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Yoshida, S.; Tanaka, S.; Hagermann, A.; Hayakawa, M.; Fujimura, A. and Mizutani, H.
(2001).
URL: http://www.lpi.usra.edu/meetings/lpsc2001/pdf/1571...
Abstract
The relationship between the Th abundance and the heat flow data of the Apollo sites and the LUANR-A sites, where the Th concentrations are in the wide range from 1 ppm to 6 ppm, will allow for a more precise estimation of the averaged heat flow value.