Soft x-ray emission of galliumlike rare-earth atoms produced by high-temperature low-density tokamak and high-density laser plasmas

Spectra of rare-earth atoms praseodymium, [ital Z]=59, to ytterbium, [ital Z]=70, emitted from the high-temperature (1 keV) low-density (10[sup 13] cm[sup [minus]3]) TEXT tokamak (at the Fusion Research Center, University of Texas, Austin) and high-density (10[sup 20] cm[sup [minus]3]) laser plasmas...

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Veröffentlicht in:Physical review. A, Atomic, molecular, and optical physics Atomic, molecular, and optical physics, 1994-09, Vol.50 (3), p.2248-2256
Hauptverfasser: Fournier, KB, Goldstein, WH, Osterheld, A, Finkenthal, M, Lippmann, S, Huang, LK, Moos, HW, Spector, N
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Sprache:eng
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Zusammenfassung:Spectra of rare-earth atoms praseodymium, [ital Z]=59, to ytterbium, [ital Z]=70, emitted from the high-temperature (1 keV) low-density (10[sup 13] cm[sup [minus]3]) TEXT tokamak (at the Fusion Research Center, University of Texas, Austin) and high-density (10[sup 20] cm[sup [minus]3]) laser plasmas have been recorded in the soft-x-ray range of 50--200 A with an image intensifier detector and on photographic plates. The brightest [ital n]=4 to [ital n]=4 transitions of galliumlike ions have been identified and their emission patterns have been studied by comparison with [ital ab] [ital initio] atomic structure calculations and collisional radiative models under the respective plasma conditions. We have investigated the use of the ratios of the intensities of 4-4 transitions as indicators of plasma densities. This is possible owing to the doublet structure of the galliumlike ground state, which leads to a strong density dependence for ratios of transitions between low-lying levels. We have also used semiempirical ionization balance calculations to characterize the charge state distribution of the tokamak plasmas, in preparation for an investigation of the use of ratios of galliumlike to zinclike and copperlike emission features as indicators of whether the impurities are in coronal equilibrium or undergoing ionization.
ISSN:1050-2947
1094-1622
DOI:10.1103/physreva.50.2248