2005
DOI: 10.2113/gscanmin.43.4.1331
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Variation in Mineralogy, Temperature, and Oxygen Fugacity in a Suite of Strongly Peralkaline Lavas and Tuffs, Pantelleria, Italy

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Cited by 66 publications
(89 citation statements)
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“…This is in accord with the general situation in peralkaline rhyolites; hedenbergite is the normal pyroxene phenocryst even in the most strongly peralkaline rocks, aegirine-augite being recorded only rarely (Macdonald et al 2011). This is probably related to the relatively low fO 2 at which the magmas evolve, at or close to FMQ (Scaillet and Macdonald 2001White et al 2005White et al , 2009Ren et al 2006;Di Carlo et al 2010). A microphenocryst in B355 has a relatively magnesian core (Ca 44.9 Mg 21.1 Fe 34.0 ), which may represent a highertemperature phase of magmatic evolution or mixing of the pantellerite with a more trachytic magma.…”
Section: Olivinesupporting
confidence: 86%
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“…This is in accord with the general situation in peralkaline rhyolites; hedenbergite is the normal pyroxene phenocryst even in the most strongly peralkaline rocks, aegirine-augite being recorded only rarely (Macdonald et al 2011). This is probably related to the relatively low fO 2 at which the magmas evolve, at or close to FMQ (Scaillet and Macdonald 2001White et al 2005White et al , 2009Ren et al 2006;Di Carlo et al 2010). A microphenocryst in B355 has a relatively magnesian core (Ca 44.9 Mg 21.1 Fe 34.0 ), which may represent a highertemperature phase of magmatic evolution or mixing of the pantellerite with a more trachytic magma.…”
Section: Olivinesupporting
confidence: 86%
“…Semi-quantitative analyses indicate, however, that it is pyrrhotite, which has also been recorded as microphenocrysts in peralkaline rhyolites from Tejeda volcano, Gran Canaria (Crisp and Spera 1987), Pantelleria (Lowenstern et al 1993;White et al 2005) and Eburru, Kenya (Ren et al 2006).…”
Section: Sulphidementioning
confidence: 99%
“…Mattia et al, 2007). The range of temperature investigated (680^8008C) encompasses that inferred by White et al (2005) for the felsic end-members, but also reflects the conditions required to match the crystal-poor condition characterizing most Pantelleria rhyolites, including the selected starting material, and the variation of this parameter with H 2 O melt .The starting material (PAN 01113) belongs to the Fastuca pumice fall eruptive unit (Orsi et al, 1989) and was sampled from the bottom portion of the deposit, which consists of dense, variably welded, pumice that has locally agglutinated to produce vitrophyric bands. Welding and agglutination to form thin, lava-like layers is common at Pantelleria in pumice-fall deposits located close to the vents (Rotolo et al, 2007).…”
mentioning
confidence: 79%
“…They did not consider the physical conditions under which magmatic differentiation occurs, such as the temperature of crystal^melt equilibration, or the melt viscosity and density, which heavily depend on temperature and volatile contents. This gap has been partly filled with the detailed petrological studies of White et al (2005White et al ( , 2009, who used thermobarometric tools (e.g. QUILF) and the MELTS solution model to work out the intensive parameters for the Pantelleria magmatic suite.…”
Section: Geological and Petrological Backgroundmentioning
confidence: 99%
“…The crystallization of Na-rich clinopyroxene (i.e., aegirine-augite and aegirine) and other Na-bearing phases, such as arfvedsonite, contribute efficaciously to the formation of peralkaline magmas (White et al 2005). The stability and composition of clinopyroxene and arfvedsonite are temperature-, H 2 O activity-, melt composition-and fO 2 -dependent (Scaillet and Macdonald 2001).…”
Section: Inferences Concerning Conditions Of Crystallizationmentioning
confidence: 99%