Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil

Detalhes bibliográficos
Autor(a) principal: Lopes, Bibiana Culau
Data de Publicação: 2022
Tipo de documento: Tese
Idioma: por
Título da fonte: Manancial - Repositório Digital da UFSM
Texto Completo: http://repositorio.ufsm.br/handle/1/25983
Resumo: Exposure to the sun is fundamental for human health and the growth and development of f lora and fauna, although excessive exposure to the sun’s UV rays can be harmful to all living things. It can affect aquatic and terrestrial animals, plants and can cause serious problems on human health, such as burns, eye damage and long-term exposure can lead to skin cancer and accelerate skin aging. Ozone is the main gas in the Earth’s atmosphere that absorbs UV radiation in the stratosphere. The Antarctic Ozone Hole (AOH) is characterized by an extreme reduction in ozone levels in the Antarctic region in the spring. The secondary effects of the AOH are caused by the displacement of ozone-poor air masses from the polar vortex to the mid-latitudes, including southern Brazil. On this basis, this study aimed to investigate the behavior of solar UV radiation, through the analysis of the UV index collected in southern Brazil (29,4◦ S, 53,8◦ O) using ground (Brewer spectrophotometer) and satellite UV radiation data. The ground-based measurements include UV index, erythemal dose, unweighted UV-B, and daily UV integral. The UV data used covers the period 2005-2017 were compared with observations from the Ozone Monitoring Instrument (OMI) experiment onboard the Aura satellite. Overall, UV radiation in southern Brazil, in Santa Maria, is dominated by the annual seasonal cycle, with a maximum in summer and a minimum in winter. However, very high and even extreme UV indices were measured in spring and fall. Spectral analysis by the wavelet method showed that the variability of UVradiation in southern Brazil is also modulated by 3 forcing: El-Nino Southern Oscillation (ENSO), the Quasi-Biennial Oscillation (QBO) and the solar cycle. As for the influence of anomalies due to the secondary effect of the AOH, we obtained an average reduction of 1% of the total ozone column, with an average increase of 4% of the UV index, under clear-sky condition.
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spelling 2022-08-25T17:52:34Z2022-08-25T17:52:34Z2022-05-13http://repositorio.ufsm.br/handle/1/25983Exposure to the sun is fundamental for human health and the growth and development of f lora and fauna, although excessive exposure to the sun’s UV rays can be harmful to all living things. It can affect aquatic and terrestrial animals, plants and can cause serious problems on human health, such as burns, eye damage and long-term exposure can lead to skin cancer and accelerate skin aging. Ozone is the main gas in the Earth’s atmosphere that absorbs UV radiation in the stratosphere. The Antarctic Ozone Hole (AOH) is characterized by an extreme reduction in ozone levels in the Antarctic region in the spring. The secondary effects of the AOH are caused by the displacement of ozone-poor air masses from the polar vortex to the mid-latitudes, including southern Brazil. On this basis, this study aimed to investigate the behavior of solar UV radiation, through the analysis of the UV index collected in southern Brazil (29,4◦ S, 53,8◦ O) using ground (Brewer spectrophotometer) and satellite UV radiation data. The ground-based measurements include UV index, erythemal dose, unweighted UV-B, and daily UV integral. The UV data used covers the period 2005-2017 were compared with observations from the Ozone Monitoring Instrument (OMI) experiment onboard the Aura satellite. Overall, UV radiation in southern Brazil, in Santa Maria, is dominated by the annual seasonal cycle, with a maximum in summer and a minimum in winter. However, very high and even extreme UV indices were measured in spring and fall. Spectral analysis by the