Surface tension and bubble nucleation in phonolite magmas
Surface tension and bubble nucleation in phonolite magmas
复制标题
声浪石岩浆中的表面张力和气泡成核
DOI:
10.1016/j.gca.2011.10.017
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发表时间:
2012
影响因子:
5
通讯作者:
J. Gardner
中科院分区:
文献类型:
--
作者:
J. Gardner
Explosive Plinian eruptions tap a wide range of magma compositions, including highly alkaline phonolite magma. Such eruptions are driven by volatiles exsolving from those magmas, and so determining how gas bubbles form is important to understanding those eruptions. Nucleation of bubbles in silicate melts is dictated strongly by the surface tension (σ) of the melt, and so this study focuses on determining σ for phonolite melts. Cylinders cored from a sodium-rich phonolite were hydrated with 5.37±0.09wt.% dissolved water at 150MPa and 1150°C, and then decompressed at either 1150°C or 875°C. Bubbles nucleated at 1150°C only when pressure dropped below 95MPa, in number densities of 104–5cm−3. At 875°C bubbles nucleated only when pressure dropped below 53MPa, in number densities of 104–7cm−3. Depending on whether the pressure within critical bubble nuclei equals the saturation pressure or a variable lower pressure, the observed number densities and nucleation rates imply that surface tension for Na-rich phonolite is 0.061 or 0.068Nm−1at 875°C and 0.052 or 0.066Nm−1at 1150°C. Importantly, temperature has little or slightly negative impact on σ, in contrast to the thermal impact on σ of rhyolite melts. Regardless of pressure assumption, the inferred surface tensions indicate that Na-rich phonolite can become highly super-saturated with water before bubbles nucleate, which could cause them to explosively degas and erupt, similar to highly viscous rhyolites.