COLLISIONS IN DUSTY PLASMAS

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DC Field	Value	Language
dc.contributor.author	Issam BENDAHMANE and Baya BENTAG	-
dc.date.accessioned	2013-12-22T11:40:08Z	-
dc.date.available	2013-12-22T11:40:08Z	-
dc.date.issued	2011-02-15	-
dc.identifier.issn	ya	-
dc.identifier.uri	http://hdl.handle.net/123456789/3724	-
dc.description	SIPP 2011 UKM Ouargla 13 15 Fevrier 2011	en_US
dc.description.abstract	In space, numerous solid micro-particles called “dust” are among the constituents of space plasmas. The latter are called “dusty plasmas”, and this dust can help determine many of the properties of interstellar media, stars, planet formation regions, planetary rings, comets tails, etc. One of the important subjects in “dusty plasmas” is dust collisions which we will study using stochastical methods to obtain their statistical properties. We will use mainly the Fokker-Plank equation in order to derive the probability distribution which will provide us with all the information that is needed to study the phenomenon (stochastic process). The general form of the Fokker-Planck equations that we will use to study plasma collisions is [1]:	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	2011;	-
dc.subject	dusty plasma	en_US
dc.subject	dust collisions	en_US
dc.subject	stochastic process	en_US
dc.subject	statistical properties	en_US
dc.title	COLLISIONS IN DUSTY PLASMAS	en_US
dc.type	Article	en_US
Appears in Collections:	1. Faculté des mathématiques et des sciences de la matière

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