2013
DOI: 10.1134/s1028334x13060111
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Stratigraphy of bottom sediments in the Mendeleev Ridge area (Arctic Ocean)

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Cited by 10 publications
(11 citation statements)
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“…The present study adds credibility to the methodological approach outlined by Somayajulu et al (), further developed by Not and Hillaire‐Marcel () and recently applied by Gusev et al () for the setting of radiometric benchmark ages of ∼140 and ∼300 ka based on the extinction of excesses in 231 Pa and 230 Th, respectively, in low sedimentation rate environments. In the case of the northern Lomonosov and Mendeleev Ridge, this approach suggests average sedimentation rates of the order of 4.3 and 1.7 mm/ka, respectively, during the late Quaternary.…”
Section: Discussionsupporting
confidence: 80%
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“…The present study adds credibility to the methodological approach outlined by Somayajulu et al (), further developed by Not and Hillaire‐Marcel () and recently applied by Gusev et al () for the setting of radiometric benchmark ages of ∼140 and ∼300 ka based on the extinction of excesses in 231 Pa and 230 Th, respectively, in low sedimentation rate environments. In the case of the northern Lomonosov and Mendeleev Ridge, this approach suggests average sedimentation rates of the order of 4.3 and 1.7 mm/ka, respectively, during the late Quaternary.…”
Section: Discussionsupporting
confidence: 80%
“…At this stage, a summary of the most robust features of 230 Th xs behavior in sediments from the central Arctic Ocean can be made: 230 Th xs ‐fluxes and inventories are similar in the Mendeleev and Lomonosov cores examined above (Figure ), likely in several other sites of the central Arctic Ocean (Gusev et al, ; Huh et al, ; Moran et al, ) and seem thus independent of the site within this area. 230 Th xs ‐fluxes and inventories are independent of the depth of the water column within the range documented here, i.e., from ∼1.2 km (Mendeleev MC‐12; Lomonosov‐030) to ∼2.5 km (Mendeleev MC‐11); thus 230 Th‐scavenging has to occur mostly outside the overlying water column and/or through a still undocumented process. If 230 Th xs ‐fluxes vary in accordance with sediment fluxes (cf. Figure b), 230 Th xs ‐inventories are independent of the sediment accumulation as illustrated by their similarity in cores from both Mendeleev and Lomonosov (MC‐11, Mc‐030, and K‐030) (Figure ), notwithstanding a 3‐fold difference in the sediment accumulation rate between the two ridges. …”
Section: Discussionmentioning
confidence: 51%
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“…If this is always the case, magnetostratigraphy will probably not be useful for the construction of a chronology for abyssal sediment sequences from the Arctic Ocean. Nevertheless, recent geochemical studies involving decay of Be (e.g., Sellén et al, ) and U‐series isotopes (e.g., Gusev et al, ; Hillaire‐Marcel et al, ; Not & Hillaire‐Marcel, ) indicate that sedimentation rates are close to those (one to several mm/kyr) originally estimated by the early magnetostratigraphic studies. All these facts indicate that challenges and uncertainty remain in the establishment of age models for the deep‐sea sediment cores and especially for the applicability and interpretation of magnetic stratigraphy in the Arctic Ocean.…”
Section: Introductionmentioning
confidence: 66%