[1] Neal C R. The Moon 35 years after Apollo: What’s left to learn[J]. Chemie der Erde Geochemistry,2009,69(1):343.
[3] Liu F J, Qiao L, Liu Z, et al. Estimation of lunar titanium content: Based on absorption features of Chang’E-1 interference imaging spectrometer (IIM)[J]. Science China Physics: Mechanics and Astronomy,2010,53(12):21362144.
[4] Wu Y Z, Zhang X, Yan B K, et al. Global absorption center map of the mafic minerals on the Moon as viewed by CE-1 IIM data[J]. Science China Physics: Mechanics and Astronomy,2010,53(12):21602171.
[9] Mouelic S L, Langevin Y. The olivine at the lunar crater Copernicus as seen by Clementine NIR data[J]. Planetary and Space Science,2001,49(1):6570.
[10] Wu Y Z, Xu X S, Xie Z D, et al. Absolute calibration of the Chang’E-1 IIM camera and its preliminary application[J]. Science in China Series G: Physics, Mechanics and Astronomy,2010,52(12):18421848.
[11] Gao B C. An operational method for estimating signal to noise ratios from data acquired with imaging spectrometers[J]. Remote Sensing of Environment,1993,43(1):2333.
[12] Roger R E, Arnold J F. Reliably estimating the noise in AVIRIS hyperspectral images[J]. International Journal of Remote Sensing,1996,17(10):19511962.
[13] Gao L R, Zhang B, Wen J T, et al. Residual-scaled local standard deviations method for estimating noise in hyperspectral images[J]. Multispectral Image Processing,2007,6787:7871378713.
[14] Shannon C E. A mathematical theory of communication[J]. Bell System Technical Journal 1948,27(3):379423.
[15] Lucey P G. Mineral maps of the Moon[J]. Geophysical Research Letters,2004,31(8),doi:10.1029/2003GL019406