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Article

Monitoring Olive Oil Mill Wastewater Disposal Sites Using Sentinel-2 and PlanetScope Satellite Images: Case Studies in Tunisia and Greece

by
Wissal Issaoui
1,2,*,
Dimitrios D. Alexakis
3,
Imen Hamdi Nasr
1,2,
Athanasios V. Argyriou
3,
Evangelos Alevizos
3,
Nikos Papadopoulos
3 and
Mohamed Hédi Inoubli
2
1
Department of Earth Sciences, Faculty of Sciences of Bizerte, Carthage University, Jarzouna, Bizerte 7021, Tunisia
2
UR-GAMM, Faculty of Sciences of Tunis, University of El Manar, Tunis 2092, Tunisia
3
Laboratory of Geophysical-Satellite Remote Sensing and Archaeoenvironment, Institute for Mediterranean Studies, Foundation for Research and Technology-Hellas (FORTH), 74100 Rethymno, Greece
*
Author to whom correspondence should be addressed.
Agronomy 2022, 12(1), 90; https://doi.org/10.3390/agronomy12010090
Submission received: 22 November 2021 / Revised: 23 December 2021 / Accepted: 27 December 2021 / Published: 30 December 2021

Abstract

:
Mediterranean countries are known worldwide for their significant contribution to olive oil production, which generates large amounts of olive mill wastewater (OMW) that degrades land and water environments near the disposal sites. OMW consists of organic substances with high concentrations of phenolic compounds along with inorganic particles. The aim of this study is to assess the effectiveness of satellite image analysis techniques using multispectral satellite data with high (PlanetScope, 3 × 3 m) and medium (Sentinel-2, 10 × 10 m) spatial resolution to detect Olive Mill Wastewater (OMW) disposal sites, both in the SidiBouzid region (Tunisia) and in the broader Rethymno region on the island of Crete, (Greece). Documentation of the sites was carried out by collecting spectral signatures of OMW at temporal periods. The study integrates the application of a variety of spectral vegetation indices (VIs), such as the Normalized Difference Vegetation Index (NDVI), in order to evaluate their efficiency in detecting OMW disposal areas. Furthermore, a set of image-processing methods was applied on satellite images to improve the monitoring of OMW ponds including the false-color composites (FCC), the Principal Component Analysis (PCA), and image fusion. Finally, different classification algorithms, such as the ISODATA, the maximum likelihood (ML), and the Support Vector Machine (SVM) were applied to both satellite images in order to assist in the overall approach to effectively detect the sites. The results obtained from different approaches were compared, evaluating the efficiency of Sentinel-2 and PlanetScope images to detect and monitor OMW disposal areas under different morphological environments.

1. Introduction

There are about 750 million productive olive trees worldwide, with 735 million of them being located in the Mediterranean region, contributing more than 97% of the olive oil world’s production. The four major olive oil producers around the world, are Spain (36%), Italy (24%), Greece at (17%) and Tunisia (8.5%) [1]. However, the olive oil production cycle generates large amounts of solid wastes and wastewater that pose a significant environmental risk due to their high phytotoxicity resulting from increased concentrations of inorganic constituents [2,3,4]. Uncontrolled disposal of olive mill wastewater in ponds can result in soil contamination caused by leachate of wastewater with high biochemical oxygen (40–95 g/L) and chemical oxygen demand (50–180 g/L), leading to phytotoxicity due to high concentration in phenolic compounds [3].
Nevertheless, a few studies have treated the negative effects of these hazardous wastes on soil microbes [5] and water environments [6,7]. OMW disposal sites cause important environmental problems, such as the odd smell due to evaporation of ammonia and the infiltration of the organic and inorganic materials that flow in different levels of soil, eventually reaching the ground water [8]. For this reason, Bailey et al. [9] indicated the vital necessity to have specific strategies in order to resolve and control OMW sites.
Remote sensing technologies are efficient methods for monitoring and mapping land cover and land use changes [10,11]. Earth Observation (EO) data have been used to monitor and map land use to meet the expanding requests for fundamental human needs and welfare [11,12,13]. In this concept, several studies have employed satellite images for monitoring environmental parameters, especially water bodies, that are affected mainly by severe anthropogenic activities [14,15]. In the recent past, satellite remote sensing integrated with a compilation of in situ spectral signature libraries have been also utilized to identify and monitor OMW disposal sites [4,16].
This work focuses on two different sites in the Mediterranean region (Tunisia and Greece) that face significant environmental pollution issues due to unsupervised disposal of OMW. The goal of this study is to assess the capability of remote sensing data to identify and map OMW disposal sites through the application of various established image-processing techniques applied in different satellite products, such as Sentinel-2 and PlanetScope.

