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NASA NTRS · 19810003044

Efficient solar cells by space processing

Abstract

Thin films of electron beam evaporated silicon were deposited on molybdenum, tantalum, tungsten and molybdenum disilicide under ultrahigh vacuum conditions. Mass spectra from a quadrapole residual gas analyzer were used to determine the partial pressure of 13 residual gases during each processing step. Surface contamination and interdiffusion were monitored by in situ Auger electron spectrometry. The presence of phosphorus in the silicon was responsible for attaining elevated temperatures with silicide formations. Heteroepitaxial silicon growth was sensitive to the presence of oxygen during deposition, the rate and length of deposition as well as the substrate orientation.

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BibTeXRIS

Schmidt, F. A., Campisi, G. J., Bevolo, A., Shanks, H. R., Williams, D. E.. 1979-01-01. Efficient solar cells by space processing. https://ntrs.nasa.gov/citations/19810003044

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