Caminhos para a complexidade na camada limite atmosférica noturna

Detalhes bibliográficos
Autor(a) principal: Costa, Felipe Denardin
Data de Publicação: 2011
Tipo de documento: Tese
Idioma: por
Título da fonte: Manancial - Repositório Digital da UFSM
dARK ID: ark:/26339/00130000080x8
Texto Completo: http://repositorio.ufsm.br/handle/1/3896
Resumo: The focus of the present thesis is the nocturnal atmospheric boundary layer, under very stable conditions. In such situation, the turbulence production by the vertical wind shear may have similar magnitude to the total turbulence destruction by the thermal stratification and molecular dissipation terms. Besides being in near balance, the turbulence production and destruction are, each of them, functions of the turbulence intensity itself. This condition causes situations on which the system behaves on a manner different than that expected from each of its parts individually. Such processes are characterized, in the present study, as paths to complexity, and are analyzed separately in the different chapters that compose the thesis. In chapter 2, the coupling state between the surface and the top of the stable boundary layer (SBL) is investigated using four different schemes to represent the turbulent exchange. An idealized SBL is assumed, with fixed wind speed and temperature at its top. The formulations compared are those that solve a prognostic equation for turbulent kinetic energy (TKE) and those that directly prescribe turbulence intensity as a function of atmospheric stability. The formulation influence on the coupling state is analyzed and it is concluded that, in general, the simple TKE formulation has a better response, although it also tends to overestimate turbulent mixing. The consequences are discussed. In chapter 3, a simplified new model for the exchange between the surface and the atmosphere under stable conditions is proposed. Its main difference from previous works consists in the fact that the turbulent intensity is determined by a prognostic equation for turbulent kinetic energy (TKE), rather than by using stability functions that arbitrarily relate it to atmospheric stability. Its main novelty is the fact that, when multiple atmospheric levels are considered, it leads to complex solutions, characterizing the occurrence of the phenomenon known as global intermittency. The vertical structure of the intermittent events is analyzed, and it shown that they are generated at the surface by a local shear increase above a threshold, propagating upward through the turbulence transfer term in the TKE equation. It is proposed that such events constitute a natural characteristic of the disconnected SBL, which occurs along with low large-scale winds and clear skies. Chapter 4 is devoted to the purpose of showing that the use of stability functions that represent the turbulence intensity as its average dependence on atmospheric stability reduces the number of degrees of freedom of the system, precluding it from reaching complex solutions. Finally, in chapter 5, a detailed system dynamics analysis is applied to the model proposed in chapter 3, with the aim of identifying whether it is or not chaotic. It is shown that the system bifurcates as the wind speed at the SBL top increases, reaching period 3 for a range of situations, a sufficient condition for chaos existence. Furthermore, positive Lyapunov exponents are found, again confirming the chaotic character of the system. It is shown that the complexity arises from the nonlinear interactions between the different vertical levels considered, through the vertical turbulence transport terms.
