Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS

Detalhes bibliográficos
Autor(a) principal: Oliveira, Lucas Ilha Gandolfi de
Data de Publicação: 2022
Tipo de documento: Dissertação
Idioma: por
Título da fonte: Manancial - Repositório Digital da UFSM
dARK ID: ark:/26339/0013000006v7d
Texto Completo: http://repositorio.ufsm.br/handle/1/27839
Resumo: Convective storms can significantly alter the evolution of the flow in the Planetary Boundary Layer (PBL). In this study, thermodynamic, kinematic and turbulent quantities were calculated in the PBL during the passage of convective storms by the micrometeorological tower located at the Federal University of Santa Maria (UFSM in Portuguese) in the state of Rio Grande do Sul. Ten events were subjectively selected for the study, in the day, day/night and night periods for the period from 2020 to 2022. Based on radar images, the storms were classified into discrete and multicellular, where 6 storms were discrete and 4 multicellular. For each selected event, time series of temperature (°C), pressure (hPa) and mean horizontal wind (m s-1), and relative humidity (%) were analyzed, identifying the events observing a decrease in T (cold pool), increase of p (mesohigh) and increase of Vh (gust front). The factor that most characterized the patterns of sensible heat fluxes and turbulent kinetic energy (TKE) was the degree of organization of gust fronts and cold pools. The discrete events presented better defined gust fronts and cold pools, with an increase in TKE with the arrival of the gust front and peaks of sensible heat flux maxima around the time they were recorded. After the passage of the gust front and with the establishment of the cold pool, there was cooling and intense turbulent flow (high TKE). This pattern was less defined for multicellular cases and had little dependence on the diurnal cycle. In both discrete and multicellular cases, some events showed pressure drops, some associated with heating and drying and others with cooling. Warm-up cases were associated with wake lows or mesolows. On the other hand, cases with cooling were associated with the passage of mesocyclones close to the tower. Finally, it was shown that the vertical wind shear field is drastically intensified by storms, especially discrete ones and in low layers of 5, 10, or 15 m. Such intensification is relevant, since intense vertical shallow wind shear is associated with the production of vortices in thunderstorms.
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spelling Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RSFrente de rajadaPiscina friaCLPFluxos turbulentosGust frontCold poolPBLTurbulent fluxesCNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIAConvective storms can significantly alter the evolution of the flow in the Planetary Boundary Layer (PBL). In this study, thermodynamic, kinematic and turbulent quantities were calculated in the PBL during the passage of convective storms by the micrometeorological tower located at the Federal University of Santa Maria (UFSM in Portuguese) in the state of Rio Grande do Sul. Ten events were subjectively selected for the study, in the day, day/night and night periods for the period from 2020 to 2022. Based on radar images, the storms were classified into discrete and multicellular, where 6 storms were discrete and 4 multicellular. For each selected event, time series of temperature (°C), pressure (hPa) and mean horizontal wind (m s-1), and relative humidity (%) were analyzed, identifying the events observing a decrease in T (cold pool), increase of p (mesohigh) and increase of Vh (gust front). The factor that most characterized the patterns of sensible heat fluxes and turbulent kinetic energy (TKE) was the degree of organization of gust fronts and cold pools. The discrete events presented better defined gust fronts and cold pools, with an increase in TKE with the arrival of the gust front and peaks of sensible heat flux maxima around the time they were recorded. After the passage of the gust front and with the establishment of the cold pool, there was cooling and intense turbulent flow (high TKE). This pattern was less defined for multicellular cases and had little dependence on the diurnal cycle. In both discrete and multicellular cases, some events showed pressure drops, some associated with heating and drying and others with cooling. Warm-up cases were associated with wake lows or mesolows. On the other hand, cases with cooling were associated with the passage of mesocyclones close to the tower. Finally, it was shown that the vertical wind shear field is drastically intensified by storms, especially discrete ones and in low layers of 5, 10, or 15 m. Such intensification is relevant, since intense vertical shallow wind shear is associated with the production of vortices in thunderstorms.