Fechar

@PhDThesis{Petri:2024:EfIlSo,
               author = "Petri, Caio Arlanche",
                title = "Efeitos de ilumina{\c{c}}{\~a}o solar em atributos 
                         espectro-espaciais da constela{\c{c}}{\~a}o planetscope obtidos 
                         na Amaz{\^o}nia",
               school = "Instituto Nacional de Pesquisas Espaciais (INPE)",
                 year = "2024",
              address = "S{\~a}o Jos{\'e} dos Campos",
                month = "2023-12-15",
             keywords = "constela{\c{c}}{\~o}es de sat{\'e}lites, ilumina{\c{c}}{\~a}o 
                         solar, alta resolu{\c{c}}{\~a}o espacial, Amaz{\^o}nia, 
                         satellite constellations, solar illumination, high spatial 
                         resolution, Amazon.",
             abstract = "Estudos fenol{\'o}gicos da vegeta{\c{c}}{\~a}o por 
                         sensoriamento remoto orbital na Amaz{\^o}nia s{\~a}o limitados 
                         pela pouca disponibilidade de dados multitemporais, com 
                         observa{\c{c}}{\~o}es de alta resolu{\c{c}}{\~a}o espacial 
                         regularmente espa{\c{c}}adas no tempo. O recente advento das 
                         constela{\c{c}}{\~o}es de sat{\'e}lites poder{\'a} suprir 
                         parte destas limita{\c{c}}{\~o}es. No entanto, quando a alta 
                         resolu{\c{c}}{\~a}o espacial {\'e} utilizada em estudos de 
                         fenologia das florestas tropicais da Amaz{\^o}nia, os efeitos das 
                         condi{\c{c}}{\~o}es de ilumina{\c{c}}{\~a}o solar e do terreno 
                         podem ser cr{\'{\i}}ticos para a determina{\c{c}}{\~a}o de 
                         alguns atributos espaciais e espectrais das imagens. N{\~a}o 
                         h{\'a}, contudo, estudos que abordem os efeitos de 
                         ilumina{\c{c}}{\~a}o solar em dados de constela{\c{c}}{\~o}es 
                         de sat{\'e}lites obtidos ao nadir na Amaz{\^o}nia. Este 
                         trabalho, portanto, teve como objetivo a investiga{\c{c}}{\~a}o 
                         de efeitos da geometria de ilumina{\c{c}}{\~a}o solar em dados 
                         de alta resolu{\c{c}}{\~a}o espacial obtidos pela 
                         constela{\c{c}}{\~a}o PlanetScope (PS) em florestas tropicais da 
                         Amaz{\^o}nia. Para isso, utilizaram-se s{\'e}ries temporais, 
                         compostas por um total de 493 imagens PS, livres de cobertura 
                         nuvens. As imagens foram obtidas entre os anos de 2017 e 2019 
                         sobre 12 {\'a}reas de estudo, abrangendo regi{\~o}es ao norte e 
                         ao sul deste bioma. O processo anal{\'{\i}}tico baseou-se na 
                         observa{\c{c}}{\~a}o da geometria de ilumina{\c{c}}{\~a}o 
                         solar, durante a aquisi{\c{c}}{\~a}o de dados PS na 
                         esta{\c{c}}{\~a}o seca (Junho a Setembro), e das 
                         rela{\c{c}}{\~o}es entre {\^a}ngulos solares com: (i) atributos 
                         espectrais de imagens PS, representados por valores de 
                         reflect{\^a}ncia, {\'{\i}}ndices de vegeta{\c{c}}{\~a}o (IVs) 
                         (Enhanced Vegetation Index - EVI e Normalized Difference 
                         Vegetation Index - NDVI), brilho da vegeta{\c{c}}{\~a}o, 
                         determinado da an{\'a}lise por componentes principais (ACP) e por 
                         fra{\c{c}}{\~o}es-sombra extra{\'{\i}}das de um modelo linear 
                         de mistura espectral {{{(MLME);}}} e (ii) atributos espaciais de 
                         imagens PS, representados por m{\'e}tricas de textura Gray-Level 
                         Co-occurrence Matrix (GLCM). Os resultados mostraram que o aumento 
                         no {\^a}ngulo zenital solar (AZS) e a redu{\c{c}}{\~a}o no 
                         {\^a}ngulo azimutal solar (AAS), em dire{\c{c}}{\~a}o ao final 
                         da esta{\c{c}}{\~a}o seca, produziu um incremento consistente na 
                         reflect{\^a}ncia das quatro bandas do PS, especialmente na banda 
                         do infravermelho pr{\'o}ximo (IVP). De forma concordante, o 
                         brilho da vegeta{\c{c}}{\~a}o aumentou de junho para setembro, 
                         conforme registrado pelos valores da primeira componente principal 
                         (CP1). O EVI, {\'{\i}}ndice mais anisotr{\'o}pico e fortemente 
                         dependente da reflect{\^a}ncia do IVP, apresentou valores mais 
                         altos em dire{\c{c}}{\~a}o a setembro, acompanhando as 
                         varia{\c{c}}{\~o}es nos {\^a}ngulos solares. O NDVI, ao 
                         contr{\'a}rio, foi pouco correlacionado com estes {\^a}ngulos. A 
                         m{\'e}dia da textura GLCM apresentou incremento do 
                         in{\'{\i}}cio para o final da esta{\c{c}}{\~a}o seca, enquanto 
                         a vari{\^a}ncia da textura diminuiu no mesmo per{\'{\i}}odo. 
