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Lewis, S. R.; Hinson, D. P. and Spiga, A.
(2011).
URL: http://meetingorganizer.copernicus.org/EPSC-DPS201...
Abstract
Radio science observations indicate that the depth of the martian convective boundary layer varies strongly with surface height, although the surface temperature does not. We show that this effect is reproduced in martian limited area models and in global climate models. The implications for the global circulation when convective boundary layer depth varies with location are considered.
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- Item ORO ID
- 29616
- Item Type
- Conference or Workshop Item
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- ?? space ??
- Copyright Holders
- © 2011 The Authors
- Depositing User
- Stephen Lewis