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Patel, N.; Hagermann, A.; Lewis, S. R.; Kaufmann, E. and Balme, M.
(2018).
URL: https://meetingorganizer.copernicus.org/EPSC2018/E...
Abstract
We have modelled the transport of heat in the martian regolith, taking into account the change in thermal properties caused by an increase in water ice content. Under these conditions we have found that the addition of water ice allows for increased ice formation at depth, rather than under the assumption that thermal properties are unchanged. This is important because it will affect estimates of global subsurface volatile deposition.
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- Item ORO ID
- 58676
- Item Type
- Conference or Workshop Item
- ISSN
- 0019-1035
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
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- Copyright Holders
- © 2018 The Authors
- Depositing User
- Narissa Patel