                         Foram observadas correla{\c{c}}{\~o}es estatisticamente 
                         significantes entre as m{\'e}tricas de textura GLCM e os 
                         {\^a}ngulos solares. O EVI apresentou alta correla{\c{c}}{\~a}o 
                         com a m{\'e}dia GLCM da textura da banda do IVP do PS, ao 
                         contr{\'a}rio do observado para o NDVI. As 
                         fra{\c{c}}{\~o}es-sombra, resultantes das varia{\c{c}}{\~o}es 
                         de ilumina{\c{c}}{\~a}o entre as copas das {\'a}rvores e no 
                         terreno, diminu{\'{\i}}ram na dire{\c{c}}{\~a}o do final da 
                         esta{\c{c}}{\~a}o seca. Estas fra{\c{c}}{\~o}es foram 
                         correlacionadas com o EVI, mas n{\~a}o com o NDVI. Em geral, os 
                         resultados destacaram a import{\^a}ncia da corre{\c{c}}{\~a}o 
                         dos efeitos de ilumina{\c{c}}{\~a}o solar e, em alguns casos, de 
                         ilumina{\c{c}}{\~a}o do terreno, se IVs anisotr{\'o}picos como 
                         o EVI forem utilizados em estudos de fenologia da 
                         vegeta{\c{c}}{\~a}o com dados de alta resolu{\c{c}}{\~a}o 
                         espacial do PS. ABSTRACT: Vegetation phenological studies using 
                         orbital remote sensing in the Amazon are hampered by the limited 
                         availability of high spatial resolution data and the analysis of 
                         regularly spaced time series observations. The recent advent of 
                         satellite constellations may overcome some of these limitations. 
                         However, when high spatial resolution is used in phenology studies 
                         of Amazonian tropical forests, the effects of solar and terrain 
                         illumination conditions can be important in determining spatial 
                         and spectral attributes from images. In this scenario, there are 
                         currently no studies addressing the effects of solar illumination 
                         on data from satellite constellations obtained at nadir in the 
                         Amazon. This work aimed to investigate the effects of solar 
                         illumination geometry on high spatial resolution data obtained by 
                         the PlanetScope (PS) constellation in tropical forests of the 
                         Amazon. A time series from a total of 493 PS cloud-free images was 
                         used. The images were obtained between 2017 and 2019 over 12 study 
                         areas, covering regions from the north and south of this biome. 
                         The analytical process was based on the observation of solar 
                         illumination geometry during the acquisition of PS data in the dry 
                         season (June to September), and the relationships between solar 
                         angles with: (i) spectral attributes of PS images, represented by 
                         reflectance values, vegetation indices (VIs) (Enhanced Vegetation 
                         Index - EVI and Normalized Difference Vegetation Index - NDVI), 
                         vegetation brightness, determined from a principal component 
                         analysis (PCA), and shade fractions extracted from a linear 
                         spectral mixture model {{{(LSMM);}}} and (ii) spatial attributes 
                         of PS images, represented by Gray-Level Co-occurrence Matrix 
                         (GLCM) texture metrics. The results showed that the increase in 
                         the solar zenith angle (SZA) and the reduction in the solar 
                         azimuth angle (SAA), towards the end of the dry season, produced a 
                         consistent increase in the reflectance of the four PS bands, 
                         especially in the near-infrared band (NIR). Concordantly, 
                         vegetation brightness increased from June to September, as 
                         recorded by the scores of the first principal component (PC1). The 
                         EVI, a more anisotropic index and strongly dependent on NIR 
                         reflectance, showed higher values towards September, following 
                         variations in solar angles. NDVI, on the contrary, was poorly 
                         correlated with these angles. The average GLCM texture increased 
                         from the beginning to the end of the dry season, while the texture 
                         variance decreased in the same period. Statistically significant 
                         correlations were observed between GLCM texture metrics and solar 
                         angles. The EVI showed a high correlation with the GLCM average of 
                         the PS NIR band texture, contrary to what was observed for the 
                         NDVI. Shade fractions, resulting from variations in illumination 
                         of tree canopies and terrain, decreased towards the end of the dry 
                         season. These fractions were correlated with EVI, but not with 
                         NDVI. Overall, the results highlighted the importance of 
                         correcting for solar illumination effects, and in some cases 
                         terrain illumination, if anisotropic VIs such as EVI are to be 
                         used in vegetation phenology studies with high spatial resolution 
                         data of PS.",
            committee = "K{\"o}rting, Thales Sehn (presidente) and Galv{\~a}o, Lenio 
                         Soares (orientador) and Arag{\~a}o, Luiz Eduardo de Oliveira e 
                         Cruz de (orientador) and Moura, Yhasmin Mendes and Breunig, 
                         F{\'a}bio Marcelo",
         englishtitle = "Solar illumination effects on spectral-spatial attributes of the 
                         planetscope constellation obtained in the Amazon",
             language = "pt",
                pages = "96",
                  ibi = "8JMKD3MGP3W34T/4AH9P78",
                  url = "http://urlib.net/ibi/8JMKD3MGP3W34T/4AH9P78",
           targetfile = "publicacao.pdf",
        urlaccessdate = "07 maio 2024"
}


Fechar