No description available.

No description available.

Thesis (doctoral)--University of Turku.

In this thesis two studies of reactive metal adsorption upon a low index single crystal silicon dioxide surface are presented in addition to a study of sulphur adsorption upon a low index single crystal nickel surface. Chromium growth upon the a-quartz Si02(0001) (J84xJ84) Rll 0 surface is studied at three coverages, 0.25±O.08 ML, 0.5±O.16 ML and 1.0±0.33 ML, using surface extended x-ray absorption fine structure (SEXAFS). SEXAFS measurements, from the chromium K-edge, recorded at both grazing and normal incidence show that chromium growth proceeds via the formation of mesoscopic particles with a body centred cubic (b.c.c.) like structure having an average nearest neighbour Cr-Cr distance of 2.36±O.03 A. This represents a contraction of 5.6 % from the bulk b.c.c. lattice spacing of 2.49 A. There is no evidence of a surface reaction between chromium and the surface oxygen. SEXAFS was used to study titanium reactional growth on a-quartz (0001) (J84xJ84) Rll 0 and (lx1). Three nominal coverages were studied, 0.25±O.08 ML, 0.5±O.16 ML and 1.0±O.33 ML. Both normal and grazing incidence SEXAFS data were recorded and show the formation of a spatially extensive region in which an interfacial reaction has occurred between surface oxygen and adsorbate titanium atoms. Coupled with this is the formation of subnanometre titanium clusters. The metal oxide has nearest neighbour Ti-O distances close to those of both the anatase and rutile forms of titania with the metallic titanium clusters having a Ti-Ti distance within experimental error that of bulk hexagonal close packed (h.c.p.) titanium, 2.89 A. A re-examination of the surface geometry of Ni(1l0)c(2x2)S using SEXAFS has been performed. Data out to an electron wavevector of 9 A-I are analysed with a new code to assess the influence of multiple scattering. The first shell S-Ni distance is determined to be 2.20±O.02 A with the next nearest neighbour distance being 2.29±O.02 A, giving a top-layer Ni expansion of 14±3% relative to the bulk. The influence of multiple scattering does not significantly alter these values from earlier studies.

No description available.

This study employed a commercial code FLUENT to simulate a chemical vapor deposition process in a rectangular chamber for deposition of a silicon dioxide layer on a rectangular substrate. We focus on the deposition rate and heat transfer coefficient (Nu number) on the substrate surface. We discuss the effects of the size of inlet region, the distance from inlet to substrate, the size of outlet region, the Reynolds number, the temperature of substrate, the ratio of the inlet flow rates of the two reaction gases on the deposition rate. The results show that the four corners at the substrate has the lowest deposition rate no matter how the variables are changed. Near the four corners there exist a region with high deposition rate. The deposition rate is more uniform when inlet is larger or equal to the substrate, and when the distance between the inlet and the substrate is small. The larger the size of the outlet region, the larger the uniform deposition rate region present on the central part of the substrate. The deposition rate increases with increasing Re number. However the uniformity remains similarly. The deposition rate also increases with increasing the substrate temperature. A study of the inlet flow rate ratio of TEOS and indicates that TEOS flow rate governs the process. A proper flow rate ratio gives a better deposition rate.

Thesis (M.S.P.H.)--University of Michigan, 1942.

Thesis (M.S.P.H.)--University of Michigan, 1942.

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Hydrated amorphous silicon dioxide (Si02.nH-,O), or opal-A, is deposited naturally from seepage and runoff water as white or brown rock surface coatings, called 'skins', that often partly obscure rock paintings and engravings, but occasionally, a thin translucent silica skin can form a protective film over rock art. White lustrous silica skins, less than 1 mm thick, occur where seepage water regularly flows from bedding and joint planes, whereas much thinner brown skins form on the sides of boulders and cliffs where runoff water periodically flows. To find the degree of silica skin variability and to determine how climate and rock type affect the properties of silica skins I collected samples at seven Australian and two Canadian rock painting sites that were located in temperate, tropical and sub-arctic regions. The skins had developed on sandstone, quartzite, schist, gneiss and migmatite. I studied the effects of the skins on rock art stability, documented their compositions, textures and structures to establish their common properties, and searched for a way to date the silica which would provide an indication of the minimum age of the underlying art. 1 also made replication experiments to determine factors that influence the properties of artificial silica skins and the rates of their precipitation so that I could propose a mechanism for natural silica skin formation, and ascertain whether an artificial silica skin could act as a protective rock art conservation measure. I was able to subdivide the analysed samples into silica skin Types I, II and III on the basis of their colour (translucent, white or brown), composition (SiO2, Al2O3 and absorbed water contents) and texture (smooth vitreous or vermiform). I propose that silica skins initially begin to form on stable rock surfaces by a process involving a combination of evaporation- and ionic-induced polymerisation of silicic acid in seepage and runoff water. Condensation reactions, random clustering of small silica spheres and deposition of the resulting aggregates eventually produce a thin surficial silica film. Deposition of silica often traps micro-organisms that live in the damp seepage and runoff water zones, and these fossils in finely laminated skins enable the radiocarbon dating of silica deposition, and therefore the dating of rock paintings enclosed by silica. Micro-excavation of silica layers associated with rock art combined with accelerator mass spectrometry gave preliminary radiocarbon determinations that were either consistent with, or contradicted, prevailing opinions about the antiquity of the rock art at selected sites. Experiments using a laser technique for combusting fossilised microorganisms in finely laminated skins were unable to generate sufficient carbon for dating. Catalysis of a mixture of equal proportions of methyl-trimethoxy silane and water produces a translucent stable film that may be suitable as a consolidant, whereas other artificial silica skins made from silica glass and tetra-ethoxy silane develop microfractures on drying, and these are unsuitable as rock art consolidants.