@InProceedings{MeloMare:2006:SiMiHo,
author = "Melo, Maria Luciene Dias de and Marengo, Jose Antonio",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Simulations of the mid holocene climate in south America using the
CPTEC AGCM",
booktitle = "Proceedings...",
year = "2006",
editor = "Vera, Carolina and Nobre, Carlos",
pages = "307--310",
organization = "International Conference on Southern Hemisphere Meteorology and
Oceanography, 8. (ICSHMO).",
publisher = "American Meteorological Society (AMS)",
address = "45 Beacon Hill Road, Boston, MA, USA",
keywords = "mid-Holocene, Paleoclimate, past climate, orbital parameters and
climate change.",
abstract = "The objective this study is to analyze the climate and climate
variability in the Mid Holocene (6000 years before present - BP),
for South America. Grasping the past climates mechanisms and
feedbacks is of great importance in the understanding of climate
variability in the present and in future climate change
projection, using global climate models. We use the atmospheric
general circulation model (AGCM) of the CPTEC (Centro de
Previs{\~a}o de Tempo e Estudos Clim{\'a}ticos), with a
resolution of T062L28. In order to simulate the climate of the
Holocene, the orbital parameters and carbon dioxide concentration
(CO2) are changed to make them more representative of the
Mid-Holocene. Using the set of climatologic sea surface
temperature (SST) for present times as representative of the
Mid-Holocene, the effect of the orbital parameters and carbon
dioxide concentration as forcing in the simulations, the resulting
climate is analyzed in the context of present times. Later, these
simulations are compared with the Mid-Holecene simulations of a
suite of AGCMs from the Paleoclimate Modelling Intercomparison
Project (PMIP). The analysis is focused on circulation,
temperature and rainfall. Simulation of short wave radiation (SW)
in the top of the atmosphere is shown as the difference between
the Mid Holcene simulation and the control run (present climate)
and suggests that a larger amount of radiation arrives during the
austral spring (August-September) in the mid-Holocene. That agrees
with previous simulations. The temperature difference fields shows
cooling in the mid-Holocene in most of South America, except for
the south and Southeastern regions, where the model shows warming.
The precipitation difference field suggests that Northeast Brazil
was slightly more humid during the mid-Holocene and Southeastern a
little drier, as compared to present climates. The near surface
circulation fields shows that the Intertropical Convergence Zone
was located to the south of its climatological position.",
conference-location = "Foz do Igua{\c{c}}u",
conference-year = "24-28 Apr. 2006",
copyholder = "SID/SCD",
language = "en",
organisation = "American Meteorological Society (AMS)",
ibi = "cptec.inpe.br/adm_conf/2005/10.10.13.43",
url = "http://urlib.net/ibi/cptec.inpe.br/adm_conf/2005/10.10.13.43",
targetfile = "307-310.pdf",
type = "Climate change in the SH",
urlaccessdate = "19 abr. 2024"
}