wavelet method showed that the variability of UVradiation in southern Brazil is also modulated by 3 forcing: El-Nino Southern Oscillation (ENSO), the Quasi-Biennial Oscillation (QBO) and the solar cycle. As for the influence of anomalies due to the secondary effect of the AOH, we obtained an average reduction of 1% of the total ozone column, with an average increase of 4% of the UV index, under clear-sky condition.L’exposition au soleil est fondamentale pour la santé humaine, la croissance et le développement de la faune et de la flore, bien que l’exposition excessive aux rayons UV solaires puisse être nocive pour tous les êtres vivants. Elle peut affecter les animaux aquatiques et terrestres, les plantes et peut causer de graves problèmes sur la santé humaine, tels que les brûlures, les lésions oculaires et l’exposition à long terme peut conduire au cancer de la peau et accélère le vieillissement de la peau. L’ozone est le principal gaz de latmosphère terrestre qui absorbe le rayonnement UV dans la stratosphère. Le trou d’ozone antarctique (AOH Antarctic Ozone Hole) se caractérise par une réduction extrême de la teneur en ozone dans la région antarctique au printemps. Les effets secondaires de l’AOH sont causés par le déplacement des masses d’air pauvres en ozone, du vortex polaire vers les latitudes moyennes, y compris le sud du Brésil. Sur cette base, cette étude visait à étudier le comportement du rayonnement UV solaire, par l’analyse de l’indice UV collecté dans le sud du Brésil (29,4ˇrS, 53,8ˇrO) en utilisant des données de rayonnement UV au sol (spectrophotomètre Brewer) et par satellite. Les mesures au sol comprennent l’indice UV, la dose érythémale, les UV-B non-pondérés et l’intégrale quotidienne des UV. Les données UV utilisées couvrant la période 2005-2017 ont été confrontées aux observations de lexpérience OMI (Ozone Monitoring Instrument) embarquée sur le satellite Aura. Globalement, le rayonnement UV au sud du Brésil, à Santa Maria, est dominé par le cycle saisonnier annuel, avec un maximum en été et un minimum en hiver. Cependant, des indices UV très élevés et même extrêmes ont été mesurés au printemps et en automne. L’analyse spectrale par la méthode des ondelettes a montré que la variabilité du rayonnement UV au sud du Brésil est également modulée par 3 forçages : l’oscillation australe El-Nino (ENSO), l’oscillation quasi-biennale (QBO) et le cycle solaire. Quant à linfluence des anomalies dues à leffet secondaire de lAOH, nous avons obtenu une réduction moyenne de 1% de la colonne totale d’ozone, avec une augmentation moyenne de 4% de l’indice UV, dans les conditions de ciel claire.A exposição ao sol é fundamental para a saúde humana e para o crescimento e desenvolvimento da flora e fauna, embora a exposição excessiva aos raios UV do sol possa ser prejudicial a todos os seres vivos. Pode afetar animais aquáticos, terrestres, plantas e pode causar sérios problemas de saúde humana, tais como queimaduras, lesões oculares, a exposição prolongada pode levar ao câncer de pele e acelerar o envelhecimento da pele. O ozônio é o principal gás na atmosfera terrestre que absorve a radiação UV na estratosfera. O Buraco de Ozônio Antártico (BOA) caracteriza-se por uma redução extrema dos níveis de ozônio na região antártica na primavera. Os efeitos secundários da AOH são causados pelo deslocamento de massas de ar pobres em ozônio do vórtice polar para as latitudes médias, incluindo o sul do Brasil. Nesta base, este estudo teve como objetivo investigar o comportamento da radiação UV solar, através da análise do índice UV coletado no sul do Brasil (29,4◦ S, 53,8◦ O) utilizando dados da radiação UV terrestre (espectrofotômetro Brewer modelo MKIII#167) e de satélite. As medidas na superfície incluem índice UV, dose eritematosa, UV-B não-oesado e integral diária de UV. Os dados de UV usados são do período de 2005-2017, foram comparados com medidas do Instrumento de Monitoramento