Refinement of a lunar FeO mapping method

Author:

Liu Jian,Ouyang Ziyuan,Li Chunlai,Zou Yongliao

Publisher

Springer Science and Business Media LLC

Subject

Geochemistry and Petrology

Reference37 articles.

1. Adams J.B. (1974) Visible and near-infrared diffuse reflectrance spectra of pyroxenes as applies to remote sensing of solid bodies in the solar system [J]. J. Geophys. Res. 79, 4829.

2. Blewett D.T., Lucey P.G., Hawke B.R., and Jolliff B.L. (1997) Clementine images of the lunar sample-return stations: Refinement of FeO and TiO2 mapping techniques [J]. J. Geophys. Res. 102, 16319–16325.

3. Burns R.G. (1993) Origin of electronic spectra of minerals in the visible to near-infrared region. In Remote Geochemical Analysis [M]. pp.3–29. Cambridge University Press, New York.

4. Cahill J.T. et al. (2004) Verification of quality and compatibility for the newly calibrated Clementine NIR Data Set. In Lunar and Planet. Sci. Conf. [C]. XXXV, 1469.

5. Charette M.P. and Adams J.B. (1977) Spectral reflectance of lunar highland rocks. In Proc. Luar Sci. Conf. 8 th [C]. 172.

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