Hagermann, A.; Tanaka, S.; Yoshida, S.; Hayakawa, M.; Fujimura, A. and Mizutani, H.
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For determining the lunar heat flow two parameters need to be measured: The thermal gradient and the thermal conductivity of the regolith. Methods for inferring these quantities from in situ measurements using the LUNAR-A penetrators will be presented.
|Item Type:||Conference Item|
|Extra Information:||Abstract #1497|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Kyra Proctor|
|Date Deposited:||20 Jul 2007|
|Last Modified:||24 Feb 2016 10:00|
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