The Open UniversitySkip to content

Martian and terrestrial dust devils

Ringrose, Tim and Zarnecki, John (2002). Martian and terrestrial dust devils. In: 33rd Lunar and Planetary Science Conference, 11-15 March 2002, Houston, Texas, USA.

Full text available as:
PDF (Not Set) - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (242Kb)
Google Scholar: Look up in Google Scholar


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
Share this page:

Actions (login may be required)

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340