2. Materials and Methods

2.1. Study Areas and Satellite Imagery

Olive groves have covered extended areas in coastal and semi-mountainous areas in Crete since the last quarter of the 20thcentury [17]. Crete is known for intensive agricultural activities where the olive industry represents a major component of its economy (Figure 1a). More than 1000 OMW ponds are located on the island and had been detected in the past using the Global Navigation Satellite Systems (GNSS) and the Geographical Information Systems (GIS) [4].
The second study area is located in the middle part of the Tunisian republic (Figure 1b). It has been chosen as a study area for its considerable contribution to the cultivation of olives and production of olive oil in the country [18]. This region is the fourth in Tunisia in terms of number of mills, with mill-density around 1 mill/100 km2. SidiBouzid is ranked as the second place in Tunisia in terms of annual oil production, totaling to about 90,000 m3 [19]. The olive groves have expanded constantly, covering 36% of the total area (254,245 ha in total), while the climate in the region is arid.
A number of medium- and high-resolution satellite images were analyzed in this study. Particularly, eight Sentinel-2 (L1C) images and eight PlanetScope images of the SidiBouzidand Rethymno areas were obtained and evaluated for their efficiency in OMW monitoring (Table 1 and Table 2). The images’ temporal acquisition period consisted of February, April, August, and October 2020.
The European Space Agency (ESA) launched, in 2015 and 2017, two satellites (S-2A and S-2B) for the Sentinel-2 mission, comprising the second environmental monitoring plan for the mission of Copernicus [20]. The Multi-Spectral Instrument (MSI) sensor that is embedded inboth satellites provides a spatial resolution of 10–60 m, according to band wavelength. The Sentinel-2 mission provides open access to image data for the global land surface with a six-day revisit period. For the needs of the study, Sentinel-2 (L1C)data were used.
The PlanetScope mission was launched in November 2018 and its constellation of approximately 130 satellites covers extensive surface areas on a daily basis (200 million km2/day). PlanetScope imagery is characterized by improved spectral and spatial resolutions, (up to 3 m), offering an increased applicability in temporal coverage of the Earth’s surface with high spatial resolution.
The last generation of PlanetScope is presently in orbit and yields restricted numbers of images with five spectral bands (Blue, Green, Red, NIR, and Red Edge). For the needs of the study, Level 3B Ortho Scene data were incorporated. The overall hierarchical structure of the methodology is described in Figure 2.

2.2. Satellite Imagery Processing Techniques

In this study, several data-preparation steps were implemented in order to convert the initial satellite images into useful descriptive layers that maximize the identification of OMW ponds during the image analysis process.
Concerning the Sentinel-2 L1C data, the digital number (DN) was converted first to radiance and then to reflectance. Moreover, atmospheric correction was applied to Sentinel-2images. Darkest pixel (DP) is a prompt and precise atmospheric correction technique that is applied through the application of dark and non-variant targets detected in satellite images [21,22]. In our study, lakes and dams were utilized as non-variant targets for that purpose. Concerning Planetscope imageries, the Level 3B Ortho Scene concerns orthorectified reflectance data that are atmospherically corrected using 6SV2.1 radiative transfer code and MODIS NRT data.

2.3. False-Color Composites

The selection of the optimum band combination for detecting OMW ponds was carried out using various False-Color Composites (FCC). Thus, the optimum index factor (OIF) was calculated to find out the best combination of three bands via the testing of three correlation coefficients and standard deviations according to Equation (1) [23].
OIF = i = 1 3 S D i j = 1 3 A C C j
where SDi is the standard deviation of band I and ACCj is the absolute value of the correlation coefficient linking any two of the feasible pairs, j.

2.4. Principal Component Analysis

Principal component analysis (PCA) was applied to all Sentinel-2 and PlanetScope datasets to improve the overall interpretation of satellite images in terms of OMW detection. PCA is an image analysis technique that transforms originally correlated bands into a set of uncorrelated principal components, organized in a descending scale referring to the degree of the original contained information [24]. This technique was implemented to optimize the size of the dataset (i.e., the dimensionality of the original bands) by combining the information collected from the original bands into the reduced number of the final principal components.

2.5. Spectral Signatures Collection

Spectral signature collection is an essential method used to monitor OMW during different time periods. In this context, band spectral signatures were collected for the two sensors, analyzed for their sensitivity to detect OMW ponds in both study areas for different temporal periods, and finally, were statistically compared. Specifically, to assess spectral pair bands of both satellite images (Sentinel-2 and PlanetScope)in terms of their minimum spectral correlation, a Euclidean distance computation was calculated for all the spectral signatures [4], as shown below (Equation (2)).
D ( x , y ) = i = 1 n ( xi yi ) 2
where xi and yi are two different points.
At this step, a proximity matrix was developed for all spectral signatures in order to measure the spectral vectors of every channel at different dates (Table 3 and Table 4).

2.6. SpectralIndices

Efficient, remote-sensing monitoring of OMW disposal sites merely depends on the surrounding land cover [25]. Numerous OMW areas are established at remote locations and are encompassed by vegetation barriers to ensure that they are secured, roofed, and that they prevent bad odors and visual interruption from adjoining settlements. Thus, various spectral indices were applied to monitor the OMW and increase the spectral difference between OMW areas and adjoining vegetation surfaces. NDVI represents the normalized ratio of red and near-infrared band Equation (3).
N D V I = Red   band NIR   band Red   band + NIR   band
Besides NDVI, the NDWI (Normalized Difference Water Index) (Equation (4)) has been calculated as well, following the normalized ratio between green and near-infrared reflectance for both satellite images in order to detect the liquid part of waste areas. Equation (4) has been developed by Mc Feeters [26] in order to identify the water bodies in wetland areas:
N D W I = Green   band NIR   band Green   band + NIR   band
In addition to the NDVI and NDWI, seven other spectral indices were applied for evaluating their efficiency in enhancing the contrast of the OMW disposal areas with their adjacent areas by applying those in medium- and high-resolution satellite imagery. Initially, the simple ratio (SR) was applied; it combines the red and the near-infrared reflectance data to detect biophysical surfaces [27]. The Renormalized Difference Vegetation Index (RDVI) was applied to linearize the relationship between the index and biophysical parameters. This index was based on the slope of constant index lines in the NIR and red reflectance and it was developed for estimating distances between lines, realizing the parallel lines to each other [28]. Huete [29] developed both the NDVI and the Soil Adjusted Vegetation Index (SAVI) in order to reduce the influence of soil characteristics in the VIs satellite images. A set of developments have been applied to the soil-adjusted vegetation index; the Modified Soil Adjusted Vegetation Index (MSAVI) proposed by Qi et al. [30]; and the Optimized Soil Adjusted Vegetation Index (OSAVI) by Rondeauxet al. [31]. The Difference Vegetation Index (DVI) was proposed by Richardson and Everitt [32] and the Enhanced Vegetation Index (EVI) was developed for incorporating the atmospheric resistance concepts and the background adjustment using feedback based on the NDVI algorithm [33]. EVI is considered to be a modified NDVI by improving the sensitivity of high biomass areas and enhancing the efficiency of vegetation reflectance as referred to atmospheric influence reduction and canopy background [34]. The equations of the spectral indices are analytically described in Table 5.
Further analysis was implemented for evaluating the contrast of OMW disposal areas with areas in the vicinity; a sensitivity analysis parameter was calculated in order to measure the spectral optimization level of images by applying the vegetation indices to satellite images [4].Thus, two sets of spectral responses (OMW disposal areas and non-occupied neighborhood areas) were calculated in order to measure the sensitivity analysis of vegetation indices (relative difference of the two patterns %) using both sensors for different case studies and time periods.

