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@PhDThesis{Ferreira:2023:CoNuEv,
               author = "Ferreira, Willian Jos{\'e}",
                title = "Contribui{\c{c}}{\~a}o das nuvens para eventos de 
                         amplifica{\c{c}}{\~a}o da irradi{\^a}ncia solar ultravioleta 
                         medida em superf{\'{\i}}cie",
               school = "Instituto Nacional de Pesquisas Espaciais (INPE)",
                 year = "2023",
              address = "S{\~a}o Jos{\'e} dos Campos",
                month = "2023-08-25",
             keywords = "radia{\c{c}}{\~a}o ultravioleta, nuvens, {\'o}ptica 
                         instrumental, sensoriamento remoto da atmosfera, ultraviolet 
                         radiation, clouds, instrumental optics, remote sensing of the 
                         atmosphere.",
             abstract = "A radia{\c{c}}{\~a}o ultravioleta (RUV, 100-400 nm) impulsiona 
                         numerosos processos fotoqu{\'{\i}}micos e fotobiol{\'o}gicos na 
                         superf{\'{\i}}cie terrestre, cabendo {\`a}s nuvens o papel de 
                         seu principal modulador atmosf{\'e}rico, em raz{\~a}o das 
                         varia{\c{c}}{\~o}es de curto per{\'{\i}}odo que promovem na 
                         irradi{\^a}ncia medida em superf{\'{\i}}cie. No entanto, 
                         in{\'u}meras vezes ao dia, Eventos de Amplifica{\c{c}}{\~a}o da 
                         Radia{\c{c}}{\~a}o Solar (EARS) fazem com que a irradi{\^a}ncia 
                         ultravioleta (UV) supere a irradi{\^a}ncia medida em 
                         condi{\c{c}}{\~a}o de c{\'e}u n{\~a}o encoberto por nuvens. 
                         Neste trabalho, quantificou-se a contribui{\c{c}}{\~a}o das 
                         nuvens para EARS, em S{\~a}o Jos{\'e} dos Campos (23,20º S, 
                         45,86º W, 621 m), a partir de irradi{\^a}ncias espectrais UV em 
                         seis comprimentos de onda (305 nm, 313 nm, 320 nm, 340 nm, 380 nm, 
                         395 nm) e banda PAR (Radia{\c{c}}{\~a}o Fotossint{\'e}tica 
                         Ativa, 400- 700 nm) obtidas em superf{\'{\i}}cie e imagens do 
                         c{\'e}u. Os eventos foram detectados quando o fator de 
                         modifica{\c{c}}{\~a}o das nuvens apresentou diferen{\c{c}}as 
                         maiores que dois erros-padr{\~a}o entre a irradi{\^a}ncia 
                         espectral medida em condi{\c{c}}{\~o}es de c{\'e}us com nuvens 
                         e a irradi{\^a}ncia de refer{\^e}ncia. A an{\'a}lise da 
                         ocorr{\^e}ncia de EARS em v{\'a}rias bandas de RUV e PAR revelou 
                         um aumento no n{\'u}mero de eventos {\`a} medida que o 
                         comprimento de onda aumenta, onde, de 1.735 EARS observados, a 
                         radia{\c{c}}{\~a}o UV-B (305nm) representa 6,0% do total, 
                         enquanto a UV-A (340 nm) e banda PAR representam 17,5% e 30,5%, 
                         respectivamente. Verificou-se que h{\'a} 99,6% de chances dos 
                         EARS serem observados com dura{\c{c}}{\~a}o de at{\'e} 5 
                         minutos, ocorrendo aumentos mais acentuados na primavera e no 
                         ver{\~a}o, e mais proeminentes na regi{\~a}o do UV-A e PAR do 
                         que no UV-B. Identificou-se que EARS em {\^a}ngulo solar de 
                         z{\^e}nite (ASZ) de 30º a 35º ocorrem, principalmente, devido a 
                         nuvens Cumulus e Stratus, mas tamb{\'e}m por nuvens de m{\'e}dia 
                         altitude, do tipo Altocumulus e Altostratus. Para ASZ de 45º a 
                         55º, as amplifica{\c{c}}{\~o}es, em sua maioria, s{\~a}o 
                         associadas a Altostratus e Cirrus. Por{\'e}m, no ver{\~a}o, 
                         quando associadas a Cumulus e Stratocumulus, essas nuvens s{\~a}o 
                         capazes de gerar aumentos de curta dura{\c{c}}{\~a}o que podem 
                         chegar a 70% no caso do UV-B (305 nm). Tamb{\'e}m foi 
                         quantificado o n{\'u}mero de pixels brilhantes das nuvens por 
                         meio da utiliza{\c{c}}{\~a}o do par{\^a}metro de brilho do 
                         espa{\c{c}}o de cores HSV, modelo que expressa as cores em termos 
                         do matiz, satura{\c{c}}{\~a}o e valor. Apesar da aus{\^e}ncia 
                         de correla{\c{c}}{\~a}o entre irradi{\^a}ncia e 
                         varia{\c{c}}{\~a}o de brilho de nuvens durante os EARS nas 
                         diferentes faixas de comprimento de onda medidas em 
                         superf{\'{\i}}cie, {\'e} crucial desenvolver algoritmos 
                         preditores para estudos futuros. Considerando os impactos dos EARS 
                         na dose di{\'a}ria de radia{\c{c}}{\~a}o, em geral, a 
