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Lunar Reconnaissance Orbiter (LRO) Observations with the Lunar Exploration Neutron Detector (LEND): Neutron Suppression Regions (NSR) and Polar Hydrogen

Authors :
Chin, G
Mitrofanov, I. G
Boynton, W. V
Golovin, D. V
Evans, L. G
Harshman, K
Kozyrev, A. S
Litvak, M. L
McClanahan, T
Milikh, G. M
Sagdeev, R
Sanin, A. B
Shevchenko, V
Shvetsov, V
Smith, D
Starr, R
Trombka, J
Zuber, M
Publication Year :
2011
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2011.

Abstract

Orbital detection of neutrons has become the dominant remote sensing technique for detecting and inferring H concentrations and its spatial distribution beneath planetary surfaces [Lawrence et al, (2010) Icarus, 205, pp. 195-209, Mitrofanov et al (2007) Science 297(5578), 78-81]. Indications for the presence of localized and relatively high water content was provided by LRO and LCROSS. LEND identified Cabeus, as the most promising LCROSS impact site [Mitrofanov I. et al. (2010) Science, 330, 483], and instruments onboard LRO and LCROSS have measured signatures of water, H2 and other volatiles in the impact plume [Colaprete A. et al. (2010) Science, 339,463, Gladstone R. et al. (2010) Science, 330, 472].

Details

Language :
English
Database :
NASA Technical Reports
Publication Type :
Report
Accession number :
edsnas.20110013457
Document Type :
Report