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    Flowage differentiation in an andesitic dyke of the Motru Dyke Swarm (Southern Carpathians, Romania) inferred from AMS, CSD and geochemistry
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    A study of amphiboles and associated minerals in samples of Soufrière Hills andesite erupted from 1995 to 2002 shows significant compositional variations within hornblende phenocrysts, a separate set of small pargasitic crystals in the groundmass, and two types of reaction rims on the phenocrysts. The composition of the amphiboles and coexisting phases defines the thermal history of the erupting magma. As many as seven zones (<200 µm wide) in the hornblende phenocrysts begin with a sharp increase in Mg and Si, and then change gradually to a more Fe- and Al-rich hornblende, a transition that is consistent with a temperature rise. Analyses of the hornblende phenocrysts and associated Fe–Ti oxides verify previous conclusions that the pre-eruption magma was at 130 MPa and 830 ± 10°C, but was variably heated before eruption. The heating occurred within ∼30 days of eruption for all magmas erupted, based on the width of Ti-rich rims on titanomagnetite phenocrysts. Experimental phase equilibria for the andesite confirm that the natural hornblende phenocrysts would be stable between 825 and 855°C at a PH2O of 130 MPa, and would be even more Al rich if crystallized at higher pressure. Pargasite is not stable in the andesite, and its presence, along with high-An plagioclase microphenocrysts, requires mafic magma mingling and hybridization with pre-existing andesite. Experimental melts of the andesite at 130 MPa and 830 and 860°C compare well with melt inclusions in quartz and plagioclase, respectively. Reaction rims on a few hornblende crystals in each andesite sample are rich in high-Ca pyroxene and are produced experimentally by heating the andesite above the stability limit for hornblende. Decompression-induced breakdown rims occur in some samples, and the rate of this reaction has been experimentally calibrated for isothermal andesite magma ascent at 830–860°C. The average ascent rate of magma during much of the 1995–2002 eruption has been >0·02 m/s, the rate that allows hornblende to erupt free of decompression-induced reaction rims.
    Phenocryst
    Hornblende
    Amphibole
    Igneous differentiation
    Citations (265)
    In this contribution the crystal size distribution (CSD) of amphibole and plagioclase from the Zanbil adakitic dacites of Iran were measured for a series of 20 samples spanning most of the exposed dome.Growth histories, residence time and textural features were studied at the rocks.All amphiboles and plagioclases show non-linear concave up CSD trends, forming a population density with two distinct parts.It can be modeled by mixing two crystal populations, here named fine grains, with intercept values of approximately 12 cm -4 for amphiboles and 7 cm -4 for plagioclase and phenocrysts, with intercept values of 8 cm -4 for amphibole and 4 cm -4 for plagioclase, each with overlapping linear CSDs.The plagioclase CSDs characterized with an individual flat part as a result of textural coarsening.The latest data show that plagioclase nucleation sites are lower than amphiboles, but growth was noticeable.The magmas bearing the fine grains and phenocrysts started to crystallize at 15-20 and 30-38 years, respectively, before each eruption, assuming a growth rate of 10 -10 cm/s.Phenocrysts crystallized during longer residence times.Subsequently, new magma containing few or no crystals was introduced and the fine grains crystallized from the mixed magma.Eruption followed 15-20 years after mixing.Such a model suggests that some porphyritic volcanic rocks erupted from shallow magma chambers that were never fully emptied.
    Amphibole
    Igneous differentiation
    Citations (3)
    The geologic and petrologic study of the Kattadake pyroclastics (around 10 ka) from the Zao volcano (NE Japan) revealed the structure of the magma plumbing system and the mixing behavior of the shallow chamber. The Kattadake pyroclastic succession is divided into lower and upper parts by a remarkable discontinuity. All rocks belong to medium-K, calc-alkaline rock series and correspond to ol-cpx-opx basaltic-andesite to andesite with 20–28 vol% phenocrystic modal percentage. All rocks were formed by mixing between andesitic magma and near aphyric basalt. The petrologic features of andesites of lower and upper parts are similar, 59–61 wt% SiO2, having low-An plagioclase and low-Mg pyroxenes, with pre-eruptive conditions corresponding to 960–980 °C, 1.9–3.5 kb, and 1.9–3.4 wt% H2O. However, the basalts were ca. 49.4 wt% SiO2 with Fo~84 olivine in the lower part and 51.8 wt% SiO2 with Fo~81 olivine and high-An plagioclase the in upper one. The percentage of basaltic magma in the mixing process was lower, but the temperature of the basalt was higher in the lower part than the upper one. This means that the shallow magma chamber was reactivated more efficiently by the hotter basalts and that the mixed magma with a 70–80% of melt fraction was formed by a smaller percentage of the basaltic magma.
    Andesites
    Basaltic andesite
    Magma chamber
    Igneous differentiation
    Citations (2)