2017
DOI: 10.1016/j.chemer.2017.02.001
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Geology, geochemistry and petrogenesis of post-collisional adakitic intrusions and related dikes in the Khoynarood area, NW Iran

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Cited by 10 publications
(7 citation statements)
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“…Strong enrichments in large‐ion lithophile elements (LILE) are obvious, such as Rb, Ba, Th, and U and depletion in compatible HFSE, such as Nb, Ta, and Ti. According to Mahmoudi Nia, Baghban, and Simmonds (2017), high Sr content and the negative anomalies of Ti, Ta, and Nb shows a lack of plagioclase fractionation and occurrence of Fe and Ti oxides throughout partial melting and crystal fractionation. Richards, Spell, Rameh, Razique, and Fletcher (2012) thought that depleted MREE‐HREE strongly propose REE fractionation controlled by hornblende leading to low Y and Yb (HREE) concentrations decreasing with increasing SiO 2 .…”
Section: Whole‐rock Geochemical Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Strong enrichments in large‐ion lithophile elements (LILE) are obvious, such as Rb, Ba, Th, and U and depletion in compatible HFSE, such as Nb, Ta, and Ti. According to Mahmoudi Nia, Baghban, and Simmonds (2017), high Sr content and the negative anomalies of Ti, Ta, and Nb shows a lack of plagioclase fractionation and occurrence of Fe and Ti oxides throughout partial melting and crystal fractionation. Richards, Spell, Rameh, Razique, and Fletcher (2012) thought that depleted MREE‐HREE strongly propose REE fractionation controlled by hornblende leading to low Y and Yb (HREE) concentrations decreasing with increasing SiO 2 .…”
Section: Whole‐rock Geochemical Resultsmentioning
confidence: 99%
“…Kay (1978) thought that adakitic rocks were related to convergent plate margin arcs through melting of oceanic crust. Mahmoudi Nia et al (2017) pointed out that in NW Iran, there are some adakitic rocks that are related to subduction of Neo‐Tethyan oceanic lithosphere.…”
Section: Discussionmentioning
confidence: 99%
“…Adakites form from partial melting of young oceanic crust in subduction zones (Defant and Drummond, 1990). They form from young and hot oceanic crust, retaining its F I G U R E 7 Plots of andesite host rocks of Sarcheshmeh PCD (Table 3) on Winchester and Floyd (1977) diagram Frost and Frost (2008) primary temperature, and are more readily melted (Defant and Drummond, 1990;Mahmoudi Nia et al, 2017). There are four types of adakites: (1) high silica adakites (HSA), (2) low silica adakites (LSA), (3) continental or potassic adakites, and (4) Archean adakites (Percival et al, 2003).…”
Section: The Origin Of Adakitic Volcanismmentioning
confidence: 99%
“…Cenozoic continental-collision-zone adakitic rocks occur mainly in the Tethyan tectonic domain across Eurasia in, for example, the Carpathian-Pannonian (e.g., Seghedi et al, 2004), Greece (e.g., Marchev et al, 2013), Turkey-Iran (e.g., Dokuz et al, 2013;Jahangiri, 2007;Moghadam et al, 2016;Nia et al, 2017;Omrani et al, 2008;Pang et al, 2016;Topuz et al, 2011), and Himalaya-Tibet (e.g., Chung et al, 2003Chung et al, , 2005Chung et al, , 2009Hou et al, 2004Hou et al, , 2012Wang et al, 2005Wang et al, , 2008bGao et al, 2007;Zeng et al, 2011;Jiang et al, 2014;Ma et al, 2014;Zhang et al, 2014;Long et al, 2015;Liu et al, 2017;Ou et al, 2017) regions. They comprise mainly granites-(granodiorite porphyries)-dacites-rhyolites with ages of 56-2.5 Ma and SiO 2 contents (57.0-77.0 wt.%) similar to those of Cenozoic arc adakitic rocks, but with higher total-alkali (3.5-13.0 wt.%), Figure 4b), consistent with multiple crustal components in their sources, such as thickened ancient lower crust and subducted continental crust.…”
Section: Cenozoic Adakitic Rocks In Continental Collision Zonesmentioning
confidence: 99%