Ringrose, Tim and Zarnecki, John
(2002).
|
PDF (Not Set)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (242Kb) |
| URL: | http://www.lpi.usra.edu/meetings/lpsc2002/pdf/1183... |
|---|---|
| Google Scholar: | Look up in Google Scholar |
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 Item |
|---|---|
| Extra Information: | Abstract #1183 |
| Academic Unit/Department: | Science > Physical Sciences |
| 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: | 04 Dec 2010 05:59 |
| URI: | http://oro.open.ac.uk/id/eprint/8779 |
Actions (login may be required)
| View Item | |
| Public: Report issue / request change |