2.7. Image Classification Algorithms

Both supervised and unsupervised algorithms were applied in order to assist in the effective monitoring of OMW sites. Initially, the ISODATA unsupervised classification algorithm was applied in order to group each pixel to a cluster according to the Euclidean distance parameter [36]. Additionally, satellite images were processed with the Maximum Likelihood (ML) classification algorithm [37]. ML classification is a widely-applied method in remote sensing that has shown increased performance in classifying datasets with a large number of classification variables [38,39,40]. In order to test an additional classification technique, the Support Vector Machine (SVM) was applied as well [41]. The main concept of the SVM algorithm is to determine a hyperplane that optimally separates two classes. The SVM algorithm is independent of data dimensionality [42], which is a key feature when using many spectral bands or when ancillary data are included in the classification process, as is the case of OMW [43]. Previous studies tested SVM and evaluated its performance using pixel-based image classification with very good results [44,45,46,47].
Both Sentinel-2 (acquired during February and August) and PlanetScope (acquired during February and August) images were processed for all study areas. The following image composites were incorporated in the classification: (a) Composite 1, using band2, band3, band4, and band8 for Sentinel-2 and band1, band2, band3, and band4 for PlanetScope, (b) Composite 2, using NDVI, NDWI, RGB, and PCA bands (first component applied for RGB-248 and RGB-234 for Sentinel-2 and PlanetScope, respectively) [4], and (c) Composite 3, our proposed image composite obtained through the application of Principal Component Analysis (PCA) to RGB, NDVI, and NDWI layers.

3. Results

3.1. False-Color Composites

Figure 3 shows that the optimum band combination applied to enhance the OMW disposal areas was calculated using RGB-248 for Sentinel-2 images and RGB-234 for PlanetScope datasets. The higher value of the OIF was recorded for the images acquired during October for both study areas (Figure 3). Thus, those RGB composites were selected as optimal for being used in the further processing steps.

3.2. PCA Analysis

The results indicated that the PCA approach (Figure 4) improved the spectral contrast of the OMW ponds compared to their neighborhood terrain by detecting OMW places for the majority of cases and therefore increased the ability of Sentinel-2 and PlanetScope images to identify the OMW disposal sites.

3.3. Spectral Signatures Collection

The results indicated that thePlanetScope signature response was slightly higher than those of Sentinel-2 (Figure 5). However, both diagrams of spectral signature analysis show high reflectance values corresponding to their chlorophyll content through the NIR band, that is, band 4 in PlanetScope and band 8 in Sentinel-2. PlanetScope can provide more discrete details in terms of reflectance values of OMW disposal areas than the Sentinel-2 imagery. In addition, it was proved that for images from both satellites, the higher sensitivity of OMW reflectance in NIR was indicated for images acquired during February when the olive wastes were exposed in the ponds.
The Euclidean distance results for Sentinel-2 showed that the most prominent spectral differences are between bands B3/B8 for both study areas. That is, the Green/NIR increases the sensitivity of these bands in detecting the chlorophyll. Concerning the PlanetScope data, the Euclidean distance revealed that the ratio between bands B1/B4 highlights the greatest spectral differences in both study areas in different time periods. This is identical to the results of Alexakis et al. [4], who analyzed the corresponding spectral difference that was detected in OMW sites between bands B5/B2 using Landsat-8.
DISentinel-2 = f (Green band, NIR band)
DIPlanetScope = f (Blue band, NIR band)
Equations (12) and (13) were defined by Equations (14) and (15) through the normalization of the difference of spectral signatures of the two selected bands in order to optimize the contribution of detection indices in identifying OMW areas and to enhance the radiometric response of imagery.
DI Sentinel - 2 = NIRband Greenband NIRband + Greenband
DI PlanetScope = NIR   band   Blue   band NIR   band + Blue   band

3.4. SpectralIndices

The NDVI and NDWI diagrams (Figure 6) reveal the fact that the spectral response of the two sensors is almost identical; OMW areas are liquid in February and April (rich in vegetal substance of olive mill wastewater) and solid (dry) in August and October. Thus, the high values of NDWI correspond to the operation period between February and April.
In the following charts, the results of relative differences of spectral indices were evaluated. Concerning Sentinel-2, the NDVI, NDWI, and DI show high sensitivity values between OMW disposal sites and their neighborhood areas (the difference is greater than 30%) for both study areas during February and April rather than August and October. PlanetScope imagery also shows equivalent responses compared to the Sentinel-2 results on both areas of study. Nonetheless, the calculated NDVI, NDWI, and DI revealed higher reflectance differences between each OMW site and its adjacent area during February and April (decreased in August and October).Thus, these are considered to be the optimum indices for enhancing the contrast between the inner and the outside parts of OMW disposal areas for both case studies. In addition, the sensitivity of PlanetScope seems to be more promising compared to Sentinel-2 (i.e., the difference of DI reaches 70% for PlanetScope and 50% for Sentinel-2 in the Greek case study) (Figure 7).

