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Toward Quantification of Ti-Oxidation States in Planetary Materials via Application of the EELS White-Line Ratio Technique

  • Lindsay R. Slick (a1), Prajkta Mane (a1), Jane Howe (a1) (a2) and Thomas Zega (a1) (a3)
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References

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[1] Garvie, L.A.J, Crvaven, A.J. Brydson, R Amer. Mineralogist 79 1994) p 411425.
[2] Beckett, J.R., et al, Geochem. Cosmochem. Acta 52 1988) p 14791495.
[3] Connelly, J.N., et al, Science 338 2012) p 651655.
[4] Stoyanov, E., Langenhorst, F. Steinle-Neimann, G. Amer. Mineralogist 92 2007) p 557586.
[5] Zega, T.J., Garvie, L.A.J. Buseck, P.R. Amer.Minerologist 88 2003) p 11691172.
[6] Van Aken, P.A. Liebscher, B. Phys Chem Minerals 29 2002) p 188200.
[7] Wu, Z., et al, J. Synchrotron Rad 8 2001) p 934936.
[8] Brydson, R., et al, J. Phys.: Condens. Matter 1 1989) p 797812.
[9] We gratefully acknowledge NASA (grants #NNX12AL47G and #NNX15AJ22G) and NSF (grants #1531243 and #0619599) for funding of instrumentation in the Kuiper Materials Imaging and Characterization Facility at the Lunar and Planetary Laboratory, University of Arizona.

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