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Detailed Reference Information |
Larson, S.M., Johnson, J.R. and Singer, R.B. (1991). Evaluation of the sensitivity of reflectance ratios to mafic minerals in the lunar regolith. Geophysical Research Letters 18: doi: 10.1029/91GL02620. issn: 0094-8276. |
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The 950/560 nm spectral ratio has been traditionally used as a qualitative indicator or lunar soil maturity because the 950 nm band falls within the major Fe2+ mineral absorption bands near 1 &mgr;m characteristic of relatively immature, crystalline surfaces. Since there are several other processes unrelated to maturation that may affect this ratio value, we have evaluated the 950/730 nm ratio as a potentially better measured of the relative 1-&mgr;m band strength. We find that the 950/730 nm ratio appears to be much more sensitive to the 1 &mgr;m band depth, but feel that other unknown variables preclude using these single ratios to provide meaningful quantitative results at this time. Because of problems with near-IR scattering in vidicon detectors used in previous studies, we have measured the scattering properties of our two CCDs and conclude that any scattering is negligible. ¿American Geophysical Union 1991 |
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Abstract |
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Keywords
Planetology, Comets and Small Bodies, Surfaces and interiors |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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