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spelling Caminhos para a complexidade na camada limite atmosférica noturnaRoutes to complexity on the nocturnal atmospheric boundary layerCamada limite estávelTurbulênciaEstado de acoplamentoIntermitênciaComplexidadeCaosStable boundary layerTurbulenceCoupling stateIntermittencyComplexityChaosCNPQ::CIENCIAS EXATAS E DA TERRA::FISICAThe focus of the present thesis is the nocturnal atmospheric boundary layer, under very stable conditions. In such situation, the turbulence production by the vertical wind shear may have similar magnitude to the total turbulence destruction by the thermal stratification and molecular dissipation terms. Besides being in near balance, the turbulence production and destruction are, each of them, functions of the turbulence intensity itself. This condition causes situations on which the system behaves on a manner different than that expected from each of its parts individually. Such processes are characterized, in the present study, as paths to complexity, and are analyzed separately in the different chapters that compose the thesis. In chapter 2, the coupling state between the surface and the top of the stable boundary layer (SBL) is investigated using four different schemes to represent the turbulent exchange. An idealized SBL is assumed, with fixed wind speed and temperature at its top. The formulations compared are those that solve a prognostic equation for turbulent kinetic energy (TKE) and those that directly prescribe turbulence intensity as a function of atmospheric stability. The formulation influence on the coupling state is analyzed and it is concluded that, in general, the simple TKE formulation has a better response, although it also tends to overestimate turbulent mixing. The consequences are discussed. In chapter 3, a simplified new model for the exchange between the surface and the atmosphere under stable conditions is proposed. Its main difference from previous works consists in the fact that the turbulent intensity is determined by a prognostic equation for turbulent kinetic energy (TKE), rather than by using stability functions that arbitrarily relate it to atmospheric stability. Its main novelty is the fact that, when multiple atmospheric levels are considered, it leads to complex solutions, characterizing the occurrence of the phenomenon known as global intermittency. The vertical structure of the intermittent events is analyzed, and it shown that they are generated at the surface by a local shear increase above a threshold, propagating upward through the turbulence transfer term in the TKE equation. It is proposed that such events constitute a natural characteristic of the disconnected SBL, which occurs along with low large-scale winds and clear skies. Chapter 4 is devoted to the purpose of showing that the use of stability functions that represent the turbulence intensity as its average dependence on atmospheric stability reduces the number of degrees of freedom of the system, precluding it from reaching complex solutions. Finally, in chapter 5, a detailed system dynamics analysis is applied to the model proposed in chapter 3, with the aim of identifying whether it is or not chaotic. It is shown that the system bifurcates as the wind speed at the SBL top increases, reaching period 3 for a range of situations, a sufficient condition for chaos existence. Furthermore, positive Lyapunov exponents are found, again confirming the chaotic character of the system. It is shown that the complexity arises from the nonlinear interactions between the different vertical levels considered, through the vertical turbulence transport terms.Coordenação de Aperfeiçoamento de Pessoal de Nível SuperiorO foco da presente tese é a camada limite atmosférica noturna, sob condições estáveis. Nesta situação, a produção de turbulência pelo cisalhamento vertical do vento pode ter magnitude similar à destruição total de turbulência devido à estratificação térmica e a dissipação molecular. Além de serem próximos no balanço, a produção de turbulência e a destruição são, cada um deles, funções da intensidade turbulenta. Esta condição causa situações nas quais o sistema se comporta de maneira diferente do que o esperado para cada uma de suas partes individualmente. Tais processos são caracterizados, no presente estudo, como caminhos para a complexidade, e são analisados separadamente em diferentes capítulos que compôem a tese. No capítulo 2, o estado de acoplamento entre a superfície e o topo da camada limite estável (CLE) é investigado usando 4 diferentes esquemas para representar a intensidade turbulenta. Uma CLE idealizada é assumida, com velocidade do vento e temperatura fixas no seu topo. As formulações comparadas são aquelas que resolvem uma equação prognóstica para a energia cinética turbulenta (ECT) e as que prescrevem diretamente a intensidade turbulenta como uma função