Refinement of lunar TiO2 analysis with multispectral features of Chang’E-1 IIM data
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s10509-012-1232-1.pdf
Reference27 articles.
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2. Charette, M.P., Mocord, T.B., Pieters, C.M., et al.: Application of remote spectral reflectance measurements to lunar geology classification and determination of titanium contents of lunar soils. J. Geophys. Res. 79(11), 1605–1613 (1974)
3. Giguere, T.A., Taylor, G.J., Hawke, B.R., et al.: The titanium contents of lunar mare basalts. Meteorit. Planet. Sci. 35(1), 193–200 (2000)
4. Gillis-Davis, J.J., Lucey, P.G., Hawke, B.R.: Testing the relation between UV-VIS color and TiO2 content of the lunar maria. Geochim. Cosmochim. Acta 70(24), 6079–6102 (2006)
5. Gillis, J.J., Jolliff, B.L., Elphic, R.C.: A revised algorithm for calculating TiO2 from Clementine UV/VIS data: a synthesis of rock, soil, and remotely sensed TiO2 concentrations. J. Geophys. Res. 108(E2), 1063–1078 (2003)
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