A multichannel magnetic probe system for analysing magnetic fluctuations in helical axis plasmas

dc.contributor.authorHaskey, S. R.
dc.contributor.authorBlackwell, B. D.
dc.contributor.authorSeiwald, B.
dc.contributor.authorHole, M. J.
dc.contributor.authorPretty, D. G.
dc.contributor.authorHoward, J.
dc.contributor.authorWach, J.
dc.date.accessioned2015-09-22T06:35:03Z
dc.date.available2015-09-22T06:35:03Z
dc.date.issued2013-09-03
dc.date.updated2016-02-24T09:25:19Z
dc.description.abstractThe need to understand the structure of magnetic fluctuations in H-1NF heliac [S. Hamberger et al., Fusion Technol. 17, 123 (1990)] plasmas has motivated the installation of a sixteen former, tri-axis helical magnetic probe Mirnov array (HMA). The new array complements two existing poloidal Mirnov arrays by providing polarisation information, higher frequency response, and improved toroidal resolution. The helical placement is ideal for helical axis plasmas because it positions the array as close as possible to the plasma in regions of varying degrees of favourable curvature in the magnetohydrodynamic sense, but almost constant magnetic angle. This makes phase variation with probe position near linear, greatly simplifying the analysis of the data. Several of the issues involved in the design, installation, data analysis, and calibration of this unique array are presented including probe coil design, frequency response measurements, mode number identification, orientation calculations, and mapping probe coil positions to magnetic coordinates. Details of specially designed digitally programmable pre-amplifiers, which allow gains and filters to be changed as part of the data acquisition initialisation sequence and stored with the probe signals, are also presented. The low shear heliac geometry [R. Jiménez-Gómez et al., Nucl. Fusion 51, 033001 (2011)], flexibility of the H-1NF heliac, and wealth of information provided by the HMA create a unique opportunity for detailed study of Alfvén eigenmodes, which could be a serious issue for future fusion reactors.
dc.description.sponsorshipThis work was supported by the Education Investment Fund under the Super Science Initiative of the Australian Government. S.R.H. wishes to thank AINSE Ltd. for providing financial assistance to enable this work on H-1NF to be conducted.en_AU
dc.identifier.issn0034-6748en_AU
dc.identifier.urihttp://hdl.handle.net/1885/15648
dc.publisherAmerican Institute of Physics
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0034-6748..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 22/09/15). Copyright 2013 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 (Haskey, S. R., et al. "A multichannel magnetic probe system for analysing magnetic fluctuations in helical axis plasmas." Review of Scientific Instruments 84.9 (2013): 093501.) and may be found at https://doi.org/10.1063/1.4819250
dc.sourceReview of Scientific Instruments
dc.subjectKeywords: Frequency response measurement; Magnetic coordinates; Magnetic fluctuation; Magnetic probes; Phase variation; Polarisation informations; Probe position; Probe signals; Frequency response; Magnetism; Magnetohydrodynamics; Probes; Magnetoplasma
dc.titleA multichannel magnetic probe system for analysing magnetic fluctuations in helical axis plasmas
dc.typeJournal article
local.bibliographicCitation.issue9en_AU
local.bibliographicCitation.startpage093501en_AU
local.contributor.affiliationHaskey, Shaun, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_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.affiliationSeiwald, Bernhard, 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.affiliationPretty, David, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationHoward, John, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationWach, John, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.authoruidu4707372en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor020204en_AU
local.identifier.absfor020303en_AU
local.identifier.ariespublicationf5625xPUB4421en_AU
local.identifier.citationvolume84en_AU
local.identifier.doi10.1063/1.4819250en_AU
local.identifier.essn1089-7623en_AU
local.identifier.scopusID2-s2.0-84885153224
local.identifier.thomsonID000325402000014
local.publisher.urlhttps://www.aip.org/en_AU
local.type.statusPublished Versionen_AU

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