P4_8 Plasma Windows

The physics behind plasma windows are explored and it is investigated whether they would be applicable on a large scale as a divider between a vacuum and a pressurised hangar. It is found that while possible, it may be difficult due to the large energy need to ionise the plasma and the large scale nature of the magnetic field

P4_11 Solar Wind

The physics behind the solar wind is investigated in order to determine whether it is possible to have a star whose solar pressure could be held back by the local interstellar medium, thus placing it in hydrostatic equilibrium with no solar wind. It is found using a simplified model that such a star probably cannot exist

A Comparison of Oxygen Fugacities of Strongly Peraluminous Granites across the Archean–Proterozoic Boundary

We constrain the oxygen fugacity (⁠f_(O2)⁠) of strongly peraluminous granites [SPGs; i.e. granites (sensu lato) generated through the partial melting of sediments] across the Archean–Proterozoic boundary, which coincides roughly with the Great Oxygenation Event (GOE), to understand whether secular changes in atmospheric O_2 levels may be imprinted on the f_(O2) of igneous rocks. SPGs were chosen to maximize the potential effects of sediments in their sources on the f_(O2) of the magmas. We studied 28 Archean (2685–2547 Ma) and 31 Meso- to Paleoproterozoic (1885–1420 Ma) geographically distributed samples from North America, spanning two cratons (Superior and Wyoming) and both orogenic and anorogenic Proterozoic provinces (Trans-Hudson Orogen, Wopmay Orogen, and SW USA). We present an analysis of both new and previously published whole-rock major and trace element data and mineral major element chemistry from the samples. All the studied samples are peraluminous high-silica plutonic rocks (all contain >67 wt % SiO_2, and 92% are true granites with >69 wt % SiO_2), and biotite + muscovite ± garnet ± tourmaline ± sillimanite are the primary aluminous minerals in all samples. Whole-rock major element and trace element abundances of all samples are consistent with derivation by partial melting of aluminous sediments. To constrain the f_(O2) of crystallization of the SPGs, we developed an alphaMELTS-based method that takes advantage of the sensitivity of biotite Fe^T/(Fe^T + Mg) ratios to f_(O2)⁠. This method is able to reproduce experimental and empirical data where biotite compositions and whole-rock compositions, pressures and temperatures of crystallization and f_(O2) are known. For the SPGs in this study, alphaMELTS modeling indicates that 68% of Proterozoic samples crystallized at an f_(O2) between NNO –1 and NNO +1·1 (where NNO is nickel–nickel oxide buffer), whereas the remaining Proterozoic samples (32%) and most of the Archean samples (75%) crystallized at ≤NNO –2. The simplest explanation of these results is that the Proterozoic SPGs were derived from metasedimentary source rocks that on average had more oxidized bulk redox states relative to their Archean counterparts. The bulk redox state of the metasedimentary source rocks of SPGs of all ages is defined by the relative abundances of oxidized (e.g. Fe^(3+) and S^(6+)) and reduced (e.g. organic matter) material. The crystallization of both Archean and Proterozoic samples at f_(O2) values of ≤NNO –2 is consistent with them having their f_(O2) buffered by graphite (formed from organic carbon) in their source regions. However, the dominantly low f_(O2) (≤NNO –2) values of the Archean SPGs plausibly reflects the presence of organic material and relatively reduced metasedimentary rocks in their source region prior to the GOE. In contrast, the elevated f_(O2) values of the majority of the Proterozoic SPGs may reflect enhanced sulfate contents or increased Fe^(3+)/Fe^T in sediments after the GOE, which, in terms of the bulk redox state of their metasedimentary source region, would have offset the reducing nature of organic matter present there

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Thesis (Ed.M.)--Boston Universit