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@PhDThesis{Melo:2007:SiClHo,
               author = "Melo, Maria Luciene Dias de",
                title = "Simula{\c{c}}{\~o}es de clima para o holoceno m{\'e}dio usando 
                         o MCGA do CPTEC, com {\^e}nfase sobre a Am{\'e}rica do Sul",
               school = "Instituto Nacional de Pesquisas Espaciais (INPE)",
                 year = "2007",
              address = "S{\~a}o Jos{\'e} dos Campos",
                month = "2007-12-10",
             keywords = "mudan{\c{c}}as clim{\'a}ticas, paleoclima, holoceno m{\'e}dio, 
                         MCGA do CPTEC, par{\^a}metros orbitais, climate change, 
                         paleoclimatology, mid-holocene, CPTEC AGCM, orbital parameter.",
             abstract = "Este trabalho tem o objetivo de analisar o clima do Holoceno 
                         M{\'e}dio (HM) para a Am{\'e}rica do Sul (AS), a partir da 
                         sinergia entre a for{\c{c}}ante dos par{\^a}metros orbitais e 
                         concentra{\c{c}}{\~a}o de CO2, utilizando o modelo de 
                         circula{\c{c}}{\~a}o geral atmosf{\'e}rica (MCGA) do Centro de 
                         Previs{\~a}o de Tempo e Estudos Clim{\'a}ticos (CPTEC) com 
                         resolu{\c{c}}{\~a}o T062 e 28 n{\'{\i}}veis na vertical 
                         (T062L28). Realizaram-se simula{\c{c}}{\~o}es clim{\'a}ticas a 
                         partir da modifica{\c{c}}{\~a}o dos par{\^a}metros orbitais e 
                         concentra{\c{c}}{\~a}o de CO2, para valores t{\'{\i}}picos do 
                         HM, utilizando dois conjuntos de temperatura da 
                         superf{\'{\i}}cie do mar (TSM) [climatol{\'o}gica do AMIP 
                         (HMS1) e gerada pela componente oce{\^a}nica do MCG 
                         oceano-atmosfera acoplado do Institut Pierre Simon Laplace-IPSL 
                         (HMS2)]. Os resultados foram comparados com as 
                         simula{\c{c}}{\~o}es de outros modelos e ind{\'{\i}}cios 
                         paleoclim{\'a}ticos, para compreender como o MCGA do CPTEC 
                         responde {\`a}s mudan{\c{c}}as clim{\'a}ticas e avaliar as 
                         diferen{\c{c}}as do clima da AS no presente e no HM. Os 
                         resultados sugerem clima mais {\'u}mido sobre o nordeste da AS, 
                         devido ao aumento do fluxo de umidade proveniente do oceano 
                         Atl{\^a}ntico trazido pela alta subtropical do Atl{\^a}ntico 
                         Sul, que no HM encontrava-se mais pr{\'o}xima do continente e 
                         ligeiramente mais intensa. Desintensifica{\c{c}}{\~a}o dos 
                         ventos al{\'{\i}}sios no HM acarretou num deslocamento mais ao 
                         norte da Zona de Converg{\^e}ncia Intertropical (ZCIT) e reduziu 
                         o fluxo de umidade do Atl{\^a}ntico tropical para a regi{\~a}o 
                         Amaz{\^o}nica, deixando-a mais seca no HM. Essa 
                         redu{\c{c}}{\~a}o da precipita{\c{c}}{\~a}o tem um impacto 
                         significativo no transporte da umidade da bacia Amaz{\^o}nica 
                         {\`a} Bacia do Prata, e consequentemente sobre a 
                         forma{\c{c}}{\~a}o da Zona de Converg{\^e}ncia do 
                         Atl{\^a}ntico Sul (ZCAS), levando a uma redu{\c{c}}{\~a}o da 
                         precipita{\c{c}}{\~a}o na posi{\c{c}}{\~a}o atual da ZCAS, e 
                         esta foi simulada ligeiramente mais fraca durante o HMS1 e sua 
                         exist{\^e}ncia n{\~a}o foi evidenciada no experimento com as TSM 
                         do IPSL (HMS2). Na temperatura, verificou-se sinal de resfriamento 
                         durante todo ano no HM, sobre a AS, exceto no oeste da regi{\~a}o 
                         Amaz{\^o}nica, que sugere um sinal de ligeiro aquecimento. 
