obtains the best SPOT DEM (8.6-m RMSE) as a URG structure (20-m cell size), and using 13 ground control points. = 95% = 0 05 Based on the results obtained in this study, the generation of DEM from Terra ASTER and SPOT HRV stereo images can be done with methods of digital restitution, leading to RMSE values less than the pixel size. The sampling interval is one of the factors that influences the quality of the DEM: The best results are obtained for a cell size twice the pixel size (i.e., 30 m from Terra ASTER; 20 m from SPOT HRV). Increasing of this distance among sampled points is not a good strategy because it is equivalent to a progressive generalization of the DEM structure. The influence of software is obvious from the experiments carried out. Erdas Imagine shows worse results from ASTER data, whereas the accuracy of SPOT DEM is similar for both Erdas and Socet Set. These results may require some explaining. We believe that the main reason is an absence of specific geometric satellite models: Erdas can work with ASTER data, but it forces to the use of a generic model unable to take full advantage of the data. In contrast, we conclude that the SPOT model is fully implemented, and the results are very similar. Ortho Engine includes an ASTER specific model that compensates the shortage of orbital parameters. B. DEM Depuration Results We have conducted the depuration process based on the hypothesis of a certain correspondence between correlation and data reliability: The presence of a low correlation value is not a definitive proof of poor quality, but is a valid warning signal and has statistical significance. The huge DEM (with no points yet removed) was denoted as MDE00. Other DEMs were generated by previously deleting those points whose correlation coefficient was less than a threshold value (Table III). For example, MDE50 was the result of taking a threshold value 0.50 for the correlation coefficient. Table IV shows error evolution versus the correlation coefficient threshold. It can be noted that error did not rise significantly when the number of eliminated points is increased, at least until a correla: ) is reached. : ) or 0.94 (SD tion threshold of 0.93 (SD On moving to 0.95, the quality of the DEM significantly drops (SD = 79 = 80 = IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 43, NO. 2, FEBRUARY 2005 12:2). MDE94 contains only 18.5% of the points of the massive original DEM (MDE00), while the MDE93 contains 23%. We emphasize that the depuration process does not imply an improvement in accuracy statistics, but it contributes to making the structure much more manageable in a GIS environment. VI. CONCLUSION Automated DEM extraction using cross-track SPOT satellite, has been known for 17 years. The addition of along-track ASTER provides an alternative for the extraction of DEM data. In addition, ASTER data are very attractive because they can be downloaded and are very affordable. We concluded that both the along-track Terra ASTER and crosstrack SPOT images will provide the opportunity for the generation of DEMs with RMSE Z values less than the pixel size. We cannot conclude that the accuracy results are affected by other factors such as the stereo capture method (along-track versus cross-track). Photogrammetric programs are not identical. SPOT geometry and data are fully implemented, but ASTER data cause more problems. Geomatica shows good ASTER RMSE values, but blunders are common. Erdas shows bad ASTER RMSE values, but blunders are infrequent. We emphasize the obligatory use of many accurate check points. The use of a very limited number of points implies a very unreliable error control that can make the results useless. We suggest a minimum of 100 points which corresponds to a confidence value of about 0.10. Since quality control procedures are ever required, carrying out the type of tests described in this communication should not be a burden. Instead, this experimentation should be done to “lighten” the DEM before it can be regarded as a finished product. ACKNOWLEDGMENT Thanks to A. Curado for the linguistic revision of this communication. REFERENCES [1] R. Priebbenow and E. E. Clerici, “Cartographic applications of SPOT imagery,” Int. Arch. Photogramm., vol. 37, pp. 289–297, 1988. [2] F. Lanzl, P. Seige, F. Lehmann, and P. Hausknecht, “Using multispectral and stereo MOMS-02 data from the Priroda mission for remote sensing applications,” in Proc. Int. Symp. Spectral Sensing Research, Melbourne, Australia, 1995. 407 [3] T. Hashimoto, “DEM generation from stereo AVNIR image,” Adv. Space Res., vol. 25, pp. 931–936, 2000. [4] R. Welch, T. Jordan, H. Lang, and H. Murakami, “ASTER as a source for topographic data in the late 1990’s,” IEEE Trans. Geosci. Remote Sens., vol. 36, no. 4, pp. 1282–1289, Jul. 1998. [5] R. Li, G. Zhou, S. Yang, G. Tuell, N. J. Schmid, and C. Fowler, “A study of the potential attainable geometric accuracy of IKONOS satellite imagery,” in Proc. 19th ISPRS Congress, Amsterdam, The Netherlands, 2000. [6] T. Toutin, “DEM generation from new VIR sensors: IKONOS, ASTER and Landsat-7,” in Proc. IGARSS, Sydney, Australia, 2001. [7] L. Chen and T. Teo, “Orbit adjuntment for EROS A1 high resolution satellite image,” in Proc. 22nd Asian Conf. Remote Sensing, Singapore, 2001. [8] G. Petrie, “The future direction of the SPOT programme: SPOT–5 International Conference,” in GeoInformatics, vol. 4, 2001, pp. 12–17. [9] P. Krzystek, “New investigations into the practical performance of automatic DEM generation,” in Proc. ACSM/ASPRS Annu. Convention, Charlotte, NC, 1995. [10] Y. Mukai, T. Sugimura, and K. Arai, “Automated generation of digital elevation model using system corrected SPOT data,” in Proc. 23th Int. Symp. Remote Sensing Environment, Bangkok, Thailand, 1990. [11] K. C. Sasowsky and G. W. 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Kääb, “Monitoring high-mountaing terrain deformation from repeated air- and spaceborne optical data: Examples using digital aerial imagery and ASTER data,” ISPRS J. Photogramm. Remote Sens., vol. 57, pp. 39–52, 2002. [16] A. Hirano, R. Welch, and H. Lang, “Mapping from ASTER stereo image data: DEM validation and accuracy assessment,” ISPRS J. Photogramm. Remote Sens., vol. 1255, pp. 1–15, 2003. [17] M. Abrams and S. J. Hook, “Simulated ASTER data for geological studies,” IEEE Trans. Geosci. Remote Sens., vol. 33, no. 3, pp. 692–699, May 1995. [18] Z. Li, “Effects of check point on the reliability of DTM accuracy estimates obtained from experimental test,” Photogrammetric Engineering. [19] USGS, Digital Elevation Models: Data Users. Reston, VA: U.S. Geol. Surv., 1987.
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