do Ozônio (OMI) a bordo do satélite Aura. De modo geral, a radiação UV no sul do Brasil, emSantaMaria, é dominada pelo ciclo sazonal anual, com um máximo no verão e um mínimo no inverno. Entretanto, índices UV muito altos e até mesmo extremos foram medidos na primavera e no outono. A análise espectral usando o método wavelet mostrou que a variabilidade UV no sul do Brasil também é modulada por 3 forçantes: a El-Nino Southern Oscillation (ENSO), a Oscilação Quasi-Bienal (QBO) e o ciclo solar. Quanto à influência das anomalias devidas ao efeito secundário do BOA, obtivemos uma redução média de 1%dacoluna de ozônio total, com um aumento médio de 4% do índice UV, nas condições de céu claro.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPESporUniversidade Federal de Santa MariaCentro de Ciências Naturais e ExatasPrograma de Pós-Graduação em MeteorologiaUFSMBrasilMeteorologiaAttribution-NonCommercial-NoDerivatives 4.0 Internationalhttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessRadiação UVÍndice UVBuraco de Ozônio na AntártidaEspectrofotômetro BrewerUV radiationUV indexAntarctic ozone holeBrewer spectrophotometerCNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIAAnalise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do BrasilAnalysis of the UVB radiation during the events of influence of the antarctic ozone hole over south of BrazilAnalyse du rayonnement pendant les événements de influence du troud’ozone antarctique sur le sud du Brésilinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesisPinheiro, Damaris Kirschhttp://lattes.cnpq.br/9528588455662843Bencherif, HassanPortafaix , ThierryPeres, Lucas VazSteffenel , Luiz AngeloDal Piva , EversonAnabor, Vagnerhttp://lattes.cnpq.br/5172603287329140Lopes, Bibiana Culau100700300004600600600600600600600600600a5a6b5cf-0af3-46df-b502-03da35313aedcf9eb58c-7a28-4d3e-89ef-19b069530964dac61789-6904-4cab-b9b1-af0f336a84d388fea1ac-d03a-4497-a05c-e0026f5a3757d48e211a-9239-4aea-8c23-b6b9d67ff239346a2c71-f1d5-4e6f-b709-42a875db276951d24ba6-5281-4437-ab1b-4e76ddbc9cd28348c898-63f3-4df1-9d2a-43b20836d779reponame:Manancial - Repositório Digital da UFSMinstname:Universidade Federal de Santa Maria (UFSM)instacron:UFSMCC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8805http://repositorio.ufsm.br/bitstream/1/25983/2/license_rdf4460e5956bc1d1639be9ae6146a50347MD52ORIGINALTES_PPGMETEOROLOGIA_2022_LOPES_BIBIANA.pdfTES_PPGMETEOROLOGIA_2022_LOPES_BIBIANA.pdfTese de doutoradoapplication/pdf8963130http://repositorio.ufsm.br/bitstream/1/25983/1/TES_PPGMETEOROLOGIA_2022_LOPES_BIBIANA.pdfd17e435da7955cd1f357fc669ff33549MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-816http://repositorio.ufsm.br/bitstream/1/25983/3/license.txt6eeec7985884eb94336b41cc5308bf0fMD531/259832022-08-25 14:52:35.043oai:repositorio.ufsm.br:1/25983Q3JlYXRpdmUgQ29tbXVucw==Repositório Institucionalhttp://repositorio.ufsm.br/PUBhttp://repositorio.ufsm.br/oai/requestopendoar:39132022-08-25T17:52:35Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)false
dc.title.por.fl_str_mv Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
dc.title.alternative.eng.fl_str_mv Analysis of the UVB radiation during the events of influence of the antarctic ozone hole over south of Brazil
dc.title.alternative.fra.fl_str_mv Analyse du rayonnement pendant les événements de influence du troud’ozone antarctique sur le sud du Brésil
title Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
spellingShingle Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
Lopes, Bibiana Culau
Radiação UV
Índice UV
Buraco de Ozônio na Antártida
Espectrofotômetro Brewer
UV radiation
UV index
Antarctic ozone hole
Brewer spectrophotometer
CNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIA
title_short Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
title_full Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
title_fullStr Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
