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@PhDThesis{Henkes:2022:ObMo,
               author = "Henkes, Alice Franci{\'e}li",
                title = "Evolu{\c{c}}{\~a}o de nuvens rasas {\`a} convec{\c{c}}{\~a}o 
                         profunda na esta{\c{c}}{\~a}o seca na Amaz{\^o}nia Central: 
                         observa{\c{c}}{\~a}o e modelagem",
               school = "Instituto Nacional de Pesquisas Espaciais (INPE)",
                 year = "2022",
              address = "S{\~a}o Jos{\'e} dos Campos",
                month = "2021-12-14",
             keywords = "camada limite atmosf{\'e}rica, esta{\c{c}}{\~a}o seca, 
                         transi{\c{c}}{\~a}o matutina, fluxo de calor, energia 
                         cin{\'e}tica turbulenta, atmospheric boundary layer, dry season, 
                         morning transition, heat flux, turbulent kinetic energy.",
             abstract = "Esta pesquisa teve o objetivo de investigar a evolu{\c{c}}{\~a}o 
                         da Camada Limite Atmosf{\'e}rica (CLA) da Amaz{\^o}nia nos 
                         regimes convectivos com transi{\c{c}}{\~a}o de nuvens cumulus 
                         rasas para profundas (ShDeep) e sem transi{\c{c}}{\~a}o, ou 
                         seja, com apenas forma{\c{c}}{\~a}o de nuvens convectivas 
                         cumulus rasas (ShCu) durante a esta{\c{c}}{\~a}o seca do projeto 
                         Green Ocean Amazon (GoAmazon) 2014-2015. Na an{\'a}lise 
                         observacional deste trabalho, os est{\'a}gios da CLA nas 
                         condi{\c{c}}{\~o}es ShDeep, desde o per{\'{\i}}odo noturno 
                         at{\'e} a fase da camada de mistura com nuvens, s{\~a}o 
                         apresentados em compara{\c{c}}{\~a}o com o regime ShCu. As 
                         condi{\c{c}}{\~o}es din{\^a}micas e termodin{\^a}micas da 
                         atmosfera, perfis verticais e vari{\'a}veis pr{\'o}ximo {\`a} 
                         superf{\'{\i}}cie foram utilizados para comparar os dois regimes 
                         de nuvens para cada est{\'a}gio da evolu{\c{c}}{\~a}o da CLA. 
                         As observa{\c{c}}{\~o}es mostram que a dura{\c{c}}{\~a}o do 
                         est{\'a}gio de transi{\c{c}}{\~a}o matutina {\'e} menor nos 
                         dias ShDeep, associado com o maior conte{\'u}do integrado da 
                         umidade e intenso cisalhamento do vento nas primeiras horas da 
                         manh{\~a}. Dessa forma, o in{\'{\i}}cio da CLA convectiva 
                         (camada bem misturada) ocorre mais cedo do que nos dias ShCu. 
                         Durante o est{\'a}gio de crescimento r{\'a}pido, os movimentos 
                         verticais mais intensos na camada sub-nuvem favorecem o 
                         aprofundamento CLA atrav{\'e}s do qual uma parcela de ar pode 
                         alcan{\c{c}}ar o n{\'{\i}}vel de condensa{\c{c}}{\~a}o por 
                         levantamento, favorecendo o desenvolvimento de nuvens convectivas. 
