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Wave modelling in a cylindrical non-uniform helicon discharge

dc.contributor.authorChang, L.
dc.contributor.authorHole, M. J.
dc.contributor.authorCaneses, J. F.
dc.contributor.authorChen, G.
dc.contributor.authorBlackwell, B. D.
dc.contributor.authorCorr, C. S.
dc.date.accessioned2015-12-08T23:18:31Z
dc.date.available2015-12-08T23:18:31Z
dc.date.issued2012-08-31
dc.date.updated2016-02-24T11:20:10Z
dc.description.abstractA radio frequency (RF) field solver based on Maxwell's equations and a cold plasma dielectric tensor is em- ployed to describe wave phenomena observed in a cylindrical non-uniform helicon discharge. The experiment is carried out on a recently built linear plasma-material interaction machine: the MAGnetized Plasma In- teraction Experiment (MAGPIE) [B. D. Blackwell, J. F. Caneses, C. Samuell, J. Wach, J. Howard, and C. S. Corr, submitted on 25 March 2012 to Plasma Sources Science and Technology], in which both plasma density and static magnetic field are functions of axial position. The field strength increases by a factor of 15 from source to target plate, and plasma density and electron temperature are radially non-uniform. With an enhancement factor of 9.5 to the electron-ion Coulomb collision frequency, 12% reduction in the antenna radius, and the same other conditions as employed in the experiment, the solver produces axial and radial profiles of wave amplitude and phase that are consistent with measurements. Ion-acoustic turbulence, which can happen if electron drift velocity exceeds the speed of sound in magnetized plasmas, may account for the factor of 9.5 used to match simulated results with experimental data. To overcome the single m vacuum solu- tion limitations of the RF solver, which can only compute the glass response to the same mode number of the antenna, we have adjusted the antenna radius to match the wave field strength in the plasma.(not finished because of the limited number of characters, please see the full paper)
dc.description.sponsorshipOne of the authors—Lei Chang—appreciates the fi- nancial support provided by Chinese Scholarship Council for his Ph.D. study at The Australian National University, and the Student Conference Support from Australian Institute of Physics for him to present this work in the 39th European Physical Society Conference on Plasma Physics and 16th International Congress on Plasma Physics (Stockholm, Sweden, 2-6 July 2012). M. J. Hole and C. S. Corr acknowledge the support of the ARC through fellowships, FT0991899 and FT100100825, respectively.en_AU
dc.identifier.issn1070-664Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/38421
dc.publisherAmerican Institute of Physics (AIP)
dc.relationhttp://purl.org/au-research/grants/arc/FT0991899
dc.relationhttp://purl.org/au-research/grants/arc/FT100100825
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/1070-664X..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 9/12/15). Copyright 2012 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in Physics of Plasmas and may be found at https://doi.org/10.1063/1.4748874
dc.sourcePhysics of Plasmas
dc.subjectKeywords: Axial gradient; Axial positions; Cold plasmas; Collision frequency; Core plasma; Coulomb collision; Edge heating; Electron ions; Enhancement factor; Field strengths; Focused fields; Helicon discharge; Helicon waves; Ionization efficiency; Nonuniform field
dc.titleWave modelling in a cylindrical non-uniform helicon discharge
dc.typeJournal article
local.bibliographicCitation.issue8en_AU
local.bibliographicCitation.startpage083511en_AU
local.contributor.affiliationChang, Lei, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationHole, Matthew, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationCaneses, Juan, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationChen, G., Oak Ridge National Laboratory, United States of Americaen_AU
local.contributor.affiliationBlackwell, Boyd, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationCorr, Cormac, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.authoruidu4646143en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor020204en_AU
local.identifier.ariespublicationu4695161xPUB95en_AU
local.identifier.citationvolume19en_AU
local.identifier.doi10.1063/1.4748874en_AU
local.identifier.scopusID2-s2.0-84865739091
local.identifier.thomsonID000309252500103
local.publisher.urlhttps://www.aip.org/en_AU
local.type.statusPublished Versionen_AU

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