2013
DOI: 10.1016/j.chemgeo.2012.11.012
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Campaign-style titanite U–Pb dating by laser-ablation ICP: Implications for crustal flow, phase transformations and titanite closure

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Cited by 223 publications
(225 citation statements)
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“…The heavy mineral residues were mounted on microscope slides (Mange & Maurer, 1992) using Meltmount TM with a refraction of 1.66 and identified under the polarising microscope, with the relative abundances determined by grain counting. For that, the microscope slide was moved along linear traverses and all grains between two parallel lines were counted (i.e., ribbon counting; (Root et al, 2005;Spencer et al, 2013;Bradley R. Hacker, pers. comm., 2014;own field observations).…”
Section: Methodsmentioning
confidence: 99%
“…The heavy mineral residues were mounted on microscope slides (Mange & Maurer, 1992) using Meltmount TM with a refraction of 1.66 and identified under the polarising microscope, with the relative abundances determined by grain counting. For that, the microscope slide was moved along linear traverses and all grains between two parallel lines were counted (i.e., ribbon counting; (Root et al, 2005;Spencer et al, 2013;Bradley R. Hacker, pers. comm., 2014;own field observations).…”
Section: Methodsmentioning
confidence: 99%
“…In the WGR they record chiefly Barrovian peak metamorphic conditions of~650-800°C and~1 GPa (Fig. 2) [Terry et al, 2000;Hacker et al, 2003;Labrousse et al, 2004;Walsh and Hacker, 2004;Root et al, 2005;Johnston et al, 2007a;Spencer et al, 2013;Fauconnier et al, 2014]. This was accompanied by partial melting that was locally extensive in the hinterland, but progressively more feeble toward the foreland [Ganzhorn et al, 2014] [Hacker et al, 2010 #5959] [ Kylander-Clark and Hacker, 2014].…”
Section: Geologic Settingmentioning
confidence: 99%
“…Like most well-exposed and extensively investigated UHP terranes, the WGR is dominated by quartzofeldspathic gneiss; eclogite and (U)HP peridotite comprise only a few volume percent of the Region. The quartzofeldspathic gneiss and eclogite protoliths formed chiefly by magmatism at~1.68-1.64 Ga, 1.29-1.24 Ga, and~990-950 Ma [Corfu and Andersen, 2002;Walsh et al, 2007;Krogh et al, 2011;Corfu et al, 2013]; regional metamorphism [Roffeis and Corfu, 2014] associated with the~1.0-0.9 Ga magmatism reached temperatures of~775-825°C [Spencer et al, 2013]. During the Caledonian orogeny, subductionrelated magmatism related to closure of the Iapetus ocean ended at 430 Ma [Corfu et al, 2006], marginal basin ophiolites and island arcs were emplaced onto the Baltica craton in the Wenlock [Andersen et al, 1990], and the previously hyperextended continental margin [Andersen et al, 2012] began to contract.…”
Section: Geologic Settingmentioning
confidence: 99%
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