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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01xg94hs15v
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dc.contributor.authorZweben, S.J.-
dc.contributor.authorTerry, J.L.-
dc.contributor.authorStotler, D.P.-
dc.contributor.authorMaqueda, R.J.-
dc.date.accessioned2017-07-20T14:23:07Z-
dc.date.available2017-07-20T14:23:07Z-
dc.date.issued2017-04-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01xg94hs15v-
dc.description.abstractGas puff imaging (GPI) is a diagnostic of plasma turbulence which uses a puff of neutral gas at the plasma edge to increase the local visible light emission for improved space-time resolution of plasma fluctuations. This paper reviews gas puff imaging diagnostics of edge plasma turbulence in magnetic fusion research, with a focus on the instrumentation, diagnostic cross-checks, and interpretation issues. The gas puff imaging hardware, optics, and detectors are described for about 10 GPI systems implemented over the past ~15 years. Comparison of GPI results with other edge turbulence diagnostic results are described and many common features are observed. Several issues in the interpretation of GPI measurements are discussed, and potential improvements in hardware and modeling are suggested.en_US
dc.description.tableofcontentsreadme, data filesen_US
dc.language.isoen_USen_US
dc.publisherPrinceton Plasma Physics Laboratory, Princeton Universityen_US
dc.relationReview of Scientific Instruments, vol. 88, P. 041101 (April 2017)en_US
dc.relation.isreferencedbyhttp://dx.doi.org/10.1063/1.4981873en_US
dc.subjectGas puff imagingen_US
dc.titleGas Puff Imaging Diagnostics of Edge Plasma Turbulence in Magnetic Fusion Devicesen_US
dc.typeDataseten_US
pu.projectgrantnumber31016 G0001 10003086 101-
pu.depositorKaye, S.M.-
dc.contributor.funderU. S. Department of Energy contract number DE-AC02-09CH11466en_US
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