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Acceleration of Macroscopic Clusters in Crossed Magnetic Fields

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dc.contributor.authorKarimov, AlexanderR.
dc.contributor.authorShikanov, AlexanderE.
dc.contributor.authorMurad, PaulA.
dc.contributor.authorTerekhov, SvyatoslavA.
dc.contributor.authorКаримов, Александр Рашатович
dc.contributor.authorШиканов, Александр Евгеньевич
dc.contributor.authorТерехов, Святослав Алексеевич
dc.date.accessioned2024-11-20T09:47:54Z
dc.date.available2024-11-20T09:47:54Z
dc.date.issued2019
dc.description.abstractThe acceleration of rotating plasma flow in crossed magnetic fields produced momentum transfer between the macroscopic degrees of freedom for a plasma flow was investigated. Results implied a concept for acceleration of plasma flow containing the charged macroscopic particles. Here, the case is treated when the plasma flow consists of electrons, protons, and heavy, multiply charged negative dust particles only. The analysis shows that these charged macroscopic particles have been trapped and, then, accelerated in the main plasma flow. As a result, such complex plasma flow can be accelerated in one axial direction to increase the thrust. It suggests that such complex plasma flow produced, for example, from cosmic dust medium may be used as a propellant and a work body for plasma thrusters.
dc.format.extentС. 1520-1525;
dc.identifier.citationAcceleration of Macroscopic Clusters in Crossed Magnetic Fields / Karimov, AlexanderR [et al.] // IEEE Transactions on Plasma Science. - 2019. - 47. - № 3. - P. 1520-1525;. - 10.1109/TPS.2019.2893368
dc.identifier.doi10.1109/TPS.2019.2893368
dc.identifier.urihttps://www.doi.org/10.1109/TPS.2019.2893368
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85062714404&origin=resultslist
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dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/16644
dc.relation.ispartofIEEE Transactions on Plasma Science
dc.titleAcceleration of Macroscopic Clusters in Crossed Magnetic Fields
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue3
oaire.citation.volume47
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