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPESTempestades convectivas podem alterar significativamente a evolução do escoamento na Camada Limite Planetária (CLP). Neste estudo, foram calculadas quantidades termodinâmicas, cinemáticas e turbulentas na CLP durante a passagem de tempestades convectivas pela torre micrometeorológica situada na Universidade Federal de Santa Maria (UFSM) no estado do Rio Grande do Sul. Foram selecionados de forma subjetiva dez eventos para o estudo, nos períodos diurno, diurno/noturno e noturno para o período de 2020 a 2022. Com base em imagens de radar, as tempestades foram classificadas entre discretas e multicelulares, onde 6 tempestades foram discretas e 4 multicelulares. Para cada evento selecionado, foram analisadas séries temporais de temperatura (°C), pressão (hPa) e vento horizontal médio (m s-1), e umidade relativa (%) identificando os eventos observando diminuição de T (piscina fria), aumento de p (mesoalta) e aumento de Vh (frente de rajada). O fator que mais caracterizou os padrões de fluxos de calor sensível e energia cinética turbulenta (ECT) foi o grau de organização das frentes de rajadas e piscinas frias. Os eventos discretos apresentaram frentes de rajada e piscinas frias mais bem definidas, com aumento de ECT com a chegada da frente de rajada e picos de máximos de fluxo de calor sensível em torno da hora em que os mesmos foram registrados. Após a passagem da frente de rajada e com o estabelecimento da piscina fria, houve resfriamento e intenso escoamento turbulento (alta ECT). Este padrão foi menos definido para casos multicelulares e teve pouca dependência no ciclo diurno. Em ambos casos discretos e multicelulares, alguns eventos apresentaram quedas de pressão, sendo alguns destes associados a aquecimento e secamento e outros com resfriamento. Os casos de aquecimento foram associados a baixas de esteira ou mesobaixas. Em contrapartida, os casos com resfriamento foram associados a passagem de mesociclones próximo à torre. Por fim, mostrou-se que o campo de cisalhamento vertical do vento é drasticamente intensificado pelas tempestades, especialmente as discretas e em camadas baixas de 5, 10, ou 15 m. Tal intensificação é relevante, uma vez que intenso cisalhamento vertical do vento raso está associado à produção de vórtices em tempestades.Universidade Federal de Santa MariaBrasilMeteorologiaUFSMPrograma de Pós-Graduação em MeteorologiaCentro de Ciências Naturais e ExatasAcevedo, Otavio Costahttp://lattes.cnpq.br/8696858608013659Oliveira, Pablo Eli Soares deNascimento, Ernani de LimaFigueiredo, Eliton Lima deOliveira, Lucas Ilha Gandolfi de2023-02-17T13:11:31Z2023-02-17T13:11:31Z2022-12-28info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/masterThesisapplication/pdfhttp://repositorio.ufsm.br/handle/1/27839ark:/26339/0013000006v7dporAttribution-NonCommercial-NoDerivatives 4.0 Internationalhttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessreponame:Manancial - Repositório Digital da UFSMinstname:Universidade Federal de Santa Maria (UFSM)instacron:UFSM2023-03-30T12:43:43Zoai:repositorio.ufsm.br:1/27839Biblioteca Digital de Teses e Dissertaçõeshttps://repositorio.ufsm.br/ONGhttps://repositorio.ufsm.br/oai/requestatendimento.sib@ufsm.br||tedebc@gmail.comopendoar:2023-03-30T12:43:43Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)false
dc.title.none.fl_str_mv Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
title Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
spellingShingle Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
Oliveira, Lucas Ilha Gandolfi de
Frente de rajada
Piscina fria
CLP
Fluxos turbulentos
Gust front
Cold pool
PBL
Turbulent fluxes
CNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIA
title_short Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
title_full Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
title_fullStr Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