3.5. Image Analysis Classification

3.5.1. Unsupervised Classification

Regarding the case study in Tunisia, the ISODATA classification performed rather well in identifying OMW areas using both Sentinel-2 and PlanetScope data. This may be attributed to the smooth landscape morphology of the study area. Comparing results for both Composite 2 and Composite 3, the ISODATA classification algorithm seems to work better for Composite 3 in differentiating the OMW ponds from adjacent areas (i.e., residential areas). This applies for the ISODATA unsupervised classification in the Greek study area as well. Moreover, several false positive results were shown in different parts of Sentinel-2 images after applying the ISODATA algorithm. These may have been caused by the shadows on the images and the mountainous morphology in the vicinity of the OMW areas. At this stage, it seems that the use of Planetscope images is more effective for applying the ISODATA unsupervised classification to detect OMW areas and decrease false spectral responses compared to Sentinel-2 images. The results show that February is the best time period for differentiating the OMW ponds from its adjacent areas. This is due to the liquid wastes residue during this period [4].
Consecutively, Composite 3 seems to work better than Composite 1 and Composite 2 for both satellites’ imagery and for both study areas. Therefore, Composite 3 was selected and used in the following classification analysis process. In fact, spatio-temporal changes in OMW areas, such as turning from a dry to liquid texture, influence the output of the ISODATA algorithm (Figure 8 and Figure 9).

3.5.2. Supervised Classification

Apart from unsupervised classification, we further considered applying the maximum likelihood (ML) and the support vector machine (SVM) classifiers using ground truth data for validation. The application of the ML classification method for the case study of Tunisia showed promising results in detecting the OMW disposal areas using Sentinel-2 and PlanetScope, respectively (Figure 10). Once again, the results from satellite images acquired during February were more effective in differentiating OMW from all adjacent areas (such as roads) by using Composite 3. This can be attributed to the flat terrain morphology of the specific study area that assisted both medium- and high-resolution satellites to identify OMW disposal areas.
For the study area in Greece, results show that the ML classification was not able to detect OMW sites in both satellite images. This is probably due to its mountainous and complex morphology (Figure 11).
The SVM classification outputs yielded good results for both satellite images in the two case study areas, detecting OMW disposal areas especially when Composite 3 with images acquired during February was used. Specifically, as it is shown in Figure 12, the SVM algorithm produces better results when PlanetScope imagery is used for both areas.
Concerning overall quantitative analysis, Kappa index was selected for evaluating the performance of the different classifiers [48]. It is a robust tool that can be estimated easily from the confusion (or error) matrix that is widely used in the classification accuracy assessment [49,50].
A detailed scale was proposed by Sakiyama et al. [51], giving the degree of accordance linked to the kappa values. Kappa values inferior to 0.4 indicate a poor accordance and kappa values equal and superior to 0.4 indicate a good accordance. Consecutively, Table 6 shows that the SVM classification is the most efficient algorithm for detecting and differentiating OMW disposal areas; so, the kappa index value of 0.653 using Composite 3 of Sentinel-2 and the kappa index value of 0.604 using Composite 3 of PlanetScope images are computed for the case study of Tunisia, and kappa values of 0.571 for Sentinel-2 and 0.510 for PlanetScope were respectively compiled for the Greek area. This is followed by the ML classification using Composite 3 with a kappa value of 0.384 for Sentinel-2 and 0.295 for PlanetScope in the study area in Tunisia. The ISODATA classification becomes third. This highlights the fact that the SVM classifier provided the optimum results for both sensors and both case studies applied to Composite 3, using imagery acquired during February 2020.

4. Discussion

The study outcomes highlight the fact that low-cost remote sensing proved to be a powerful tool for effective monitoring of OMW ponds on a regional scale. In this study, different satellite image analysis algorithms were applied for: (a) enhancing the quality of image interpretation, (b) improving the quality of satellite images and (c) detecting and monitoring OMW areas. OMW spectral signatures were collected and the performance of various spectral indices was assessed in discriminating OMW disposal areas from surrounding areas during different time periods. In addition, detection and differentiation of OMW disposal sites from adjacent areas were also carried out by applying different vegetation indices and both unsupervised and supervised classification algorithms to various image composites. The final results were compared with images from the two satellite sensors, for both case studies and for various time periods in order to detect the ideal dataset and period for detecting OMW areas. Specifically, examination of spectral signatures concluded that the optimum bands for monitoring OMW are the NIR bands, represented by band 8 for Sentinel-2 and band 4 for PlanetScope. In addition, the efficiency of NDVI, NDWI, and DI indices for monitoring OMW disposal areas for a spatial-temporal variable frame was highlighted and confirmed the role of the mentioned VIs by Alexakis et al. [4]. The application of different image analysis algorithms indicated that PCA analysis can be effectively used for mapping OMW ponds. Furthermore, the SVM classification algorithm showed optimum performance in differentiating and identifying OMW sites from neighbor areas, as it was proved by Agapiou et al. [16]. It is noteworthy to mention that, within our research, Composite 3 was used with images acquired during the winter period (February 2020). In addition, it was proved that the Tunisian case study, (with a more simplified terrain morphology), is a more suitable pilot area compared to the mountainous Greek case study.
Furthermore, the final results showed that the freely available satellite images of medium spatial resolution, such as Sentinel-2, can be efficiently used for monitoring OMW disposal areas. Although the performance of Planetscope images, in most cases, was better, the response of Sentinel-2 can be described as successful.

