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dc.contributor.authorMetzger, S.
dc.contributor.authorBalme, M.
dc.contributor.authorTowner, Martin
dc.contributor.authorBos, B.
dc.contributor.authorRingrose, T.
dc.contributor.authorPatel, M.
dc.date.accessioned2017-01-30T14:47:06Z
dc.date.available2017-01-30T14:47:06Z
dc.date.created2015-03-03T20:16:24Z
dc.date.issued2011
dc.identifier.citationMetzger, S. and Balme, M. and Towner, M. and Bos, B. and Ringrose, T. and Patel, M. 2011. In situ measurements of particle load and transport in dust devils. Icarus. 214 (2): pp. 766-772.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/40945
dc.identifier.doi10.1016/j.icarus.2011.03.013
dc.description.abstract

In situ (mobile) sampling of 33 natural dust devil vortices reveals very high total suspended particle (TSP) mean values of 296 mg m−3 and fine dust loadings (PM10) mean values ranging from 15.1 to 43.8 mg m−3 (milligrams per cubic meter). Concurrent three-dimensional wind profiles show mean tangential rotation of 12.3 m s−1 and vertical uplift of 2.7 m s−1 driving mean vertical TSP flux of 1689 mg m−3 s−1 and fine particle flux of ~1.0 to ~50 mg m−3 s−1. Peak PM10 dust loading and flux within the dust column are three times greater than mean values, suggesting previous estimates of dust devil flux might be too high. We find that deflation rates caused by dust devil erosion are ~2.5–50 μm per year in dust devil active zones on Earth. Similar values are expected for Mars, and may be more significant there where competing erosional mechanisms are less likely.

dc.publisherAcademic Press
dc.titleIn situ measurements of particle load and transport in dust devils
dc.typeJournal Article
dcterms.source.volume214
dcterms.source.number2
dcterms.source.startPage766
dcterms.source.endPage772
dcterms.source.issn0019-1035
dcterms.source.titleIcarus
curtin.accessStatusFulltext not available


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