On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models
Differences between climate conditions during the Last Glacial Maximum (LGM) and the Mid-Holocene (MH) in southern South America inferred from the state-of-the-art PMIP3 paleoclimatic simulations are described for the first time in this paper. The aim is to expose characteristics of past climate cha...
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02773791_v185_n_p113_Berman http://hdl.handle.net/20.500.12110/paper_02773791_v185_n_p113_Berman |
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paper:paper_02773791_v185_n_p113_Berman2023-06-08T15:25:59Z On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models Last Glacial Maximum Mid-Holocene Pampa Patagonia PMIP3 models South America Climate change Glacial geology Holocenes Last Glacial Maximum Pampa Patagonia South America Climate models air temperature climate conditions Holocene Last Glacial Maximum numerical model paleoclimate precipitation (climatology) Andes Argentina Cordillera Pampas Paraguay Patagonia Differences between climate conditions during the Last Glacial Maximum (LGM) and the Mid-Holocene (MH) in southern South America inferred from the state-of-the-art PMIP3 paleoclimatic simulations are described for the first time in this paper. The aim is to expose characteristics of past climate changes occurred without human influence. In this context, numerical simulations are an indispensable tool for inferring changes in near-surface air temperature and precipitation in regions where proxy information is scarce or absent. The analyzed PMIP3 models describe MH temperatures significantly warmer than those of LGM with magnitudes of change depending on the season and the specific geographic region. In addition, models indicate that seasonal mean precipitation during MH increased with respect to LGM values in wide southern continental areas to the east of the Andes Cordillera whereas seasonal precipitation developed in areas to the west of Patagonian Andes reduced from LGM to MH. © 2018 Elsevier Ltd 2018 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02773791_v185_n_p113_Berman http://hdl.handle.net/20.500.12110/paper_02773791_v185_n_p113_Berman |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Last Glacial Maximum Mid-Holocene Pampa Patagonia PMIP3 models South America Climate change Glacial geology Holocenes Last Glacial Maximum Pampa Patagonia South America Climate models air temperature climate conditions Holocene Last Glacial Maximum numerical model paleoclimate precipitation (climatology) Andes Argentina Cordillera Pampas Paraguay Patagonia |
spellingShingle |
Last Glacial Maximum Mid-Holocene Pampa Patagonia PMIP3 models South America Climate change Glacial geology Holocenes Last Glacial Maximum Pampa Patagonia South America Climate models air temperature climate conditions Holocene Last Glacial Maximum numerical model paleoclimate precipitation (climatology) Andes Argentina Cordillera Pampas Paraguay Patagonia On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models |
topic_facet |
Last Glacial Maximum Mid-Holocene Pampa Patagonia PMIP3 models South America Climate change Glacial geology Holocenes Last Glacial Maximum Pampa Patagonia South America Climate models air temperature climate conditions Holocene Last Glacial Maximum numerical model paleoclimate precipitation (climatology) Andes Argentina Cordillera Pampas Paraguay Patagonia |
description |
Differences between climate conditions during the Last Glacial Maximum (LGM) and the Mid-Holocene (MH) in southern South America inferred from the state-of-the-art PMIP3 paleoclimatic simulations are described for the first time in this paper. The aim is to expose characteristics of past climate changes occurred without human influence. In this context, numerical simulations are an indispensable tool for inferring changes in near-surface air temperature and precipitation in regions where proxy information is scarce or absent. The analyzed PMIP3 models describe MH temperatures significantly warmer than those of LGM with magnitudes of change depending on the season and the specific geographic region. In addition, models indicate that seasonal mean precipitation during MH increased with respect to LGM values in wide southern continental areas to the east of the Andes Cordillera whereas seasonal precipitation developed in areas to the west of Patagonian Andes reduced from LGM to MH. © 2018 Elsevier Ltd |
title |
On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models |
title_short |
On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models |
title_full |
On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models |
title_fullStr |
On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models |
title_full_unstemmed |
On the differences between Last Glacial Maximum and Mid-Holocene climates in southern South America simulated by PMIP3 models |
title_sort |
on the differences between last glacial maximum and mid-holocene climates in southern south america simulated by pmip3 models |
publishDate |
2018 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02773791_v185_n_p113_Berman http://hdl.handle.net/20.500.12110/paper_02773791_v185_n_p113_Berman |
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1768544501160214528 |