5. Conclusions

Remote-sensing techniques offer supplementary advantages compared to in situ observations and reduce the overall costs of environmental monitoring. The OMW disposal sites represent a vital environmental issue for the Mediterranean region and especially for the SidiBouzid region, (Tunisia) and the island of Crete, (Greece). The enormous amount of OMWs generated annually from olive oil production suggest that optimum treatment is an inevitable necessity.
This research highlights the use of satellite time-series imagery for monitoring OMW disposal sites in the Mediterranean region. The final results indicated that the integrated use of various image processing algorithms contribute significantly to OMW monitoring. The innovation of the specific work lays on the fact that for the very first time, satellite imageries of different spatial resolution (Sentinel-2 and PlanetScope) and corresponding image analysis algorithms are compared for their efficiency and applied in completely different landscape environments. The results indicate that, under certain circumstances, the freely distributed Copernicus data (Sentinel-2) can offer an optimum alternative in multi-temporal environmental surveillance. In this concept, the high-resolution satellite image data, such as PlanetScope, constitute an ideal solution for monitoring earth surface from space.
In the near future, the research team will carry out additional research in both study areas by using sampling and chemical analysis in order to associate olive mill wastewater spectral signatures with specific contaminant types. In addition, we plan to elaborate the use of UAV/drones in the overall research in order to improve substantially the spatial analysis of the acquired images.

Author Contributions

Conceptualization, W.I., D.D.A. and I.H.N.; methodology, W.I. and D.D.A.; software, W.I., D.D.A. and E.A.; validation, W.I., D.D.A., N.P. and M.H.I.; formal analysis, A.V.A.; investigation, W.I. and D.D.A.; resources, W.I., D.D.A. and A.V.A.; data curation, W.I., D.D.A. and A.V.A., writing—original draft, W.I., D.D.A., A.V.A., E.A., N.P., I.H.N. and M.H.I., writing review and editing, W.I., D.D.A., A.V.A., E.A., N.P., I.H.N. and M.H.I. supervision, D.D.A. and M.H.I. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Conflicts of Interest

The authors declare no conflict of interest.

Availability of Data and Material

The data sets generated during and/or analyzed during the current study are available from the corresponding author on reasonable request.

