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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01gf06g542h
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dc.contributor.authorKim, E.-W.-
dc.contributor.authorBertelli, N.-
dc.contributor.authorJohnson, J.R.-
dc.contributor.authorValeo, E.-
dc.contributor.authorHosea, J.-
dc.contributor.authorPerkins, R.-
dc.date.accessioned2018-10-03T13:42:54Z-
dc.date.available2018-10-03T13:42:54Z-
dc.date.issued2018-10-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01gf06g542h-
dc.description.abstractWe illustrate the capabilities of a recently developed two-dimensional full wave code (FW2D) in space and tokamak plasmas by adopting various values of density, magnetic field configuration and strength as well as boundary shape. As example, we first showed fast compressional wave propagation in the inner magnetosphere is dramatically modified by a plasmaspheric plume at Earth's magnetosphere. The results show that wave energy is trapped in the plume showing a leaky eigenmode-like structure with plume, which is similar to the detected magnetosonic waves. We also performed simulations of high harmonic fast waves in the scrape-off layer (SOL) plasmas of the National Spherical Torus eXperiment (NSTX)/NSTX-Upgrade. Comparison the results with previous full-wave simulations show that although the FW2D code uses a cold plasma approximation, the electric field and the fraction of the power losses in the SOL plasmas show excellent consistency and agreement with the previous full wave simulations performed by the AORSA code.en_US
dc.description.tableofcontentsreadme and digital data filesen_US
dc.language.isoen_USen_US
dc.publisherPrinceton Plasma Physics Laboratory, Princeton Universityen_US
dc.relationPhys. Plasmasen_US
dc.titleTwo-dimensional full-wave simulations of waves in space and tokamak plasmasen_US
dc.typeDataseten_US
pu.projectgrantnumber31016 G0001 10003086 101-
pu.depositorKaye, Stanley-
dc.contributor.funderU. S. Department of Energy contract number DE-AC02-09CH11466en_US
Appears in Collections:NSTX-U

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