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dc.contributor.authorBanerjee, S.-
dc.contributor.authorA. Diallo-
dc.contributor.authorS.J. Zweben-
dc.date.accessioned2016-04-04T20:48:13Z-
dc.date.available2016-04-04T20:48:13Z-
dc.date.issued2016-04-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp0170795b055-
dc.description.abstractA quasi-coherent mode with frequency f = 40 kHz is observed in Ohmic plasmas in NSTX with the gas puff imaging diagnostic (GPI). This mode is located predominantly just inside the separatrix, with a maximum fluctuation amplitude similar to that of the broadband turbulence in the same frequency range. The quasi-coherent mode has a poloidal wavelength 16 cm and a poloidal velocity 49 km/s in the electron diamagnetic direction, which are similar to the characteristics expected from a linear drift-wave like mode in the edge.en_US
dc.description.tableofcontentsreadme and hdf5 filesen_US
dc.language.isoen_USen_US
dc.publisherPrinceton Plasma Physics Laboratory, Princeton Universityen_US
dc.relationPhysics of Plasmas, vol. 23, p. 044502, April 2016en_US
dc.relation.isreferencedbydoi: 10.1063/1.4946871en_US
dc.subjectTurbulenceen_US
dc.titleObservation of quasi-coherent edge fluctuations in Ohmic plasmas on NSTXen_US
dc.typeDataseten_US
pu.projectgrantnumber31016 G0001 10003086 101en_US
pu.depositorKaye, Stanley-
dc.contributor.funderU. S. Department of Energy contract number DE-AC02-09CH11466en_US
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