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Figure 1. (a) Greek study areas, (red circle: OMW disposal areas), (b) Tunisian study areas, (red circle: OMW disposal areas).
Figure 1. (a) Greek study areas, (red circle: OMW disposal areas), (b) Tunisian study areas, (red circle: OMW disposal areas).
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Figure 2. Hierarchical structure of methodology and satellite image data processing.
Figure 2. Hierarchical structure of methodology and satellite image data processing.
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Figure 3. (a): Sentinel-2 RGB image (RGB-248) in 25/February/2020, Tunisian study areas, (b): Sentinel-2 RGB image (RGB-248) in 26/August/2020, Tunisian study areas, (c): PlanetScope RGB image (RGB-234) in 25/February/2020, Tunisian study areas, (d): PlanetScope RGB image (RGB-234) in 25/August/2020, Tunisian study areas, (e): Sentinel-2 RGB image (RGB-248) in 25/February/2020, Greek study area, (f): Sentinel-2 RGB image (RGB-248) in 18/August/2020, Greek study areas, (g): PlanetScope RGB image (RGB-234) in 25/February/2020, Greek study areas, (h): PlanetScope RGB image (RGB-234) in 18/August/2020, Greek study areas. The simple false-color composite fails to depict the OMW disposal areas efficiently for Greek study areas (indicated inside the red frame).
Figure 3. (a): Sentinel-2 RGB image (RGB-248) in 25/February/2020, Tunisian study areas, (b): Sentinel-2 RGB image (RGB-248) in 26/August/2020, Tunisian study areas, (c): PlanetScope RGB image (RGB-234) in 25/February/2020, Tunisian study areas, (d): PlanetScope RGB image (RGB-234) in 25/August/2020, Tunisian study areas, (e): Sentinel-2 RGB image (RGB-248) in 25/February/2020, Greek study area, (f): Sentinel-2 RGB image (RGB-248) in 18/August/2020, Greek study areas, (g): PlanetScope RGB image (RGB-234) in 25/February/2020, Greek study areas, (h): PlanetScope RGB image (RGB-234) in 18/August/2020, Greek study areas. The simple false-color composite fails to depict the OMW disposal areas efficiently for Greek study areas (indicated inside the red frame).
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Figure 4. Results of the application of PCA method to the image shown in Figure 3 (Sentinel-2 and PlanetScope, Tunisian and Greek study areas). (a): Sentinel-2 PCA composite (RGB-248 band 2, band 4, band8) in 25/February/2020, Tunisian study areas, (b): Sentinel-2 PCA composite (band 2, band 4, band8) in 26/August/2020, Tunisian study areas, (c): PlanetScope PCA composite (band 2, band 3, band4) in 25/February/2020, Tunisian study areas, (d): PlanetScope PCA composite (band 2, band 3, band4) in 25/August/2020, Tunisian study areas, (e): Sentinel-2 PCA composite (band 2, band 4, band8) in 25/February/2020, Greek study areas, (f): Sentinel-2 PCA composite (band 2, band 4, band8) in 18/August/2020, Greek study areas, (g): PlanetScope PCA composite (band 2, band 3, band4) in 25/February/2020, Greek study areas, (h): PlanetScope PCA composite (band 2, band 3, band4) in 18/August/2020, Greek study areas.
Figure 4. Results of the application of PCA method to the image shown in Figure 3 (Sentinel-2 and PlanetScope, Tunisian and Greek study areas). (a): Sentinel-2 PCA composite (RGB-248 band 2, band 4, band8) in 25/February/2020, Tunisian study areas, (b): Sentinel-2 PCA composite (band 2, band 4, band8) in 26/August/2020, Tunisian study areas, (c): PlanetScope PCA composite (band 2, band 3, band4) in 25/February/2020, Tunisian study areas, (d): PlanetScope PCA composite (band 2, band 3, band4) in 25/August/2020, Tunisian study areas, (e): Sentinel-2 PCA composite (band 2, band 4, band8) in 25/February/2020, Greek study areas, (f): Sentinel-2 PCA composite (band 2, band 4, band8) in 18/August/2020, Greek study areas, (g): PlanetScope PCA composite (band 2, band 3, band4) in 25/February/2020, Greek study areas, (h): PlanetScope PCA composite (band 2, band 3, band4) in 18/August/2020, Greek study areas.
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Figure 5. Spectral signature of OMW disposal areas.
Figure 5. Spectral signature of OMW disposal areas.
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Figure 6. NDVI and NDWI mean values of OMW disposal sites for Tunisian and Greek studies areas; (a): NDVI mean values of wastes areas using Sentinel-2, (b): NDWI mean values of wastes areas using Sentinel-2, (c) NDVI mean values of wastes areas using PlanetScope, and (d): NDWI mean values of wastes areas using PlanetScope.
Figure 6. NDVI and NDWI mean values of OMW disposal sites for Tunisian and Greek studies areas; (a): NDVI mean values of wastes areas using Sentinel-2, (b): NDWI mean values of wastes areas using Sentinel-2, (c) NDVI mean values of wastes areas using PlanetScope, and (d): NDWI mean values of wastes areas using PlanetScope.
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Figure 7. Spectral indices performance; (a): Sentinel-2 spectral indices performance for Tunisian study areas, (b): Sentinel-2 spectral indices performance for Greek study areas, (c): PlanetScope spectral indices performance for Tunisian study areas, (d): PlanetScope spectral indices performance for Greek study areas.
Figure 7. Spectral indices performance; (a): Sentinel-2 spectral indices performance for Tunisian study areas, (b): Sentinel-2 spectral indices performance for Greek study areas, (c): PlanetScope spectral indices performance for Tunisian study areas, (d): PlanetScope spectral indices performance for Greek study areas.
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Figure 8. ISODATA classification for Tunisian study areas; (a): unsupervised classification using Sentinel-2 RGB image in February, (b): unsupervised classification using Sentinel-2 RGB image in August, (c): unsupervised classification using Sentinel-2 Composite 3 in February, (d): unsupervised classification using Sentinel-2 Composite 3 in August, (e): unsupervised classification using PlanetScope RGB image in February, (f): unsupervised classification using PlanetScope RGB image in August, (g): unsupervised classification using PlanetScope Composite 3 in February, (h): unsupervised classification using PlanetScope Composite 3 in August, (i): unsupervised classification using Sentinel-2 Composite 1 image in February; OMW disposal areas are indicated inside the red frame.
