FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2145665915> ?p ?o ?g. }

• W2145665915 endingPage "19790" @default.
• W2145665915 startingPage "19771" @default.
• W2145665915 abstract "Basalts from the Southwest Indian Ridge reflect a gradual, irregular isotopic transition in the MORB (mid‐ocean ridge basalt) source mantle between typical Indian Ocean‐type compositions on the east and Atlantic‐like ones on the west. A probable southwestern limit to the huge Indian Ocean isotopic domain is indicated by incompatible‐element‐depleted MORBs from 17° to 26°E, which possess essentially North Atlantic‐ or Pacific‐type signatures. Superimposed on the regional along‐axis gradient are at least three localized types of isotopically distinct, incompatible‐element‐enriched basalts. One characterizes the ridge between 36° and 39°E, directly north of the proposed Marion hotspot, and appears to be caused by mixing between hotspot and high ∈ Nd , normal MORB mantle; oceanic island products of the hotspot itself exhibit a very restricted range of isotopic values (e.g., 206 Pb/ 204 Pb = 18.5–18.6) which are more MORB‐like than those of other Indian Ocean islands. Between 39° and 41°E, high Ba/Nb lavas with unusually low 206 Pb/ 204 Pb (16.87–17.44) and ∈ Nd (−4 to +3) are dominant; these compositions are not only unlike those of the Marion (or any other) hotspot but also are unique among MORBs globally. Incompatible‐elementenriched lavas in the vicinity of the Indomed Fracture Zone (∼46°E) differ isotopically from those at 39°–41°E, 36°–39°E, and both the Marion and Crozet hotspots. Thus, no simple model of ridgeward flow of plume mantle can explain the presence or distribution of all the incompatible‐element‐enriched MORBs on the central Southwest Indian Ridge. The upper mantle at 39°–41°E, in particular, may contain stranded continental lithosphere, thermally eroded from Indo‐Madagascar in the middle Cretaceous. Alternatively, the composition of the; Marion hotspot must be grossly heterogeneous in space and/or time, and one of its intrinsic components must have substantially lower 206 Pb/ 204 Pb than yet measured for any hotspot. The origin of the broadly similar but much less extreme isotopic signatures of MORBs throughout most of the Indian Ocean could be related to the initiation of the Marion, Kerguelen, and Crozet hotspots, which together may have formed a more than 4400‐km‐long band of juxtaposed plume heads beneath the nearly stationary lithosphere of prebreakup Gondwana." @default.
• W2145665915 created "2016-06-24" @default.
• W2145665915 creator A5037001562 @default.
• W2145665915 creator A5055355437 @default.
• W2145665915 creator A5060793840 @default.
• W2145665915 creator A5063906827 @default.
• W2145665915 creator A5087209075 @default.
• W2145665915 date "1992-12-10" @default.
• W2145665915 modified "2023-10-18" @default.
• W2145665915 title "Southwestern limits of Indian Ocean Ridge Mantle and the origin of low ²⁰⁶Pb/²⁰⁴Pb mid‐ocean ridge basalt: Isotope systematics of the central Southwest Indian Ridge (17°–50°E)" @default.
• W2145665915 cites W1581358550 @default.
• W2145665915 cites W1961804608 @default.
• W2145665915 cites W1964725979 @default.
• W2145665915 cites W1964975629 @default.
• W2145665915 cites W1965410050 @default.
• W2145665915 cites W1966917681 @default.
• W2145665915 cites W1966918338 @default.
• W2145665915 cites W1968122867 @default.
• W2145665915 cites W1968206413 @default.
• W2145665915 cites W1970194063 @default.
• W2145665915 cites W1970947232 @default.
• W2145665915 cites W1977793670 @default.
• W2145665915 cites W1978265571 @default.
• W2145665915 cites W1978788058 @default.
• W2145665915 cites W1982431325 @default.
• W2145665915 cites W1985040296 @default.
• W2145665915 cites W1988908945 @default.
• W2145665915 cites W1995720681 @default.
• W2145665915 cites W1995857854 @default.
• W2145665915 cites W1997722926 @default.
• W2145665915 cites W2006372142 @default.
• W2145665915 cites W2010846207 @default.
• W2145665915 cites W2011580798 @default.
• W2145665915 cites W2022648729 @default.
• W2145665915 cites W2025049414 @default.
• W2145665915 cites W2028135028 @default.
• W2145665915 cites W2028495206 @default.
• W2145665915 cites W2030466700 @default.
• W2145665915 cites W2032347816 @default.
• W2145665915 cites W2032800272 @default.
• W2145665915 cites W2039100744 @default.
• W2145665915 cites W2045064243 @default.
• W2145665915 cites W2048090129 @default.
• W2145665915 cites W2051226147 @default.
• W2145665915 cites W2052984571 @default.
• W2145665915 cites W2054486238 @default.
• W2145665915 cites W2055309769 @default.
• W2145665915 cites W2058031585 @default.
• W2145665915 cites W2061397657 @default.
• W2145665915 cites W2062346847 @default.
• W2145665915 cites W2062708633 @default.
• W2145665915 cites W2066335781 @default.
• W2145665915 cites W2067481326 @default.
• W2145665915 cites W2073599973 @default.
• W2145665915 cites W2073754098 @default.
• W2145665915 cites W2092473060 @default.
• W2145665915 cites W2093567690 @default.
• W2145665915 cites W2094025567 @default.
• W2145665915 cites W2095203624 @default.
• W2145665915 cites W2095320098 @default.
• W2145665915 cites W2103311221 @default.
• W2145665915 cites W2119482687 @default.
• W2145665915 cites W2141723634 @default.
• W2145665915 cites W2159506096 @default.
• W2145665915 cites W2314202908 @default.
• W2145665915 cites W2314777318 @default.
• W2145665915 cites W265672673 @default.
• W2145665915 cites W2915997760 @default.
• W2145665915 cites W4211037545 @default.
• W2145665915 cites W61168061 @default.
• W2145665915 doi "https://doi.org/10.1029/92jb01424" @default.
• W2145665915 hasPublicationYear "1992" @default.
• W2145665915 type Work @default.
• W2145665915 sameAs 2145665915 @default.
• W2145665915 citedByCount "259" @default.
• W2145665915 countsByYear W21456659152012 @default.
• W2145665915 countsByYear W21456659152013 @default.
• W2145665915 countsByYear W21456659152014 @default.
• W2145665915 countsByYear W21456659152015 @default.
• W2145665915 countsByYear W21456659152016 @default.
• W2145665915 countsByYear W21456659152017 @default.
• W2145665915 countsByYear W21456659152018 @default.
• W2145665915 countsByYear W21456659152019 @default.
• W2145665915 countsByYear W21456659152020 @default.
• W2145665915 countsByYear W21456659152021 @default.
• W2145665915 countsByYear W21456659152022 @default.
• W2145665915 countsByYear W21456659152023 @default.
• W2145665915 crossrefType "journal-article" @default.
• W2145665915 hasAuthorship W2145665915A5037001562 @default.
• W2145665915 hasAuthorship W2145665915A5055355437 @default.
• W2145665915 hasAuthorship W2145665915A5060793840 @default.
• W2145665915 hasAuthorship W2145665915A5063906827 @default.
• W2145665915 hasAuthorship W2145665915A5087209075 @default.
• W2145665915 hasConcept C121332964 @default.
• W2145665915 hasConcept C127313418 @default.
• W2145665915 hasConcept C146481406 @default.
• W2145665915 hasConcept C147894010 @default.
• W2145665915 hasConcept C151730666 @default.

• next