da estabilidade atmosférica. A influência da formulação no estado de acoplamento é analisada e é concluído que, em geral, a formulação simples de ECT tem a melhor resposta, embora esta tenda a superestimar a mistura turbulenta. As consequências são discutidas. No capítulo 3, um novo modelo simplificado para interação entre a superfície e a atmosfera em condições estáveis é proposto. A principal diferença com relação a estudos anteriores, consiste no fato que a intensidade turbulenta é determinada por uma equação prognóstica para a ECT, ao invés de usar funções de estabilidade que são arbitráriamente relacionadas com a estabilidade atmosférica. A principal novidade é o fato que, quando multipos níveis atmosféricos são considerados, este apresenta soluções complexas, caracterizando a ocorrência do fenômeno conhecido como intermitência global. A estrutura vertical dos eventos intermitentes é analisada, e esta mostra que os eventos são gerados na superfície pelo aumento local do cisalhamento acima de uma fronteira, propagando-se para cima através do termo de transporte turbulento na equação da ECT. É proposto que tais eventos constituam uma característica natural da CLE desconectada, a qual ocorre em condições de ventos de grande escala fracos e com céu claro. O capítulo 4 tem como propósito mostrar que o uso de funções de estabilidade que representam a intensidade da turbulência como a dependência média desta com a estabilidade atmosférica, reduz os graus de liberdade do sistema, assim evitando que este encontre soluções complexas. Finalmente, no capítulo 5, uma análise dinâmica detalhada é aplicada no modelo proposto no capítulo 3, com meta de identificar se este é caótico ou não. É mostrado que as soluções do sistema bifurcam-se com o aumento da velocidade do vento no topo da CLE, encontrando soluções com período 3 para um intervalo de situações, uma condição suficiente para a existência de caos. Além disso, expoentes de Lyapunov positivos são encontrados, novamente confirmando o caráter caótico do sistema. É mostrado que a complexidade surge através de interações não lineares entre os diferentes níveis verticais considerados, através do termo de transporte vertical de turbulência.Universidade Federal de Santa MariaBRFísicaUFSMPrograma de Pós-Graduação em FísicaAcevedo, Otavio Costahttp://lattes.cnpq.br/8696858608013659Dias, Pedro Leite da Silvahttp://lattes.cnpq.br/9273702863744424Rivero, Silvio Nilo Figueroahttp://lattes.cnpq.br/2191790439726897Moraes, Osvaldo Luiz Leal dehttp://lattes.cnpq.br/0593135962205202Degrazia, Gervásio Anneshttp://lattes.cnpq.br/3195210233978887Costa, Felipe Denardin2017-05-082017-05-082011-12-09info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/doctoralThesisapplication/pdfapplication/pdfCOSTA, Felipe Denardin. Routes to complexity on the nocturnal atmospheric boundary layer. 2011. 134 f. Tese (Doutorado em Física) - Universidade Federal de Santa Maria, Santa Maria, 2011.http://repositorio.ufsm.br/handle/1/3896ark:/26339/00130000080x8porinfo:eu-repo/semantics/openAccessreponame:Manancial - Repositório Digital da UFSMinstname:Universidade Federal de Santa Maria (UFSM)instacron:UFSM2021-09-15T12:06:25Zoai:repositorio.ufsm.br:1/3896Biblioteca Digital de Teses e Dissertaçõeshttps://repositorio.ufsm.br/ONGhttps://repositorio.ufsm.br/oai/requestatendimento.sib@ufsm.br||tedebc@gmail.comopendoar:2021-09-15T12:06:25Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)false
dc.title.none.fl_str_mv Caminhos para a complexidade na camada limite atmosférica noturna
Routes to complexity on the nocturnal atmospheric boundary layer
title Caminhos para a complexidade na camada limite atmosférica noturna
spellingShingle Caminhos para a complexidade na camada limite atmosférica noturna
Costa, Felipe Denardin
Camada limite estável
Turbulência
Estado de acoplamento
Intermitência
Complexidade
Caos
Stable boundary layer
Turbulence
Coupling state
Intermittency
Complexity
Chaos
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA
title_short Caminhos para a complexidade na camada limite atmosférica noturna
title_full Caminhos para a complexidade na camada limite atmosférica noturna
title_fullStr Caminhos para a complexidade na camada limite atmosférica noturna
title_full_unstemmed Caminhos para a complexidade na camada limite atmosférica noturna
title_sort Caminhos para a complexidade na camada limite atmosférica noturna
author Costa, Felipe Denardin
author_facet Costa, Felipe Denardin
author_role author
dc.contributor.none.fl_str_mv Acevedo, Otavio Costa
http://lattes.cnpq.br/8696858608013659
Dias, Pedro Leite da Silva
http://lattes.cnpq.br/9273702863744424
Rivero, Silvio Nilo Figueroa
http://lattes.cnpq.br/2191790439726897
Moraes, Osvaldo Luiz Leal de
http://lattes.cnpq.br/0593135962205202
Degrazia, Gervásio Annes
http://lattes.cnpq.br/3195210233978887
dc.contributor.author.fl_str_mv Costa, Felipe Denardin
