Ringrose, Tim and Zarnecki, John
(2002).
![]()
|
PDF (Not Set)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (248kB) |
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 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) |
Item ID: | 8779 |
Depositing User: | Kyra Proctor |
Date Deposited: | 23 Jul 2007 |
Last Modified: | 19 Dec 2017 09:57 |
URI: | http://oro.open.ac.uk/id/eprint/8779 |
Share this page: | ![]() ![]() ![]() ![]() |
Download history for this item
These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.