Figure 8. ISODATA classification for Tunisian study areas; (a): unsupervised classification using Sentinel-2 RGB image in February, (b): unsupervised classification using Sentinel-2 RGB image in August, (c): unsupervised classification using Sentinel-2 Composite 3 in February, (d): unsupervised classification using Sentinel-2 Composite 3 in August, (e): unsupervised classification using PlanetScope RGB image in February, (f): unsupervised classification using PlanetScope RGB image in August, (g): unsupervised classification using PlanetScope Composite 3 in February, (h): unsupervised classification using PlanetScope Composite 3 in August, (i): unsupervised classification using Sentinel-2 Composite 1 image in February; OMW disposal areas are indicated inside the red frame.
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Figure 9. ISODATA classification for Greek study areas; (a): unsupervised classification using Sentinel-2 RGB image in February, (b): unsupervised classification using Sentinel-2 RGB image in August, (c): unsupervised classification using Sentinel-2 Composite 3 in February, (d): unsupervised classification using Sentinel-2 Composite 3 in August, (e): unsupervised classification using PlanetScope RGB image in February, (f): unsupervised classification using PlanetScope RGB image in August, (g): unsupervised classification using PlanetScope Composite 3 in February, (h): unsupervised classification using PlanetScope Composite 3 in August, (i): unsupervised classification using Sentinel-2 Composite 1 image in February; OMW disposal areas are indicated inside the red frame.
Figure 9. ISODATA classification for Greek study areas; (a): unsupervised classification using Sentinel-2 RGB image in February, (b): unsupervised classification using Sentinel-2 RGB image in August, (c): unsupervised classification using Sentinel-2 Composite 3 in February, (d): unsupervised classification using Sentinel-2 Composite 3 in August, (e): unsupervised classification using PlanetScope RGB image in February, (f): unsupervised classification using PlanetScope RGB image in August, (g): unsupervised classification using PlanetScope Composite 3 in February, (h): unsupervised classification using PlanetScope Composite 3 in August, (i): unsupervised classification using Sentinel-2 Composite 1 image in February; OMW disposal areas are indicated inside the red frame.
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Figure 10. Maximum likelihood classification for Tunisian study areas; (a): ML classification using Sentinel-2 RGB image in February, (b): ML classification using Sentinel-2 RGB image in August, (c): ML classification using Sentinel-2 Composite 3 in February, (d): ML classification using Sentinel-2 Composite 3 in August, (e): ML classification using PlanetScope RGB image in February, (f): ML classification using PlanetScope RGB image in August, (g): ML classification using PlanetScope Composite 3 in February, (h): ML classification using PlanetScope Composite 3 in August; OMW disposal areas are indicated inside a red frame.
Figure 10. Maximum likelihood classification for Tunisian study areas; (a): ML classification using Sentinel-2 RGB image in February, (b): ML classification using Sentinel-2 RGB image in August, (c): ML classification using Sentinel-2 Composite 3 in February, (d): ML classification using Sentinel-2 Composite 3 in August, (e): ML classification using PlanetScope RGB image in February, (f): ML classification using PlanetScope RGB image in August, (g): ML classification using PlanetScope Composite 3 in February, (h): ML classification using PlanetScope Composite 3 in August; OMW disposal areas are indicated inside a red frame.
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Figure 11. Maximum likelihood classification for Greek study areas; (a): ML classification using Sentinel-2 RGB image in February, (b): ML classification using Sentinel-2 RGB image in August, (c): ML classification using Sentinel-2 Composite 3 in February, (d): ML classification using Sentinel-2 Composite 3 in August, (e): ML classification using PlanetScope RGB image in February, (f): ML classification using PlanetScope RGB image in August, (g): ML classification using PlanetScope Composite 3 in February, (h): ML classification using PlanetScope Composite 3 in August; OMW disposal areas are indicated inside the red frame.
Figure 11. Maximum likelihood classification for Greek study areas; (a): ML classification using Sentinel-2 RGB image in February, (b): ML classification using Sentinel-2 RGB image in August, (c): ML classification using Sentinel-2 Composite 3 in February, (d): ML classification using Sentinel-2 Composite 3 in August, (e): ML classification using PlanetScope RGB image in February, (f): ML classification using PlanetScope RGB image in August, (g): ML classification using PlanetScope Composite 3 in February, (h): ML classification using PlanetScope Composite 3 in August; OMW disposal areas are indicated inside the red frame.
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Figure 12. SVM classification for Tunisian study areas; (a): SVM classification using Sentinel-2 RGB image in February, (b): SVM classification using Sentinel-2 Composite 3 in February, (c): SVM classification using PlanetScope RGB image in February, (d): SVM classification using PlanetScope Composite 3 in February, (e): SVM classification using Sentinel-2 Composite 1 image in February. OMW disposal areas are indicated inside the red frame.
Figure 12. SVM classification for Tunisian study areas; (a): SVM classification using Sentinel-2 RGB image in February, (b): SVM classification using Sentinel-2 Composite 3 in February, (c): SVM classification using PlanetScope RGB image in February, (d): SVM classification using PlanetScope Composite 3 in February, (e): SVM classification using Sentinel-2 Composite 1 image in February. OMW disposal areas are indicated inside the red frame.
