Michelle McCann
Australian National University
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Publication
Featured researches published by Michelle McCann.
Solar Energy Materials and Solar Cells | 2001
Kylie R. Catchpole; Michelle McCann; Klaus Weber; Andrew Blakers
Approximately half the cost of a finished crystalline silicon solar module is due to the silicon itself. Combining this fact with a high-efficiency potential makes thin-film crystalline silicon solar cells a growing research area. This paper, written in two parts, aims to outline world-wide research on this topic. The subject has been divided into techniques which use native substrates and techniques which use foreign substrates. Light trapping, vapour- and liquid-phase deposition techniques, cell fabrication and some general considerations are also discussed with reference to thin-film cells.
Solar Energy | 1999
Keith Lovegrove; Andreas Luzzi; Michelle McCann; Oliver Freitag
The reversible dissociation of ammonia is one of the candidate reactions for use in closed loop solar thermochemical energy storage systems. The major determinant of achievable performance for such a system is the degree of thermodynamic irreversibility associated with the heat recovery process. Exergy analysis of a semi realistic 30 MPa isobaric system has revealed that the major irreversibilities occur within the exothermic reactor and the counterflow heat exchanger between ingoing and outgoing reactants. In this study, optimum reactor control yielded exergetic efficiencies up to 71%, which should translate to overall solar to electric conversion efficiencies of around 20%.
Journal of Crystal Growth | 2002
Michelle McCann; Klaus Weber; Mladen Petravic; Andrew Blakers
This paper presents the results of a study of the incorporation of boron into silicon layers grown from a tin melt by liquid phase epitaxy. Boron was added to the melt through the use of boron-doped silicon source wafers. There is a large discrepancy between the amount of boron incorporated into the epitaxial layer and that available in the source wafer. This mismatch is explained by the gradual removal of boron from our system, most likely as a result of boron precipitation in the tin melt. This situation allows for control of the boron profile by adjusting the cooling rate and adding a dwell time. In this way, we have grown an epitaxial layer with an abrupt and highly doped p-type region at the epitaxial layer/substrate interface. This is useful for thin film solar cell applications as it allows the growth of a back surface field and a lightly doped bulk in a single growth step.
Progress in Photovoltaics | 2005
Michelle McCann; Klaus Weber; Andrew Blakers
Solar Energy Materials and Solar Cells | 2004
D. Buie; Michelle McCann; Klaus Weber; Christopher Dey
Archive | 2002
Klaus Weber; Matthew Stocks; Andrew Blakers; Michelle McCann
Archive | 2001
Michelle McCann; Klaus Weber; Matthew Stocks; Andrew Blakers
Proceedings of the 16th European Photovoltaic Solar Energy Conference | 2000
Michelle McCann; Klaus Weber; Matthew Stocks; Kylie R. Catchpole; Andrew Blakers
ISES 2001 Solar World Congress: Proceedings | 2003
Michelle McCann; Klaus Weber; Andrew Blakers
Proceedings of the 16th European Photovoltaic Solar Energy Conference | 2000
Kylie R. Catchpole; Michelle McCann; Klaus Weber; Andrew Blakers