Monte Carlo Modeling of the Thermal Cond
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Yossi Shoshany; Dina Prialnik; Morris Podolak
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Article
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2002
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Elsevier Science
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English
⚖ 236 KB
The basic structure of comet nuclei is an aggregation of grains, with a size distribution that extends over several orders of magnitude and a similar distribution of pores. Although attempts have been made to assess the effect of porosity on the thermal conductivity, the effect of pore size distribu