dc.contributor.author | Rice, John E. | en_US |
dc.contributor.author | Sciortino, Francesco | en_US |
dc.contributor.author | Gu, M. | en_US |
dc.contributor.author | Cao, N. | en_US |
dc.contributor.author | Hughes, Jerry W. | en_US |
dc.contributor.author | Irby, J.H. | en_US |
dc.contributor.author | Marmar, E.S. | en_US |
dc.contributor.author | Mordijck, S. | en_US |
dc.contributor.author | Reinke, M.L. | en_US |
dc.contributor.author | Reksoatmodjo, R. | en_US |
dc.date.accessioned | 2025-03-21T20:14:57Z | |
dc.date.available | 2025-03-21T20:14:57Z | |
dc.date.issued | 2021-07 | |
dc.identifier | 21ja026 | |
dc.identifier.uri | https://hdl.handle.net/1721.1/158616 | |
dc.description | Submitted for publication in Journal of Physics B: Atomic, Molecular and Optical Physics | |
dc.description.abstract | X-ray transitions of the very high-n Rydberg series in Ar^16+ have been observed from Alcator C-Mod tokamak plasmas. Individual emission lines up to 1s16p - 1s^2 have been resolved and the central chord line brightnesses with principal quantum number n between 7 and 16 are generally found to decay as 1/n^alpha, with alpha slightly larger than 3. In the plasma periphery, emission from 1s9p - 1s^2 and 1s10p - 1s^2 are found to be significantly enhanced relative to this decrease, indicative of selected population of these levels through charge exchange between background neutral deuterium in the ground state and Ar^17+. An unresolved feature between the wavelengths of 1s27p - 1s^2 and 1s30p - 1s^2 is also present, which arises through charge exchange with neutral deuterium in the n^* = 3 excited state. The brightnesses of transitions populated by charge exchange are spatially up/down asymmetric, with an excess on the side of the magnetic surface X-point. The relative brightness of the unresolved very high-n feature compared to 1s7p - 1s^2 is found to increase with electron temperature and decrease with electron density. Simulations of line emission just on the long wavelength side of the Ar^16$ ionization limit indicate that the principal quantum number decay exponent is closer to alpha = 4 at very high n. The brightness dependence on n below 16 is in excellent agreement with calculations from the Flexible Atomic Code package. | |
dc.publisher | IOP | en_US |
dc.relation.isversionof | doi.org/10.1088/1361-6455/ac2722 | |
dc.source | Plasma Science and Fusion Center | en_US |
dc.title | The Very High n Rydberg Series of Ar^16+ in Alcator C-Mod Tokamak Plasmas | en_US |
dc.type | Article | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Plasma Science and Fusion Center | |
dc.relation.journal | Journal of Physics B: Atomic, Molecular and Optical Physics | |