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Measurements of poloidal rotation velocity using cross-correlation spectroscopy in the H-1 heliac

dc.contributor.authorShats, M. G.
dc.contributor.authorPunzmann, H.
dc.contributor.authorXia, H.
dc.contributor.authorSolomon, W. M.
dc.date.accessioned2015-10-09T04:31:33Z
dc.date.available2015-10-09T04:31:33Z
dc.date.issued2003-03
dc.date.updated2015-12-12T08:20:34Z
dc.description.abstractA correlation spectroscopy diagnostic [M.G. Shats and J. Howard, Fusion Eng. Des. 34–35, 271 (1997)] measures fluctuation spectra and local fluctuation intensities in a radiation-dominated plasma, such as the low-temperature plasma in the H-1 heliac (Te<50 eV, ne<2×10¹⁸ m⁻³). When the fluctuation coherence lengths in the poloidal and radial directions are shorter than the plasma radius, the cross-correlation function of the two crossed-sightline fluctuating intensities contains information about the fluctuations amplitude and their phase in the intersection volume. The optical setup on the H-1 heliac uses two nearly orthogonal views to image 20 optical fibers arranged into two linear arrays in the plasma poloidal cross section. A matrix of 10×10 cross-correlation functions is then analyzed to determine the poloidal phase velocity of the fluctuations, poloidal and radial correlation lengths, and the radial profiles of the fluctuations intensity. The results on the poloidal propagation velocity measured using the cross-correlation technique (time delay of the cross-correlation functions) are compared with the poloidal velocity measured using poloidally separated probes in the plasma. Both velocities are found to be in good agreement and also agree well with the E×B drift velocity in this plasma.
dc.identifier.issn0034-6748en_AU
dc.identifier.urihttp://hdl.handle.net/1885/15853
dc.publisherAmerican Institute of Physics (AIP)
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 8/10/15). Copyright 2003 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 Review of Scientific Instruments and may be found at https://doi.org/10.1063/1.1537032
dc.sourceReview of Scientific Instruments
dc.subjectKeywords: Magnetic field effects; Optical fibers; Plasma oscillations; Plasma turbulence; Spectroscopic analysis; Poloidal rotation velocity; Plasmas
dc.titleMeasurements of poloidal rotation velocity using cross-correlation spectroscopy in the H-1 heliac
dc.typeJournal article
local.bibliographicCitation.issue3en_AU
local.bibliographicCitation.lastpage2047en_AU
local.bibliographicCitation.startpage2044en_AU
local.contributor.affiliationShats, Michael, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationPunzmann, Horst, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationXia, Hua, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.affiliationSolomon, W., College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National Universityen_AU
local.contributor.authoruidu9113958en_AU
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor020204en_AU
local.identifier.ariespublicationMigratedxPub16297en_AU
local.identifier.citationvolume74en_AU
local.identifier.doi10.1063/1.1537032en_AU
local.identifier.scopusID2-s2.0-0037350129
local.publisher.urlhttps://www.aip.org/en_AU
local.type.statusPublished Versionen_AU

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