                         radia{\c{c}}{\~a}o adicional em eventos prolongados equivale a 
                         cerca de 5% do total. Embora a contribui{\c{c}}{\~a}o dos 
                         eventos possa parecer insignificante, considerou-se que o aumento 
                         repentino do {\'{\I}}ndice Ultravioleta (IUV) ao longo do tempo 
                         tem o potencial de afetar o meio ambiente e agravar os indicadores 
                         de sa{\'u}de em diversas regi{\~o}es. ABSTRACT: Ultraviolet 
                         radiation (RUV, 100-400 nm) drives numerous photochemical and 
                         photobiological processes at the Earth's surface, with clouds 
                         playing the role of the main atmospheric modulator due to the 
                         short-term variations in surface irradiance they induce. However, 
                         many times a day, radiation enhancement events (REE) cause 
                         ultraviolet (UV) irradiance to exceed that measured under 
                         clear-sky conditions. This study quantified the cloud contribution 
                         to REE at S{\~a}o Jos{\'e} dos Campos (23.20º S, 45.86º W, 621 
                         m) using UV spectral irradiances at six wavelengths (305 nm, 313 
                         nm, 320 nm, 340 nm, 380 nm, 395 nm) and the PAR band 
                         (Photosynthetically Active Radiation, 400-700 nm) obtained at the 
                         surface, as well as sky images. Events were detected when the 
                         cloud modification factor showed differences greater than two 
                         standard errors between the spectral irradiance measured under 
                         cloudy conditions and the reference irradiance. Evaluation of the 
                         occurrence of REE in different RUV and PAR bands showed an 
                         increase in the number of events with longer wavelengths, with 
                         UV-B radiation (305 nm) making up 6.0% of the 1,735 REE observed, 
                         while UV-A (340 nm) and PAR bands accounted for 17.5% and 30.5%, 
                         respectively. It was found that there is a 99.6% chance of 
                         observing REE up to 5 minutes in duration, with more pronounced 
                         increases in spring and summer, and more pronounced increases in 
                         the UV-A and PAR regions than in the UV-B region. REE with a solar 
                         zenith angle (SZA) of 30º to 35º are mainly caused by cumulus and 
                         stratus clouds, but also by mid-level clouds such as altocumulus 
                         and altostratus. For SZA of 45º to 55º, most enhancements are 
                         associated with altostratus and cirrus clouds. However, in summer, 
                         when associated with cumulus and stratocumulus clouds, these 
                         clouds can produce short term enhancements that can reach up to 
                         70% in the case of UV-B (305 nm). The number of bright cloud 
                         pixels was also quantified using the brightness parameter in the 
                         HSV color space model, which expresses colors in terms of hue, 
                         saturation, and value. Although no statistical correlation was 
                         found between surface spectral irradiance and cloud brightness 
                         variation during REE for any of the wavelengths evaluated, it was 
                         considered critical to develop predictive algorithms for spectral 
                         irradiance and reference brightness under cloudy sky conditions 
                         for future research. The effect of the extended REE on the daily 
                         radiation dose is about 5% of the total. Despite the apparent 
                         insignificance, a sustained increase in the UV index could have an 
                         impact on the environment and worsen health indicators in 
                         different regions.",
            committee = "Alves, Maria Virginia (presidente) and Alval{\'a}, 
                         Pl{\'{\i}}nio Carlos (orientador) and Silva, Abel Ant{\^o}nio 
                         da (orientador) and Echer, Ezequiel and Gobbi, Delano and 
                         Pinheiro, Damaris Kirsch and Martins, Fernando Ramos",
         englishtitle = "Contribution of cloudiness to solar ultraviolet irradiance 
                         enhancement events measured at the surface",
             language = "pt",
                pages = "134",
                  ibi = "8JMKD3MGP3W34T/49P9NS5",
                  url = "http://urlib.net/ibi/8JMKD3MGP3W34T/49P9NS5",
           targetfile = "publicacao.pdf",
        urlaccessdate = "16 jun. 2024"
}


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