                         Verificou-se intensifica{\c{c}}{\~a}o do fluxo de umidade em 850 
                         hPa, sobre continente, durante o HM, consequ{\^e}ncia da 
                         intensifica{\c{c}}{\~a}o e proximidade do continente da Alta 
                         Subtropical do Atl{\^a}ntico Sul (ASAS). Este padr{\~a}o durante 
                         o ver{\~a}o no HM {\'e} similar ao observado no outono e inverno 
                         no clima presente. Tamb{\'e}m verificou-se a 
                         intensifica{\c{c}}{\~a}o do escoamento a leste dos Andes ao sul 
                         de 20šS, que sugere uma poss{\'{\i}}vel influ{\^e}ncia na 
                         intensidade da circula{\c{c}}{\~a}o do jato de baixos 
                         n{\'{\i}}veis nos regimes clim{\'a}ticos do centro oeste, sul e 
                         sudeste do Brasil. ABSTRACT: Climate variations and change are 
                         analyzed during the Mid-Holocene (MH) for South America (SA), 
                         using the atmospheric general circulation model (AGCM) from the 
                         Center for Weather Forecasts and Climate Studies (CPTEC) with a 
                         T062L28 resolution. Simulations were made by modifying the orbital 
                         parameters and CO2 concentration, using typical MH values used by 
                         other studies on MH simulations, and with sea surface temperature 
                         (SST) data from two different groups [AMIP climatologic (HMS1) and 
                         that generated by the ocean component of the coupled 
                         ocean-atmosphere from the Institute Pierre Simon Laplace-IPSL 
                         (HMS2)]. The results were compared with simulations made by 
                         previous MH climate simulations from the Paleoclimate Modeling 
                         Intercomparison Project (PMIP) I and II and paleoclimate 
                         indicators, to understand how much the CPTEC AGCM is able to 
                         simulate changes in the SA climate during the MH. A wetter 
                         behavior was detected over Northeastern SA during almost all year 
                         long, excepting from autumn where a northward displacement of the 
                         Intertropical Convergence Zone (ITCZ) is verified, associated with 
                         a weakening of the northeast trade winds and the moisture flow 
                         from Tropical Atlantic into the Amazon region. The Amazon region 
                         was found drier except in autumn and spring in the MH. The 
                         reduction of the precipitation has an important impact in the 
                         moisture transport from the Amazon basin to Parana-Plata basin, 
                         and consequently over the South Atlantic Convergence Zone (SACZ) 
                         formation, leading to a reduction of the precipitation in the SACZ 
                         current position. The SCAZ is slightly weaker during HMS1 and its 
                         existence was not detected in the experiment with IPSL TSM (HMS2). 
                         In the temperature, a signal of cooling during all over the year 
                         in the MH was verified, over SA, except in the west of the Amazon 
                         region that suggests evidences for a weak warming. Moisture flow 
                         intensification in the 850 hPa level was verified over the 
                         continent east of the Andes and South of 20 S during the MH, as 
                         consequence of the intensification and proximity of the South 
                         Atlantic Subtropical High (SASH) to the continent. These patterns, 
                         during summer in the MH, are similar to those observed in autumn 
                         and winter in the current climate. Weakening of the moisture flow 
                         from the tropical Atlantic north of 20šS to the East of the Andes 
                         was also verified.",
            committee = "Oyama, Marcos Daisuke (presidente) and Orsini, Jos{\'e} Antonio 
                         Marengo (orientador) and Reyes Fernandez, Julio Pablo and Nobre, 
                         Carlos Afonso and Pessenda, Luiz Carlos Ruiz and Dias, Pedro Leite 
                         da Silva",
           copyholder = "SID/SCD",
         englishtitle = "Climate simulations of the mid-holocene as produced by the CPTEC 
                         atmospheric general circulation model in the South America",
             language = "pt",
                pages = "201",
                  ibi = "6qtX3pFwXQZGivnK2Y/SuJ6y",
                  url = "http://urlib.net/ibi/6qtX3pFwXQZGivnK2Y/SuJ6y",
        urlaccessdate = "09 maio 2024"
}


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