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dc.contributor.authorLand, Victor
dc.contributor.authorMatthews, Lorin
dc.contributor.authorHyde, Truell
dc.contributor.authorBolser, Diana
dc.date.accessioned2010-05-12T16:20:43Z
dc.date.available2010-05-12T16:20:43Z
dc.date.issued2010-05-12
dc.identifier.citationPhys. Rev. E, 81, 056402, 2010en
dc.identifier.urihttp://hdl.handle.net/2104/5771
dc.description.abstractA self-consistent dusty plasma fluid model has been extended to incorporate all the noble gases as the carrier gas. An analysis of void closure in complex plasma composed of these gases over a wide range of experimental parameters is presented. Driving potential-pressure maps are constructed, which show the range in parameter space where isotropic void-free dust crystals can be expected, where a void is to be expected and where the discharge is expected to extinguish.en
dc.format.extent493542 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoenen
dc.publisherPhysics Review Een
dc.titleFluid modeling of void closure in microgravity noble gas complex plasmasen
dc.typeArticleen
dc.identifier.doi10.1103/PhysRevE.81.056402
dc.description.keywordscomplex plasmaen
dc.description.keywordsdusty plasmaen
dc.description.keywordsfluid modelen
dc.description.keywordsdust voiden
dc.description.keywordsnoble gasen


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