2018
DOI: 10.1016/j.quascirev.2018.01.013
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The MIS 3 maximum of the Torres del Paine and Última Esperanza ice lobes in Patagonia and the pacing of southern mountain glaciation

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Cited by 50 publications
(108 citation statements)
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“…Although some glaciers showed extensive retreat at this time and never recovered, other glaciers readvanced to full glacial extent until the very end of the LGM at 18 ka, giving a short-term asymmetry of Patagonian glacier responses to the deglacial signal. The close paleoclimate link between the WDC and some Patagonian glacier records exposes the sensitivity of both sites to the changes in the Southern Ocean sea surface temperatures and sea ice extent, ultimately controlled by local insolation (WAIS Divide Project Members, 2013), and thereby suggesting a paleoclimate teleconnection between mid- and high latitudes (e.g., Kaplan et al 2008; Denton et al, 2010; WAIS Divide Project Members, 2013; Darvill et al, 2016; García et al, 2018).…”
Section: Discussionmentioning
confidence: 99%
“…Although some glaciers showed extensive retreat at this time and never recovered, other glaciers readvanced to full glacial extent until the very end of the LGM at 18 ka, giving a short-term asymmetry of Patagonian glacier responses to the deglacial signal. The close paleoclimate link between the WDC and some Patagonian glacier records exposes the sensitivity of both sites to the changes in the Southern Ocean sea surface temperatures and sea ice extent, ultimately controlled by local insolation (WAIS Divide Project Members, 2013), and thereby suggesting a paleoclimate teleconnection between mid- and high latitudes (e.g., Kaplan et al 2008; Denton et al, 2010; WAIS Divide Project Members, 2013; Darvill et al, 2016; García et al, 2018).…”
Section: Discussionmentioning
confidence: 99%
“…García et al, 2019;Iglesias et al, 2016;Van Daele et al, 2016) there remains a general lack of published detailed mapping and geochronological data across the northeastern sector of the former ice sheet, between ∼39°S and ∼46.5°S (Darvill et al, 2015;Davies et al, 2020;Mendelová et al, 2017). Robust reconstructions from this region are needed to understand fully the PIS response to the Last Glacial Maximum (LGM) at these latitudes, and to investigate latitudinal dependencies on the timing of the local LGM throughout Patagonia (Darvill et al, 2015;Davies et al, 2020;García et al, 2018;Sagredo et al, 2011). A vital component of such reconstructions is detailed, glacier-scale geomorphological mapping (Chandler et al, 2018;Clark et al, 2018;Evans & Orton, 2015).…”
Section: Introductionmentioning
confidence: 99%
“…Even when the nature of these millennial-scale climate changes are still a subject of debate and we cannot expect to find their record in our coastal assemblages (sea level was lower than present during MIS 4-3), they are documented for southern South America, both in surface waters off Chile (Lamy et al, 2004;Kaiser et al, 2005) and in the Andean continental record (García et al, 2018), and northwards off Brazil (Carvahlo-Campos et al, 2016). The less stable climate during MIS 3 and MIS 2 compared to MIS5 (Brook and Buizert, 2018) and the associated oscillations in atmospheric CO 2 concentrations -that remain so far unexplained or at least poorly constrained-, in the southern westerlies wind belt position, in release of icebergs, subglacial meltwater and in iron inputs from icebergs/meltwater around western Antarctica-Drake Passage must have had pronounced impacts on productivity (Ó Cofaigh et al, 2014;Armour and Bitz, 2015;Gottschalk et al, 2016) and are expected to have affected the geochemical properties of the southern SWA in a measurable way.…”
Section: Which Changes Could Explain the Different Holocene Pattern?mentioning
confidence: 91%
“…11C) a number of environmental changes were reported to have occurred linked to Patagonia including the rising sea-level from the Last Glacial Maximum (MIS 2; lowest sea-level globally at -120 m ca. 22 ka or 48 ka in southern Chile; García et al, 2018) across the glacial-interglacial transition (−40 m at ca. 11 ka) into the Holocene (Ponce et al, 2011;Isla and Schnack, 2016).…”
Section: Which Changes Could Explain the Different Holocene Pattern?mentioning
confidence: 99%