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dc.contributor.authorRice, John E.en_US
dc.contributor.authorFournier, K.B.en_US
dc.contributor.authorKemp, G.E.en_US
dc.contributor.authorBitter, M.en_US
dc.contributor.authorCao, N.en_US
dc.contributor.authorDelgado-Aparicio, L.en_US
dc.contributor.authorHill, K.en_US
dc.contributor.authorHubbard, Amanda E.en_US
dc.contributor.authorHughes, Jerry W.en_US
dc.contributor.authorReinke, M.L.en_US
dc.date.accessioned2025-03-21T20:14:53Z
dc.date.available2025-03-21T20:14:53Z
dc.date.issued2019-07
dc.identifier19ja031
dc.identifier.urihttps://hdl.handle.net/1721.1/158615
dc.descriptionSubmitted for publication in Journal of Physics B: Atomic, Molecular and Optical Physics
dc.description.abstractX-ray spectra in the wavelength range from 2.70 to 2.76 A from xenon (Z = 54) in near neon-like charge states have been observed in Alcator C-Mod tokamak plasmas. The 3D (2p^6 - (2p^5)_{3/2}3d_{5/2}, 2720.4 mA) and 3F (2p^6 - (2p^5)_{1/2}3s_{1/2}, 2729.0 mA) transitions from neon-like Xe^{44+} have been identified, along with nearby Na-, Mg- and Al-like satellites. The intensity ratio of 3D to the Mg-like satellite near 2.74 A increases strongly with electron temperature in the range from 3 to 4 keV.
dc.publisherIOPen_US
dc.relation.isversionofdoi.org/10.1088/1361-6455/ab5c7f
dc.sourcePlasma Science and Fusion Centeren_US
dc.titleX-ray Observations of Ne-like Xe and Satellites from C-Mod Tokamak Plasmasen_US
dc.typeArticleen_US
dc.contributor.departmentMassachusetts Institute of Technology. Plasma Science and Fusion Center
dc.relation.journalJournal of Physics B: Atomic, Molecular and Optical Physics


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