Ringrose, Tim and Zarnecki, John
(2002).
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| URL: | http://www.lpi.usra.edu/meetings/lpsc2002/pdf/1183... |
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Abstract
When dust devils or convective vortices form they can be identified by specific meteorological parameters, a ‘signature’. If martian and terrestrial dust devil signatures are compared similarities can be identified.
| Item Type: | Conference or Workshop Item |
|---|---|
| Extra Information: | Abstract #1183 |
| Academic Unit/School: | 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) |
| Item ID: | 8779 |
| Depositing User: | Kyra Proctor |
| Date Deposited: | 23 Jul 2007 |
| Last Modified: | 06 Oct 2016 10:58 |
| URI: | http://oro.open.ac.uk/id/eprint/8779 |
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