Yoshida, S.; Tanaka, S.; Hagermann, A.; Hayakawa, M.; Fujimura, A. and Mizutani, H.
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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.
|Item Type:||Conference Item|
|Extra Information:||Abstract #1571|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Kyra Proctor|
|Date Deposited:||20 Jul 2007|
|Last Modified:||02 Aug 2016 15:46|
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