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Radiometric correction effects in Landsat multi‐date/multi‐sensor change detection studies

, , , &
Pages 685-704 | Published online: 22 Feb 2007
 

Abstract

Radiometric corrections serve to remove the effects that alter the spectral characteristics of land features, except for actual changes in ground target, becoming mandatory in multi‐sensor, multi‐date studies. In this paper, we evaluate the effects of two types of radiometric correction methods (absolute and relative) for the determination of land cover changes, using Landsat TM and Landsat ETM+ images. In addition, we present an improvement made to the relative correction method addressed. Absolute correction includes a cross‐calibration between TM and ETM+ images, and the application of an atmospheric correction protocol. Relative correction normalizes the images using pseudo‐invariant features (PIFs) selected through band‐to‐band PCA analysis. We present a new algorithm for PIFs selection in order to improve normalization results. A post‐correction evaluation index (Quadratic Difference Index (QD)), and post‐classification and change detection results were used to evaluate the performance of the methods. Only the absolute correction method and the new relative correction method presented in this paper show good post‐correction and post‐classification results (QD index ≈ 0; overall accuracy >80%; kappa >0.65) for all the images used. Land cover change estimations based on uncorrected images present unrealistic change rates (two to three times those obtained with corrected images), which highlights the fact that radiometric corrections are necessary in multi‐date multi‐sensor land cover change analysis.

Acknowledgements

This paper was funded by grants from CONICET (Consejo Nacional de Investigaciones Científicas y Técnicas), Argentina and MAE‐AECI (Ministerio de Asuntos Exteriores‐Agencia Española de Cooperación Internacional), Spain. Satellite images were provided by CONAE (Comisión Nacional de Avtividades Espaciales), Argentina as part of a L. Paolini's A.O. project. The work presented in this paper was carried out while L. Paolini was a visiting researcher at the Global Change Unit (Universitat de Valencia, Spain) and at the Instituto de Astronomía y Física del Espacio (CONICET, Argentina), whose support is gratefully acknowledged. The authors would like to thank Dr. Héctor R. Grau for his helpful suggestions and comments.

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