title_full_unstemmed Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
title_sort Analise da radiação UV-B durante os eventos de influência do buraco de ozônio antártico na região sul do Brasil
author Lopes, Bibiana Culau
author_facet Lopes, Bibiana Culau
author_role author
dc.contributor.advisor1.fl_str_mv Pinheiro, Damaris Kirsch
dc.contributor.advisor1Lattes.fl_str_mv http://lattes.cnpq.br/9528588455662843
dc.contributor.advisor-co1.fl_str_mv Bencherif, Hassan
dc.contributor.referee1.fl_str_mv Portafaix , Thierry
dc.contributor.referee2.fl_str_mv Peres, Lucas Vaz
dc.contributor.referee3.fl_str_mv Steffenel , Luiz Angelo
dc.contributor.referee4.fl_str_mv Dal Piva , Everson
dc.contributor.referee5.fl_str_mv Anabor, Vagner
dc.contributor.authorLattes.fl_str_mv http://lattes.cnpq.br/5172603287329140
dc.contributor.author.fl_str_mv Lopes, Bibiana Culau
contributor_str_mv Pinheiro, Damaris Kirsch
Bencherif, Hassan
Portafaix , Thierry
Peres, Lucas Vaz
Steffenel , Luiz Angelo
Dal Piva , Everson
Anabor, Vagner
dc.subject.por.fl_str_mv Radiação UV
Índice UV
Buraco de Ozônio na Antártida
Espectrofotômetro Brewer
topic Radiação UV
Índice UV
Buraco de Ozônio na Antártida
Espectrofotômetro Brewer
UV radiation
UV index
Antarctic ozone hole
Brewer spectrophotometer
CNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIA
dc.subject.eng.fl_str_mv UV radiation
UV index
Antarctic ozone hole
Brewer spectrophotometer
dc.subject.cnpq.fl_str_mv CNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIA
description Exposure to the sun is fundamental for human health and the growth and development of f lora and fauna, although excessive exposure to the sun’s UV rays can be harmful to all living things. It can affect aquatic and terrestrial animals, plants and can cause serious problems on human health, such as burns, eye damage and long-term exposure can lead to skin cancer and accelerate skin aging. Ozone is the main gas in the Earth’s atmosphere that absorbs UV radiation in the stratosphere. The Antarctic Ozone Hole (AOH) is characterized by an extreme reduction in ozone levels in the Antarctic region in the spring. The secondary effects of the AOH are caused by the displacement of ozone-poor air masses from the polar vortex to the mid-latitudes, including southern Brazil. On this basis, this study aimed to investigate the behavior of solar UV radiation, through the analysis of the UV index collected in southern Brazil (29,4◦ S, 53,8◦ O) using ground (Brewer spectrophotometer) and satellite UV radiation data. The ground-based measurements include UV index, erythemal dose, unweighted UV-B, and daily UV integral. The UV data used covers the period 2005-2017 were compared with observations from the Ozone Monitoring Instrument (OMI) experiment onboard the Aura satellite. Overall, UV radiation in southern Brazil, in Santa Maria, is dominated by the annual seasonal cycle, with a maximum in summer and a minimum in winter. However, very high and even extreme UV indices were measured in spring and fall. Spectral analysis by the wavelet method showed that the variability of UVradiation in southern Brazil is also modulated by 3 forcing: El-Nino Southern Oscillation (ENSO), the Quasi-Biennial Oscillation (QBO) and the solar cycle. As for the influence of anomalies due to the secondary effect of the AOH, we obtained an average reduction of 1% of the total ozone column, with an average increase of 4% of the UV index, under clear-sky condition.
publishDate 2022
dc.date.accessioned.fl_str_mv 2022-08-25T17:52:34Z
dc.date.available.fl_str_mv 2022-08-25T17:52:34Z
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dc.publisher.none.fl_str_mv Universidade Federal de Santa Maria
Centro de Ciências Naturais e Exatas
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publisher.none.fl_str_mv Universidade Federal de Santa Maria
Centro de Ciências Naturais e Exatas
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