dc.subject.por.fl_str_mv Camada limite estável
Turbulência
Estado de acoplamento
Intermitência
Complexidade
Caos
Stable boundary layer
Turbulence
Coupling state
Intermittency
Complexity
Chaos
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA
topic Camada limite estável
Turbulência
Estado de acoplamento
Intermitência
Complexidade
Caos
Stable boundary layer
Turbulence
Coupling state
Intermittency
Complexity
Chaos
CNPQ::CIENCIAS EXATAS E DA TERRA::FISICA
description The focus of the present thesis is the nocturnal atmospheric boundary layer, under very stable conditions. In such situation, the turbulence production by the vertical wind shear may have similar magnitude to the total turbulence destruction by the thermal stratification and molecular dissipation terms. Besides being in near balance, the turbulence production and destruction are, each of them, functions of the turbulence intensity itself. This condition causes situations on which the system behaves on a manner different than that expected from each of its parts individually. Such processes are characterized, in the present study, as paths to complexity, and are analyzed separately in the different chapters that compose the thesis. In chapter 2, the coupling state between the surface and the top of the stable boundary layer (SBL) is investigated using four different schemes to represent the turbulent exchange. An idealized SBL is assumed, with fixed wind speed and temperature at its top. The formulations compared are those that solve a prognostic equation for turbulent kinetic energy (TKE) and those that directly prescribe turbulence intensity as a function of atmospheric stability. The formulation influence on the coupling state is analyzed and it is concluded that, in general, the simple TKE formulation has a better response, although it also tends to overestimate turbulent mixing. The consequences are discussed. In chapter 3, a simplified new model for the exchange between the surface and the atmosphere under stable conditions is proposed. Its main difference from previous works consists in the fact that the turbulent intensity is determined by a prognostic equation for turbulent kinetic energy (TKE), rather than by using stability functions that arbitrarily relate it to atmospheric stability. Its main novelty is the fact that, when multiple atmospheric levels are considered, it leads to complex solutions, characterizing the occurrence of the phenomenon known as global intermittency. The vertical structure of the intermittent events is analyzed, and it shown that they are generated at the surface by a local shear increase above a threshold, propagating upward through the turbulence transfer term in the TKE equation. It is proposed that such events constitute a natural characteristic of the disconnected SBL, which occurs along with low large-scale winds and clear skies. Chapter 4 is devoted to the purpose of showing that the use of stability functions that represent the turbulence intensity as its average dependence on atmospheric stability reduces the number of degrees of freedom of the system, precluding it from reaching complex solutions. Finally, in chapter 5, a detailed system dynamics analysis is applied to the model proposed in chapter 3, with the aim of identifying whether it is or not chaotic. It is shown that the system bifurcates as the wind speed at the SBL top increases, reaching period 3 for a range of situations, a sufficient condition for chaos existence. Furthermore, positive Lyapunov exponents are found, again confirming the chaotic character of the system. It is shown that the complexity arises from the nonlinear interactions between the different vertical levels considered, through the vertical turbulence transport terms.
publishDate 2011
dc.date.none.fl_str_mv 2011-12-09
2017-05-08
2017-05-08
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/doctoralThesis
format doctoralThesis
status_str publishedVersion
dc.identifier.uri.fl_str_mv COSTA, Felipe Denardin. Routes to complexity on the nocturnal atmospheric boundary layer. 2011. 134 f. Tese (Doutorado em Física) - Universidade Federal de Santa Maria, Santa Maria, 2011.
http://repositorio.ufsm.br/handle/1/3896
dc.identifier.dark.fl_str_mv ark:/26339/00130000080x8
identifier_str_mv COSTA, Felipe Denardin. Routes to complexity on the nocturnal atmospheric boundary layer. 2011. 134 f. Tese (Doutorado em Física) - Universidade Federal de Santa Maria, Santa Maria, 2011.
ark:/26339/00130000080x8
url http://repositorio.ufsm.br/handle/1/3896
dc.language.iso.fl_str_mv por
language por
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Universidade Federal de Santa Maria
BR
Física
UFSM
Programa de Pós-Graduação em Física
publisher.none.fl_str_mv Universidade Federal de Santa Maria
BR
Física
UFSM
Programa de Pós-Graduação em Física
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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