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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6129
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dc.contributor.authorShukla, P. K-
dc.contributor.authorMorfill, G. E-
dc.contributor.authorKrishan, V-
dc.date.accessioned2013-06-24T13:42:51Z-
dc.date.available2013-06-24T13:42:51Z-
dc.date.issued2004-
dc.identifier.citationPhysica Scripta, Vol. T113, pp. 149–150en
dc.identifier.issn0031-8949-
dc.identifier.urihttp://hdl.handle.net/2248/6129-
dc.descriptionRestricted Accessen
dc.description.abstractWe show that the Hall dust magnetohydrodynamic equations admit a non-stationary dust-Alfvénic shock solution in dusty plasmas. The dust-Alfvénic shocklet (DAS) occurs on a long temporal (dust gyroperiod) and spatial (dust skin depth) scales. The present result can have relevance to acceleration of charged grains by the DAS in space dusty plasmas.en
dc.language.isoenen
dc.publisherIOP Publishingen
dc.relation.urihttp://dx.doi.org/10.1238/Physica.Topical.113a00149en
dc.rights© IOP Publishingen
dc.subjectDusty or complex plasmasen
dc.subjectPlasma crystalsen
dc.subjectMagnetohydrodynamic waves-
dc.titleDust-Alfvenic Shocklets in Dusty Plasmasen
dc.typeArticleen
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