title_full_unstemmed Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
title_sort Caracterização do comportamento da camada limite planetaria durante a passagem de tempestades severas na região de Santa Maria, RS
author Oliveira, Lucas Ilha Gandolfi de
author_facet Oliveira, Lucas Ilha Gandolfi de
author_role author
dc.contributor.none.fl_str_mv Acevedo, Otavio Costa
http://lattes.cnpq.br/8696858608013659
Oliveira, Pablo Eli Soares de
Nascimento, Ernani de Lima
Figueiredo, Eliton Lima de
dc.contributor.author.fl_str_mv Oliveira, Lucas Ilha Gandolfi de
dc.subject.por.fl_str_mv Frente de rajada
Piscina fria
CLP
Fluxos turbulentos
Gust front
Cold pool
PBL
Turbulent fluxes
CNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIA
topic Frente de rajada
Piscina fria
CLP
Fluxos turbulentos
Gust front
Cold pool
PBL
Turbulent fluxes
CNPQ::CIENCIAS EXATAS E DA TERRA::GEOCIENCIAS::METEOROLOGIA
description Convective storms can significantly alter the evolution of the flow in the Planetary Boundary Layer (PBL). In this study, thermodynamic, kinematic and turbulent quantities were calculated in the PBL during the passage of convective storms by the micrometeorological tower located at the Federal University of Santa Maria (UFSM in Portuguese) in the state of Rio Grande do Sul. Ten events were subjectively selected for the study, in the day, day/night and night periods for the period from 2020 to 2022. Based on radar images, the storms were classified into discrete and multicellular, where 6 storms were discrete and 4 multicellular. For each selected event, time series of temperature (°C), pressure (hPa) and mean horizontal wind (m s-1), and relative humidity (%) were analyzed, identifying the events observing a decrease in T (cold pool), increase of p (mesohigh) and increase of Vh (gust front). The factor that most characterized the patterns of sensible heat fluxes and turbulent kinetic energy (TKE) was the degree of organization of gust fronts and cold pools. The discrete events presented better defined gust fronts and cold pools, with an increase in TKE with the arrival of the gust front and peaks of sensible heat flux maxima around the time they were recorded. After the passage of the gust front and with the establishment of the cold pool, there was cooling and intense turbulent flow (high TKE). This pattern was less defined for multicellular cases and had little dependence on the diurnal cycle. In both discrete and multicellular cases, some events showed pressure drops, some associated with heating and drying and others with cooling. Warm-up cases were associated with wake lows or mesolows. On the other hand, cases with cooling were associated with the passage of mesocyclones close to the tower. Finally, it was shown that the vertical wind shear field is drastically intensified by storms, especially discrete ones and in low layers of 5, 10, or 15 m. Such intensification is relevant, since intense vertical shallow wind shear is associated with the production of vortices in thunderstorms.
publishDate 2022
dc.date.none.fl_str_mv 2022-12-28
2023-02-17T13:11:31Z
2023-02-17T13:11:31Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/masterThesis
format masterThesis
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://repositorio.ufsm.br/handle/1/27839
dc.identifier.dark.fl_str_mv ark:/26339/0013000006v7d
url http://repositorio.ufsm.br/handle/1/27839
identifier_str_mv ark:/26339/0013000006v7d
dc.language.iso.fl_str_mv por
language por
dc.rights.driver.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Universidade Federal de Santa Maria
Brasil
Meteorologia
UFSM
Programa de Pós-Graduação em Meteorologia
Centro de Ciências Naturais e Exatas
publisher.none.fl_str_mv Universidade Federal de Santa Maria
Brasil
Meteorologia
UFSM
Programa de Pós-Graduação em Meteorologia
Centro de Ciências Naturais e Exatas
dc.source.none.fl_str_mv reponame:Manancial - Repositório Digital da UFSM
instname:Universidade Federal de Santa Maria (UFSM)
instacron:UFSM
instname_str Universidade Federal de Santa Maria (UFSM)
instacron_str UFSM
institution UFSM
reponame_str Manancial - Repositório Digital da UFSM
collection Manancial - Repositório Digital da UFSM
repository.name.fl_str_mv Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)
repository.mail.fl_str_mv atendimento.sib@ufsm.br||tedebc@gmail.com
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