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Table 1. Satellite sensor specifications.
Table 1. Satellite sensor specifications.
BandsDescriptionCentral Wavelength (μm)Resolution (m)
Sentinel-2
Band 1Coastal aerosol0.44360
Band 2Blue0.49010
Band 3Green0.56010
Band 4Red0.66510
Band 5Vegetation Red Edge0.70520
Band 6Vegetation Red Edge0.74020
Band 7Vegetation Red Edge0.78320
Band 8NIR0.84210
Band 8AVegetation Red Edge0.86520
Band 9Water vapor0.94560
Band 10SWIR-Cirrus1.37560
Band 11SWIR1.61020
Band 12SWIR2.19020
Planetscope
Band 1Blue0.455–0.5153
Band 2Green0.500–50.903
Band 3Red0.590–0.6703
Band 4NIR0.780–0.8603
Table 2. Satellite imageacquisition dates.
Table 2. Satellite imageacquisition dates.
Tunisian Study AreaGreek Study Area
Sentinel-2 images25 February 202025 February 2020
28 April 202017 April 2020
26 August 202018 August 2020
02 October 202002 October 2020
PlanetScope images25 February 202025 February 2020
28 April 202017 April 2020
25 August 202018 August 2020
02 October 202003 October 2020
Table 3. Euclidean distance using Sentinel-2; (a): Tunisian study areas, (b): Greek study areas.
Table 3. Euclidean distance using Sentinel-2; (a): Tunisian study areas, (b): Greek study areas.
B2B3B4B8 B2B3B4B8
B20.0000.0490.0240.361B20.0000.0220.0100.220
B30.0490.0000.0520.408B30.0220.0000.0250.240
B40.0240.0520.0000.358B40.0100.0250.0000.217
B80.3610.4080.3580.000B80.2200.2400.2170.000
February (a)April (a)
B2B3B4B8 B2B3B4B8
B20.0000.0250.0170.021B20.0000.0170.0260.065
B30.0250.0000.0110.030B30.0170.0000.0210.067
B40.0170.0110.0000.020B40.0260.0210.0000.047
B80.0210.0300.0200.000B80.0650.0670.0470.000
August (a)October (a)
B2B3B4B8 B2B3B4B8
B20.0000.0200.0650.225B20.0000.0230.0660.266
B30.0200.0000.0450.244B30.0230.0000.0460.284
B40.0650.0450.0000.287B40.0660.0460.0000.329
B80.2250.2440.2870.000B80.2660.2840.3290.000
February (b)April (b)
B2B3B4B8 B2B3B4B8
B20.0000.0070.0230.258B20.0000.0190.0190.172
B30.0070.0000.0280.263B30.0190.0000.0090.190
B40.0230.0280.0000.243B40.0190.0090.0000.188
B80.2580.2630.2430.000B80.1720.1900.1880.000
August (b)October (b)
Table 4. Euclidean distance using PlanetScope; (a): Tunisian study areas, (b): Greek study areas.
Table 4. Euclidean distance using PlanetScope; (a): Tunisian study areas, (b): Greek study areas.
B1B2B3B4 B1B2B3B4
B10.0000.0620.1580.559B10.0000.0370.1140.394
B20.0620.0000.0980.499B20.0370.0000.0770.358
B30.1580.0980.0000.401B30.1140.0770.0000.284
B40.5590.4990.4010.000B40.3940.3580.2840.000
February (a)April (a)
B1B2B3B4 B1B2B3B4
B10.0000.0850.1600.299B10.0000.0660.1340.229
B20.0850.0000.0750.215B20.0660.0000.0690.164
B30.1600.0750.0000.140B30.1340.0690.0000.096
B40.2990.2150.1400.000B40.2290.1640.0960.000
August (a)October (a)
B1B2B3B4 B1B2B3B4
B10.0000.0220.0220.236B10.0000.0240.0320.234
B20.0220.0000.0020.214B20.0240.0000.0090.210
B30.0220.0020.0000.215B30.0320.0090.0000.203
B40.2360.2140.2150.000B40.2340.2100.2030.000
February (b)April (b)
B1B2B3B4 B1B2B3B4
B10.0000.0220.0380.273B10.0000.0370.0630.227
B20.0220.0000.0170.251B20.0370.0000.0250.190
B30.0380.0170.0000.235B30.0630.0250.0000.165
B40.2730.2510.2350.000B40.2270.1900.1650.000
August (b)October (b)
Table 5. Equations of different spectral indices used.
Table 5. Equations of different spectral indices used.
IndicesEquations
SR NIR   band Red   band ;(5)
RDVI NIR   band Red   band ( NIR   band + Red   band ) ;(6)
SAVI ( 1 + L ) ( Red   band NIR   band ) ( NIR   band + Red   band + L ) ;(7)
MSAVI 0.5     ( ( 2   NIR   band + 1 )   ( ( 2 NIR   band ) 2   8 ( NIR   band     Red   band ) ) ;(8)
OSAVI 1.16   NIR   band Red   band NIR   band + Red   band + 0.16 ;(9)
DVINIR band − a ∗ Red band;(10)
EVI G   NIR   band Red   band NIR   band + ( C 1 Red   band C 2 Blue   band ) + F ;(11)
where the NIR band is reflectance in the NIR part of spectrum; the Red band is the reflectance in the red part of spectrum; the Blue band is the reflectance in the blue part of spectrum;.a = 0.96916, L = 0.5 [32]; F is a soil adjustment factor, and C1 and C2 are coefficients used to correct aerosol scattering in the red band using the blue band. In general, G = 2.5, C1 = 6.0, C2 = 7.5, and F = 1 [35].
Table 6. Results of kappa index calculated for images acquired during February for different classification algorithms.
Table 6. Results of kappa index calculated for images acquired during February for different classification algorithms.
Classification AlgorithmSatellite SensorTunisian Study AreaGreek Study Area
ISODATASentinel-2SC = 0.246
PCA = 0.394
_
PlanetScopeSC = 0.154
PCA = 0.294
SC = 0.047
PCA = 0.190
MLSentinel-2SC = 0.077
PCA = 0.384
_
PlanetScopeSC = 0.134
PCA = 0.295
_
SVMSentinel-2SC = 0.574
PCA = 0.653
SC = 0.653
PCA = 0.571
PlanetScopeSC = 0.616
PCA = 0.604
SC = 0.618
PCA = 0.510
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Issaoui, W.; Alexakis, D.D.; Nasr, I.H.; Argyriou, A.V.; Alevizos, E.; Papadopoulos, N.; Inoubli, M.H. Monitoring Olive Oil Mill Wastewater Disposal Sites Using Sentinel-2 and PlanetScope Satellite Images: Case Studies in Tunisia and Greece. Agronomy 2022, 12, 90. https://doi.org/10.3390/agronomy12010090

AMA Style

Issaoui W, Alexakis DD, Nasr IH, Argyriou AV, Alevizos E, Papadopoulos N, Inoubli MH. Monitoring Olive Oil Mill Wastewater Disposal Sites Using Sentinel-2 and PlanetScope Satellite Images: Case Studies in Tunisia and Greece. Agronomy. 2022; 12(1):90. https://doi.org/10.3390/agronomy12010090

Chicago/Turabian Style

Issaoui, Wissal, Dimitrios D. Alexakis, Imen Hamdi Nasr, Athanasios V. Argyriou, Evangelos Alevizos, Nikos Papadopoulos, and Mohamed Hédi Inoubli. 2022. "Monitoring Olive Oil Mill Wastewater Disposal Sites Using Sentinel-2 and PlanetScope Satellite Images: Case Studies in Tunisia and Greece" Agronomy 12, no. 1: 90. https://doi.org/10.3390/agronomy12010090

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