Matches in SemOpenAlex for { <https://semopenalex.org/work/W2743489374> ?p ?o ?g. }
- W2743489374 endingPage "276" @default.
- W2743489374 startingPage "263" @default.
- W2743489374 abstract "Recognition of the nature of potential mantle sources of continental flood basalts is complicated by possible overprinting related to crustal contamination as magmas migrate to the surface (Arndt and Christensen, 1992). However, in picritic lava flows primitive olivine phenocrysts that formed early in the crystallization sequence can potentially provide unperturbed information of their mantle source. We have carried out an integrated chemical and oxygen isotopic (in situ SIMS) study of primitive olivine grains (Fo ranging from 88 to 92.6 mol%) in the Emeishan picrites at different locations (Wulongba, Wuguijing, Tanglanghe and Maoniuping). We use these data to evaluate the geochemical nature of mantle sources for magmas from which the primitive olivine crystallized. The primitive olivine grains in the samples from Maoniuping, Wuguijing and Tanglanghe are characterized by mantle-like δ18O values (mean values are 5.1 ± 0.3‰ (2σ, n = 53), 5.2 ± 0.3‰ (2σ, n = 122) and 5.3 ± 0.3‰ (n = 25), respectively) coupled with generally low Fo contents (mean values are 88.7 ± 1.4 mol% (2σ, n = 53), 89.8 ± 1.8 mol% (2σ, n = 122) and 89.4 ± 1.8 mol% (2σ, n = 25), respectively). In contrast, the olivine grains in the samples from Wulongba are characterized by elevated δ18O values (mean = 5.6 ± 0.3‰ (2σ, n = 58)) coupled with generally higher Fo contents (mean = 91 ± 2.8 mol% (2σ, n = 58)) than primitive olivine in the samples from the other locations. Based on olivine compositions, primitive olivine in picrites from Maoniuping, Tanglanghe and Wuguijing are consistent with derivation from hybrid mantle sources containing similar proportions of peridotite and pyroxenite/eclogite components. The δ18O values of these primitive olivine grains are consistent with melting of plume source materials. The chemical composition of the primitive olivine from Wulongba are also consistent with derivation from a hybrid peridotite/pyroxenite source, but the high δ18O values suggest that at least locally the pyroxenitic source was characterized by 18O-enrichment related to a higher degree of seawater interaction with the oceanic crust protolith. An alternative explanation is that olivine in the Wulongba picrite reflects derivation from lithospheric mantle that was modified by subduction-related processes in the Neoproterozoic. The high-Fo content of the Wulongba picrites may be due to the higher fO2 conditions of the partial melt generated in the subduction modified lithospheric mantle, or to a higher degree of partial melting." @default.
- W2743489374 created "2017-08-17" @default.
- W2743489374 creator A5007388525 @default.
- W2743489374 creator A5011065438 @default.
- W2743489374 creator A5014742790 @default.
- W2743489374 creator A5060933989 @default.
- W2743489374 creator A5062195279 @default.
- W2743489374 creator A5080552201 @default.
- W2743489374 date "2017-10-01" @default.
- W2743489374 modified "2023-10-12" @default.
- W2743489374 title "An integrated chemical and oxygen isotopic study of primitive olivine grains in picrites from the Emeishan Large Igneous Province, SW China: Evidence for oxygen isotope heterogeneity in mantle sources" @default.
- W2743489374 cites W1026197542 @default.
- W2743489374 cites W1527757327 @default.
- W2743489374 cites W1971003680 @default.
- W2743489374 cites W1978484550 @default.
- W2743489374 cites W1979082610 @default.
- W2743489374 cites W1979704880 @default.
- W2743489374 cites W1981002430 @default.
- W2743489374 cites W1988978036 @default.
- W2743489374 cites W1990740187 @default.
- W2743489374 cites W1995582998 @default.
- W2743489374 cites W1998707404 @default.
- W2743489374 cites W2001022785 @default.
- W2743489374 cites W2004240468 @default.
- W2743489374 cites W2005539087 @default.
- W2743489374 cites W2010771702 @default.
- W2743489374 cites W2013259970 @default.
- W2743489374 cites W2014338623 @default.
- W2743489374 cites W2016060298 @default.
- W2743489374 cites W2017247293 @default.
- W2743489374 cites W2024203368 @default.
- W2743489374 cites W2031194632 @default.
- W2743489374 cites W2035383650 @default.
- W2743489374 cites W2037386539 @default.
- W2743489374 cites W2042860388 @default.
- W2743489374 cites W2045511581 @default.
- W2743489374 cites W2049566684 @default.
- W2743489374 cites W2051704045 @default.
- W2743489374 cites W2053273118 @default.
- W2743489374 cites W2055779151 @default.
- W2743489374 cites W2055859870 @default.
- W2743489374 cites W2056509981 @default.
- W2743489374 cites W2056583736 @default.
- W2743489374 cites W2061751167 @default.
- W2743489374 cites W2062471418 @default.
- W2743489374 cites W2066300646 @default.
- W2743489374 cites W2066695862 @default.
- W2743489374 cites W2069053606 @default.
- W2743489374 cites W2072709625 @default.
- W2743489374 cites W2073474967 @default.
- W2743489374 cites W2087494921 @default.
- W2743489374 cites W2088278318 @default.
- W2743489374 cites W2090035514 @default.
- W2743489374 cites W2090185758 @default.
- W2743489374 cites W2090640707 @default.
- W2743489374 cites W2095108102 @default.
- W2743489374 cites W2095293218 @default.
- W2743489374 cites W2098391368 @default.
- W2743489374 cites W2102405759 @default.
- W2743489374 cites W2111918073 @default.
- W2743489374 cites W2115096774 @default.
- W2743489374 cites W2130958906 @default.
- W2743489374 cites W2132697398 @default.
- W2743489374 cites W2134504371 @default.
- W2743489374 cites W2138522501 @default.
- W2743489374 cites W2140136526 @default.
- W2743489374 cites W2147038702 @default.
- W2743489374 cites W2153857340 @default.
- W2743489374 cites W2157202268 @default.
- W2743489374 cites W2160619377 @default.
- W2743489374 cites W2160773634 @default.
- W2743489374 cites W2162017737 @default.
- W2743489374 cites W2163156840 @default.
- W2743489374 cites W2255407013 @default.
- W2743489374 cites W2281399880 @default.
- W2743489374 cites W2331988102 @default.
- W2743489374 cites W2522029964 @default.
- W2743489374 cites W2602002743 @default.
- W2743489374 cites W2724853380 @default.
- W2743489374 cites W3148515913 @default.
- W2743489374 cites W4377589703 @default.
- W2743489374 doi "https://doi.org/10.1016/j.gca.2017.08.007" @default.
- W2743489374 hasPublicationYear "2017" @default.
- W2743489374 type Work @default.
- W2743489374 sameAs 2743489374 @default.
- W2743489374 citedByCount "31" @default.
- W2743489374 countsByYear W27434893742017 @default.
- W2743489374 countsByYear W27434893742018 @default.
- W2743489374 countsByYear W27434893742019 @default.
- W2743489374 countsByYear W27434893742020 @default.
- W2743489374 countsByYear W27434893742021 @default.
- W2743489374 countsByYear W27434893742022 @default.
- W2743489374 countsByYear W27434893742023 @default.
- W2743489374 crossrefType "journal-article" @default.
- W2743489374 hasAuthorship W2743489374A5007388525 @default.
- W2743489374 hasAuthorship W2743489374A5011065438 @default.
- W2743489374 hasAuthorship W2743489374A5014742790 @default.
- W2743489374 hasAuthorship W2743489374A5060933989 @default.