2016
DOI: 10.1016/j.quascirev.2016.01.029
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Peruvian sediments as recorders of an evolving hiatus for the last 22 thousand years

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Cited by 24 publications
(22 citation statements)
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“…Core 029 from 9°S at 400 m water depth is located within an area where at present only small amounts of sediment are deposited due to high‐energy hydrographic conditions, such as peak velocities of the PCUC (for details see Erdem et al . []). Hence, both the modern and Holocene SRs (11–20 cm ka −1 ) and ARs (mean AR bSi value = 1.1 g cm −2 ka −1 ) were relatively low (Figure f).…”
Section: Resultsmentioning
confidence: 99%
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“…Core 029 from 9°S at 400 m water depth is located within an area where at present only small amounts of sediment are deposited due to high‐energy hydrographic conditions, such as peak velocities of the PCUC (for details see Erdem et al . []). Hence, both the modern and Holocene SRs (11–20 cm ka −1 ) and ARs (mean AR bSi value = 1.1 g cm −2 ka −1 ) were relatively low (Figure f).…”
Section: Resultsmentioning
confidence: 99%
“…The age model of core 052 [ Erdem et al ., ] is based on five Accelerator Mass Spectrometer (AMS) 14 C datings of the planktonic foraminifera species Neogloboquadrina dutertrei in combination with orbital tuning of δ 18 O values of nearby core M77/2‐059 [ Mollier‐Vogel et al ., ] and supported by correlation to the δ 18 O of the EPICA ice core [ European Project for Ice Coring in Antarctica Community Members , 2006]. The conventional radiocarbon dates were calibrated using the software Calib 7.0 and applying the marine calibration set Marine13 [ Reimer and Bard , ].…”
Section: Methodsmentioning
confidence: 99%
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“…The age model of the core M77/2-59-1 (3°57'S 997 m) was established by (Mollier-Vogel et al, 2013). Age models of the other cores were previously described elsewhere (Erdem et al, 2016). Sedimentary δ 15 N data of core 52-2 and 59-1 were taken from Glock et al (2018) and Mollier-Vogel et al (2019), respectively (Table 3).…”
Section: Sediment Coresmentioning
confidence: 99%
“…The two most important are waves sourced by the strong westerly winds in the Southern Ocean (Beccario, http://earth.nullschool.net) [ López et al ., ] and along‐margin oceanic currents such as the Peru‐Chile (Humboldt) Currents [ Chaigneau et al ., ] (Figure ). Sediment archives at the seafloor from 3°S to 18°S are characteristic of current‐dominated regimes [ Reinhardt et al ., ] with ongoing phosphorite formation, tide‐topography interaction, and resultant nonlinear internal waves [ Erdem et al ., ]. Mooring experiments documented current speeds of up to 20 cm/s in the upper 200 m of the continental shelf of Peru from 5°S to 15°30′S [ Brockmann et al ., ].…”
Section: Introductionmentioning
confidence: 99%