Regionalization of the Atmospheric Dust Cycle on the Periphery of the East Antarctic Ice Sheet Since the Last Glacial Maximum

Autor: Baccolo G.[1, 2, Delmonte B.[2], Albani S.[4], Baroni C.[5, Cibin G.[7], Frezzotti M.[8], Hampai D.[9], Marcelli A.[9, 10] Revel M.[11], Salvatore M.C.[5, 6] Stenni B.[12], Maggi V.[2
Přispěvatelé: Department of Earth and Environmental Sciences [Milano], Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Earth Sciences Department, University of Pisa - Università di Pisa, DIAMOND Light source, Italian National agency for new technologies, Energy and sustainable economic development [Frascati] (ENEA), INFN Frascati, Istituto Nazionale di Fisica Nucleare (INFN), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Department of Environmental Sciences, Informatics and Statistics [Venezia], University of Ca’ Foscari [Venice, Italy], Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Baccolo, G., Delmonte, B., Albani, S., Baroni, Carlo, Cibin, G., Frezzotti, M., Hampai, D., Marcelli, A., Revel, M., Salvatore, M. C., Stenni, B., Maggi, V., Baccolo, G, Delmonte, B, Albani, S, Baroni, C, Cibin, G, Frezzotti, M, Hampai, D, Marcelli, A, Revel, M, Salvatore, M, Stenni, B, Maggi, V
Jazyk: angličtina
Rok vydání: 2018
Předmět:
Zdroj: Geochemistry, Geophysics, Geosystems
Geochemistry, Geophysics, Geosystems, AGU and the Geochemical Society, 2018, 19 (9), pp.3540-3554. ⟨10.1029/2018GC007658⟩
Geochemistry, geophysics, geosystems 19 (2018): 3540–3554. doi:10.1029/2018GC007658
info:cnr-pdr/source/autori:Baccolo G.[1,2,3], Delmonte B.[2], Albani S.[4], Baroni C.[5,6], Cibin G.[7], Frezzotti M.[8], Hampai D.[9], Marcelli A.[9,10] Revel M.[11], Salvatore M.C.[5,6] Stenni B.[12], Maggi V.[2,3]/titolo:Regionalization of the Atmospheric Dust Cycle on the Periphery of the East Antarctic Ice Sheet Since the Last Glacial Maximum/doi:10.1029%2F2018GC007658/rivista:Geochemistry, geophysics, geosystems/anno:2018/pagina_da:3540/pagina_a:3554/intervallo_pagine:3540–3554/volume:19
Geochemistry, Geophysics, Geosystems, 2018, 19 (9), pp.3540-3554. ⟨10.1029/2018GC007658⟩
ISSN: 1525-2027
Popis: Ice cores from inner East Antarctica provided some of the longest and most detailed climatic reconstructions and allowed understanding the relationships between atmospheric mineral dust and climate. In this work we present synchrotron radiation X-ray Fluorescence geochemical data of dust from the TALDICE ice core drilled at Talos Dome, a peripheral ice dome of East Antarctica (Western Ross Sea). Results highlight a dominant southern South American origin for dust at TALDICE during the Last Glacial Maximum, similarly to other sites located further inland onto the polar plateau. On the contrary, a different scenario concerns Talos Dome during the Holocene if it is compared to more inner sites. The tight connection between high southern latitudes and Antarctica that characterizes cold climate stages becomes weaker since the onset of the last climatic transition and throughout the Holocene. The net effect of this process at Talos Dome is a modification of the atmospheric and environmental settings, owing to local Antarctic sources of Victoria Land to gain importance and become the dominant ones. At the same time in inner East Antarctica the provenance of dust remains remote also during Holocene, revealing an evolution of the homogeneous scenario observed in glacial periods. The enhanced sensitivity of peripheral ice sheet sites to local dust sources makes Talos Dome an ideal site to assess the climatic and atmospheric changes of the peripheral sectors of East Antarctica during the current interglacial period.Plain Language Summary During the Last Glacial Maximum, about 20,000 years ago, mineral dust from South America was massively transported toward Antarctica as a consequence of impressive environmental and climatic changes. Many ice cores drilled from the inner sectors of the Antarctic ice sheets support this scenario. Little is known when attention is shifted to peripheral areas and to interglacial periods. A new record of mineral particles at Talos Dome, a peripheral area of the East Antarctic ice sheet (Western Ross Sea sector), is here presented to partially close these gaps. Combining the data about concentration, composition, and grain size of the dust deposited at Talos Dome, it was possible to appreciate the influence played by local Antarctic dust sources to the depositional budget of the site. These local sources, corresponding to localized ice-free areas, are extremely important when attention is given to the peripheries of the ice sheets. This is particularly true for interglacial periods, when the transport and the deposition of mineral dust from South America to Antarctica is much reduced.
Databáze: OpenAIRE
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