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Martian and terrestrial dust devils

By Tim Ringrose and John Zarnecki

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

Year: 2002
OAI identifier: oai:oro.open.ac.uk:8779
Provided by: Open Research Online

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