2018
DOI: 10.1016/j.epsl.2018.07.032
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Conditions of pinnacle formation and glass hydration in cooling ignimbrite sheets from H and O isotope systematics at Crater Lake and the Valley of Ten Thousand Smokes

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Cited by 25 publications
(12 citation statements)
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“…Meteoric waters infiltrate and modify the composition of volcanic glass following eruptive emplacement on timescales of <10–10 4 years (Cassel & Breeker, 2017; Giachetti et al., 2020; Nolan & Bindeman, 2013; Seligman et al., 2018). The meteoric water modifies the primary magmatic hydrogen isotope composition initially preserved in volcanic glass because meteoric waters are enriched in D relative to H, with the ratio controlled by precipitation, temperature, latitude, and altitude (e.g., Cassel et al., 2009; Giachetti et al., 2020, 2015; Hudak & Bindeman, 2018; Ingraham & Taylor, 1991; Jackson et al., 2019; Seligman et al., 2016). Meteoric water and groundwater in the vicinity of Long Valley have δ D in the range of −90‰ to −110‰, values enriched in H relative to D as expected on the rain shadowed, high‐altitude eastern flank of the Sierra Nevada (Friedman et al., 2002; Ingraham & Taylor, 1991).…”
Section: Discussionmentioning
confidence: 99%
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“…Meteoric waters infiltrate and modify the composition of volcanic glass following eruptive emplacement on timescales of <10–10 4 years (Cassel & Breeker, 2017; Giachetti et al., 2020; Nolan & Bindeman, 2013; Seligman et al., 2018). The meteoric water modifies the primary magmatic hydrogen isotope composition initially preserved in volcanic glass because meteoric waters are enriched in D relative to H, with the ratio controlled by precipitation, temperature, latitude, and altitude (e.g., Cassel et al., 2009; Giachetti et al., 2020, 2015; Hudak & Bindeman, 2018; Ingraham & Taylor, 1991; Jackson et al., 2019; Seligman et al., 2016). Meteoric water and groundwater in the vicinity of Long Valley have δ D in the range of −90‰ to −110‰, values enriched in H relative to D as expected on the rain shadowed, high‐altitude eastern flank of the Sierra Nevada (Friedman et al., 2002; Ingraham & Taylor, 1991).…”
Section: Discussionmentioning
confidence: 99%
“…Meteoric waters infiltrate and modify the composition of volcanic glass following eruptive emplacement on timescales of <10-10 4 years (Cassel & Breeker, 2017;Giachetti et al, 2020;Nolan & Bindeman, 2013;Seligman et al, 2018). The meteoric water modifies the primary magmatic hydrogen isotope composition initially preserved in volcanic glass because meteoric waters are enriched in D relative to H, with the ratio controlled by precipitation, temperature, latitude, and altitude (e.g., Cassel et al, 2009;Giachetti et al, 2020Giachetti et al, , 2015Hudak & Bindeman, 2018;Ingraham & Taylor, 1991;Jackson et al, 2019;Seligman et al, 2016). Meteoric water and groundwater in the vicinity of Long Valley have δD in the range of −90‰ to −110‰, Newman et al (1988); gray triangles are Mono Craters from J. D. Barnes et al (2014a); gray squares are Mono-Inyo Craters from Taylor et al (1983); gray diamonds are Medicine Lake from Taylor et al (1983); white diamonds are Medicine Lake from Giachetti et al (2020); white circles and triangles are Chaitén and Cordón Caulle, respectively, from Castro et al (2014); and white squares are Mazama from Mandeville et al (2009).…”
Section: Meteoric Rehydrationmentioning
confidence: 99%
“…The H 2 O contents in both the Karymshina samples and those from other volcanoes are similar and appropriate for fresh amphiboles and biotites, suggesting that this depletion is not due to chlorite alteration (a mineral with 12 wt% H 2 O which easily exchanges with surface water). The large range of δD values, especially in biotites, likely reflects incipient exchange of D and H after intracaldera ignimbrite emplacement into the shallow crust with meteoric waters, and could also be due to post-eruption alteration of the cooling ignimbrite deposits (e.g., Hudak and Bindeman, 2008;Seligman et al, 2018). It is also possible that some of the low δD values are attributable to hydrothermal alteration of the magma source rock prior to genesis and eruption of the 1.78 Ma magma, and reflect lower-δD subglacial meteoric water values as glaciation in the northern hemisphere started at 2-2.6 Ma.…”
Section: Hydrogen Isotopes Of Amphiboles and Biotitesmentioning
confidence: 99%
“…On the experimental side researchers have developed oxygen isotopic proxies for carbonate in paleosols (Quade et al, 2007) and paleolake sediments (Davis et al, 2009), fossil teeth (Kohn et al, 2002), clay minerals (Chamberlain et al, 1999), and chert (Ibarra et al, 2021). For hydrogen isotopes we have the additional proxies such as hydrated volcanic glasses (Mulch et al, 2008;Cassel et al, 2009;Hudak and Bindeman, 2018), clay minerals (Capuano, 1992;Delgado and Reyes, 1996;Mulch et al, 2006), plant leaf waxes (Hren et al, 2010) and metamorphic micas (Mulch et al, 2004).…”
Section: Introductionmentioning
confidence: 99%