                         Na segunda parte deste trabalho, dois casos de estudo foram 
                         analisados com simula{\c{c}}{\~o}es num{\'e}ricas em alta 
                         resolu{\c{c}}{\~a}o com o modelo Mesoescale Non-Hydrostatic 
                         model Meso-NH. Os resultados das simula{\c{c}}{\~o}es mostraram 
                         que o local e o momento do in{\'{\i}}cio das nuvens convectivas 
                         foram criticamente influenciados pela distribui{\c{c}}{\~a}o 
                         vertical da umidade na CLA. Al{\'e}m disso, o efeito brisa de rio 
                         mostrou ser crucial para o desenvolvimento de nuvens rasas para a 
                         regi{\~a}o analisada. Com rela{\c{c}}{\~a}o a 
                         transi{\c{c}}{\~a}o matutina, as simula{\c{c}}{\~o}es com o 
                         Meso-NH foram consistentes com as observa{\c{c}}{\~o}es, 
                         mostrando um in{\'{\i}}cio da CLA convectiva mais cedo no caso 
                         ShDeep. A simula{\c{c}}{\~a}o indica que a transi{\c{c}}{\~a}o 
                         mais r{\'a}pida para o in{\'{\i}}cio da CLA convectiva pode ser 
                         atribu{\'{\i}}da a produ{\c{c}}{\~a}o mec{\^a}nica e 
                         produ{\c{c}}{\~a}o t{\'e}rmica de energia cin{\'e}tica 
                         turbulenta (TKE), associada ao maior fluxo de calor 
                         sens{\'{\i}}vel na superf{\'{\i}}cie no processo de 
                         eros{\~a}o da invers{\~a}o noturna. O in{\'{\i}}cio mais cedo 
                         da CLA convectiva, devido {\`a}s condi{\c{c}}{\~o}es ambientais 
                         mais prop{\'{\i}}cias, mostrou ter um importante efeito no 
                         movimento vertical, TKE e instabilidade no est{\'a}gio de 
                         crescimento r{\'a}pido da CLA convectiva. Nessa 
                         condi{\c{c}}{\~o}es, a fase de crescimento da CLA e a 
                         forma{\c{c}}{\~a}o de nuvens rasas s{\~a}o fortemente modulados 
                         pela instabilidade e pela energia total dispon{\'{\i}}vel na 
                         CLA, enquanto que a umidade na atmosfera livre {\'e} determinante 
                         na transi{\c{c}}{\~a}o de nuvem convectiva rasa para profunda. 
                         ABSTRACT: This work aimed to investigate the Amazonian Atmospheric 
                         Boundary Layer (BL) on shallow convective days (ShCu) and 
                         shallow-to-deep convective days (ShDeep) during the dry season 
                         using a suite of ground-based measurements from the Observation 
                         and Modeling of the Green Ocean Amazon (GoAmazon 2014/5) 
                         Experiment and modeling results. In the observational analysis, 
                         the BL stages in ShDeep days, from the nighttime to the cloudy 
                         mixing layer stage, are then described in comparison with ShCu 
                         days. Atmospheric thermodynamics and dynamics, environmental 
                         profiles, and near-surface variables were employed to compare 
                         these two distinct situations for each stage of the BL evolution. 
                         Results show that the decrease in time duration of the morning 
                         transition on ShDeep days is associated with high humidity and 
                         well-established vertical wind shear patterns in the early morning 
                         hours. Therefore, the onset of full convection (e.g, well-mixed 
                         layer) is earlier on the ShDeep conditions. During the rapid 
                         growth stage, vertical mixing in the deeper BL will entrain moist 
                         air into the BL through which the air parcel can reach the LCL 
                         (thus causing the first cell of shallow cumulus to emerge) and 
                         thus favoring deep convection. In the second part of this work, 
                         two case studies were analyzed with A 200-m grid spacing LES run 
                         with the Mesoescale Non-Hydrostatic model Meso-NH. The results of 
                         the simulations showed that the location and timing of convective 
                         cloud onset were critically influenced by the vertical 
                         distribution of moisture in the BL. In addition, the river breeze 
                         effect has been shown to be crucial for the development of shallow 
                         clouds for the analyzed region. In terms of the morning BL 
                         condition, the Meso-NH is consistent with the observations, 
                         showing an earlier onset of convective CLA on ShDeep case. The 
                         simulation results indicates that the sorter morning transition to 
                         the onset of convective CLA can be attributed to mechanical 
                         production and thermal production of turbulent kinetic energy 
                         (TKE), associated with the higher surface sensible heat flux in 
                         the erosion process of the nocturnal inversion. Earlier onset of 
                         convective BL, due to more favorable environmental conditions, has 
                         been shown to have an important effect on vertical motion, TKE, 
                         and instability in the rapid growth stage of convective BL. Under 
                         these conditions, the BL growth phase and shallow cloud formation 
                         are strongly modulated by instability and the total available BL 
                         energy, while higher humidity above the BL favors the evolution 
                         from shallow to deep cumulus clouds.",
            committee = "Randow, Celso von (presidente) and Fisch, Gilberto Fernando 
                         (orientador) and Machado, Luiz Augusto Toledo (orientador) and 
                         Campos Velho, Haroldo Fraga de and Acevedo, Ot{\'a}vio Costa and 
                         Dias J{\'u}nior, Cl{\'e}o Quaresma",
         englishtitle = "From shallow to deep convective cloud evolution during the dry 
                         season in the Central Amazon",
             language = "pt",
                pages = "117",
                  ibi = "8JMKD3MGP3W34T/45QKLUS",
                  url = "http://urlib.net/ibi/8JMKD3MGP3W34T/45QKLUS",
           targetfile = "publicacao.pdf",
        urlaccessdate = "04 jun. 2024"
}


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