Dust-Alfvenic Shocklets in Dusty Plasmas

dc.contributor.author	Shukla, P. K
dc.contributor.author	Morfill, G. E
dc.contributor.author	Krishan, V
dc.date.accessioned	2013-06-24T13:42:51Z
dc.date.available	2013-06-24T13:42:51Z
dc.date.issued	2004
dc.identifier.citation	Physica Scripta, Vol. T113, pp. 149–150	en
dc.identifier.issn	0031-8949
dc.identifier.uri	http://hdl.handle.net/2248/6129
dc.description	Restricted Access	en
dc.description.abstract	We 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.iso	en	en
dc.publisher	IOP Publishing	en
dc.relation.uri	http://dx.doi.org/10.1238/Physica.Topical.113a00149	en
dc.rights	© IOP Publishing	en
dc.subject	Dusty or complex plasmas	en
dc.subject	Plasma crystals	en
dc.subject	Magnetohydrodynamic waves
dc.title	Dust-Alfvenic Shocklets in Dusty Plasmas	en
dc.type	Article	en