Physics
Scientific paper
Mar 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..119b&link_type=abstract
Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 119.
Physics
2
Lunar Probes, Clementine Spacecraft, Satellite Imagery, Lunar Maps, Titanium Oxides, Lunar Soil, Lunar Surface, Return To Earth Space Flight, Spectral Reflectance, Ultraviolet Spectroscopy, Apollo 16 Flight
Scientific paper
The present method for determining the TiO2 content of the lunar surface via extended-visible reflectance spectrometry attempts to develop a calibration for the full resolution UVVIS images of Clementine, on the basis of images of the lunar sample-return sites. The images were converted to 'absolute' reflectance by dividing by the spectrum of the Apollo 16 telescopic site extracted from the Clementine images, then multiplying by the laboratory spectrum of Apollo 16 soil 62231.
Blewett Dave T.
Hawke Bernard Ray
Jolliff Brad L.
Lucey Paul G.
No associations
LandOfFree
Clementine images of the lunar sample-return stations - Improvements to the TiO2 mapping technique does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Clementine images of the lunar sample-return stations - Improvements to the TiO2 mapping technique, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clementine images of the lunar sample-return stations - Improvements to the TiO2 mapping technique will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-871314