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dc.contributor.authorKoopmans, L.
dc.contributor.authorMcCarthy, W.
dc.contributor.authorMagee, C.
dc.date.accessioned2022-03-02T11:30:26Z
dc.date.available2022-03-02T11:30:26Z
dc.date.issued2022-03-01
dc.identifier278023854
dc.identifiera32ca3eb-4e14-4c99-bc5a-4a5e94f198d7
dc.identifier000776516500018
dc.identifier85127230183
dc.identifier.citationKoopmans , L , McCarthy , W & Magee , C 2022 , ' Dyke architecture, mineral layering, and magmatic convection; new perspectives from the Younger Giant Dyke Complex, S Greenland ' , Geochemistry, Geophysics, Geosystems , vol. 23 , no. 3 , e2021GC010260 . https://doi.org/10.1029/2021GC010260en
dc.identifier.issn1525-2027
dc.identifier.otherRIS: urn:6C71E4783CCD0063FA5A833C000D62C1
dc.identifier.otherORCID: /0000-0002-7214-1449/work/109316248
dc.identifier.urihttps://hdl.handle.net/10023/24978
dc.descriptionThe expedition was funded by the Mining Institute of Scotland Trust, the Institute of Materials, Minerals and Mining, the Society of Economic Geologists Hickok-Radford Fund, the Edinburgh Geological Society, the Augustine Courtauld trust and the Scott Polar Research Institute.en
dc.description.abstractIgneous sheet intrusions are a fundamental component of volcano plumbing systems. Identifying how sheet intrusion emplacement and geometry controls later magmatic processes is critical to understanding the distribution of volcanic eruptions and magma-related ore deposits. Using the Younger Giant Dyke Complex, a Mesoproterozoic suite of large (< 800 m wide) mafic dykes in southern Greenland, we assess the influence sheet of emplacement and geometry on subsequent magma flow and mush evolution. Through structural mapping, petrographic observations, and anisotropy of magnetic susceptibility fabric analyses, we show that the Younger Giant Dyke Complex was emplaced as a series of individual dyke segments, which following coalescence into a sheet intrusion remained largely isolated during their magmatic evolution. Through petrographic evidence for liquid-rich growth of cumulus phases, concentric magnetic fabrics, and the detailed study layered zones within the Younger Giant Dyke Complex, we infer magma convection occurred within the cores of each dyke element. We particularly relate layering to hydrodynamic sorting processes at a magma-mush boundary towards the base of each convection cell. Overall, our work demonstrates that the initial geometry of sheet intrusions can constrain magma flow patterns and affect the distribution of crystallisation regimes.
dc.format.extent22
dc.format.extent9286619
dc.language.isoeng
dc.relation.ispartofGeochemistry, Geophysics, Geosystemsen
dc.subjectAnisotropy of magnetic susceptibilityen
dc.subjectLayered igneous systemsen
dc.subjectRock magneticsen
dc.subjectMagma chamber processesen
dc.subjectMesoproterozoicen
dc.subjectSheet segmentationen
dc.subjectQE Geologyen
dc.subjectDASen
dc.subjectMCCen
dc.subject.lccQEen
dc.titleDyke architecture, mineral layering, and magmatic convection; new perspectives from the Younger Giant Dyke Complex, S Greenlanden
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. St Andrews Isotope Geochemistryen
dc.identifier.doihttps://doi.org/10.1029/2021GC010260
dc.description.statusPeer revieweden


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