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Selenology Today # 7 July 2007 - Home

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GEOLOGIC LUNAR RESEARCH SELENOLOGY TODAY # 7<br />

on the surface of the moon. COSPAR Workshop: The moon recent<br />

results: science, future robotic and human exploration workshop. abstract<br />

#154.<br />

15. Gillis JJ and Lucey PG. 2005. Evidence that UVVIS ratio is not a simple<br />

linear function of TiO2 content for lunar mare basalts. Lunar and<br />

Planetary Science XXXVI abstract #2252.<br />

16. Holsclaw GM et al. 2005. Comparison of newly acquired lunar spectra<br />

with the titanium abundance maps derived from Clementine. Lunar and<br />

Planetary Science XXXVI abstract #2376.<br />

17. Pieters CM (1978). Mare basalt types on the front side of the moon. A<br />

survey of spectral reflectance data. Proc. Lunar and Planetary Science<br />

Conf. IX, p. 2825-49.<br />

18. Singer RB and Geissler PE. 1988. An independent Assessment of<br />

Derivative Analysis of Reflectance Spectra. Lunar and Planetary Science<br />

Conference Vol. 19, p. 1087.<br />

19. Evans RJ. 2006. Exploring false color and ratio images using Clementine<br />

UVVIS/NIR data. <strong>Selenology</strong> <strong>Today</strong>. Volume 3, pp. 38-64.<br />

20. Pieters, CM (1999). The moon as a spectral calibration standard enabled<br />

by lunar samples: the Clementine Example. Workshop on new views of<br />

the moon: understanding the moon through the integration of diverse<br />

datasets p.47.<br />

21. Robinson MS, McEwen AS, Eliason E et al. (1999) Clementine UVVIS<br />

global mosaic: a new tool for understanding the lunar crust. Lunar and<br />

Planetary Science Conference XXX, abstract #1931.<br />

22. Hillier JK, Buratti BJ, and Hill K. (1999) Multispectral photometry of the<br />

moon and absolute calibration of the Clementine UVVIS camera. Icarus<br />

vol. 141, issue Icarus pp. 205-225.<br />

23. Opanasenko NV, Shkuratov YG, Kreslavsky MA et al. (1999) A<br />

comparison of Clementine and Earth based observations of the moon.<br />

Lunar and Planetary Science Conference XXX, abstract #1130.<br />

page 25

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