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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp012v23vx30c
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dc.contributor.authorZweben SJ-
dc.contributor.authorFredrickson ED-
dc.contributor.authorMyra JR-
dc.contributor.authorPodesta M-
dc.contributor.authorScotti F-
dc.date.accessioned2020-07-08T17:00:05Z-
dc.date.available2020-07-08T17:00:05Z-
dc.date.issued2020-05-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp012v23vx30c-
dc.description.abstractThis paper describes a study of the cross-correlations between edge fluctuations as seen in the gas puff imaging (GPI) diagnostic and low frequency coherent magnetic fluctuations (MHD) in H-mode plasmas in NSTX. The main new result was that large blobs in the SOL were significantly correlated with MHD activity the 3-6 kHz range in 21 of the 223 shots examined. There were also many other shots in which fluctuations in the GPI signal level and its peak radius Rpeak were correlated with MHD activity, but without any significant correlation of the MHD with large blobs. The structure and motion of the MHD is compared with that of the correlated blobs, and some possible theoretical mechanisms for the MHD-blob correlation are discussed.en_US
dc.description.tableofcontentsreadme and digital data filesen_US
dc.language.isoen_USen_US
dc.publisherPrinceton Plasma Physics Laboratory, Princeton Universityen_US
dc.relationPhysics of Plasmasen_US
dc.subjectblobsen_US
dc.subjectMHDen_US
dc.subjectNSTXen_US
dc.titleMHD-blob correlations in NSTXen_US
dc.typeDataseten_US
dc.contributor.funderU. S. Department of Energyen_US
Appears in Collections:NSTX

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