Abstract

Radiometric precision is difficult to maintain in orbital images due to several factors (atmospheric conditions, Earth-sun distance, detector calibration, illumination, and viewing angles). These unwanted effects must be removed for radiometric consistency among temporal images, leaving only land-leaving radiances, for optimum change detection. A variety of relative radiometric correction techniques were developed for the correction or rectification of images, of the same area, through use of reference targets whose reflectance do not change significantly with time, i.e., pseudo-invariant features (PIFs). This paper proposes a new technique for radiometric normalization, which uses three sequential methods for an accurate PIFs selection: spectral measures of temporal data (spectral distance and similarity), density scatter plot analysis (ridge method), and robust regression. The spectral measures used are the spectral angle (Spectral Angle Mapper, SAM), spectral correlation (Spectral Correlation Mapper, SCM), and Euclidean distance. The spectral measures between the spectra at times t1 and t2 and are calculated for each pixel. After classification using threshold values, it is possible to define points with the same spectral behavior, including PIFs. The distance and similarity measures are complementary and can be calculated together. The ridge method uses a density plot generated from images acquired on different dates for the selection of PIFs. In a density plot, the invariant pixels, together, form a high-density ridge, while variant pixels (clouds and land cover changes) are spread, having low density, facilitating its exclusion. Finally, the selected PIFs are subjected to a robust regression (M-estimate) between pairs of temporal bands for the detection and elimination of outliers, and to obtain the optimal linear equation for a given set of target points. The robust regression is insensitive to outliers, i.e., observation that appears to deviate strongly from the rest of the data in which it occurs, and as in our case, change areas. New sequential methods enable one to select by different attributes, a number of invariant targets over the brightness range of the images.

Highlights

  • Spectral images acquired from the same area at different times contain valuable information for regular monitoring of the Earth’s surface, allowing us to describe the land-cover evolution, vegetation phenology, and natural hazard events

  • A PIF selection with less points should adopt a threshold with a high value to the SCMCD method; low angles from Spectral Angle Mapper for change detection (SAMCD), and low Euclidean Distance for change detection (EDCD) values

  • In order to emphasize the results of this method for the figure, the original data are regarded as input, rather than points previously selected using spectral measurements

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Summary

Introduction

Spectral images acquired from the same area at different times contain valuable information for regular monitoring of the Earth’s surface, allowing us to describe the land-cover evolution, vegetation phenology, and natural hazard events. It is difficult to maintain radiometric accuracy in orbital images due to changes in atmospheric conditions, Earth-Sun distance, detector calibration, illumination angles, viewing angles, and sensor oscillation, as are required in order to highlight the spectral changes of interest. Another common problem in change-detection analysis from different sensors, such as Landsat Thematic Mapper (TM) and Landsat Enhanced Thematic Mapper plus (ETM+) images is that they, require the evaluation of radiometric consistency between sensors to ensure comparability between the temporal images [1,2]. The radiometric properties of an image are adjusted to match a reference image [7,8], image normalization uses a histogram-matching method [9] or a linear-regression method [10]

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