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000007943 084__ $$2WoS$$aPhysics, Fluids & Plasmas
000007943 084__ $$2WoS$$aPhysics, Mathematical
000007943 1001_ $$0P:(DE-Juel1)VDB75892$$aRosato, J.$$b0$$uFZJ
000007943 245__ $$aStark broadening of hydrogen lines in low-density magnetized plasmas
000007943 260__ $$aCollege Park, Md.$$bAPS$$c2009
000007943 264_1 $$2Crossref$$3online$$bAmerican Physical Society (APS)$$c2009-04-27
000007943 264_1 $$2Crossref$$3print$$bAmerican Physical Society (APS)$$c2009-04-01
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000007943 440_0 $$04924$$aPhysical Review E$$vE79$$x1539-3755$$y4
000007943 500__ $$aThis work was partially supported by the project "Radiation Absorption Effects" of the French Federation de Recherche sur la Fusion Magnetique, by the project "PHOTONITER" of the French Agence Nationale de la Recherche (Contract No. ANR-07-BLAN-0187-01), and by the collaboration LRC DSM 99-14 (PIIM/CEA Cadarache)
000007943 520__ $$aStark broadening of hydrogen lines in the presence of a magnetic field is revisited, with emphasis on the role of the ion component under typical conditions of magnetized fusion devices. An impact theory for ions valid at low density (N-e less than or similar to 10(14) cm(-3)) and taking into account the Zeeman degeneracy removal of the atomic states is developed. It is shown that the Stark widths of the Lorentz triplet components strongly depend on the magnetic field. The model is validated by a computer simulation method. For the lateral sigma components of Ly alpha, we show that the impact approximation still holds for densities as high as N-e similar to 10(15) cm(-3). In contrast, for the central pi component as well as for the other lines from low principal quantum number, significant discrepancies between the proposed theory and the simulation results appear at high density. Application to D alpha in tokamak divertor plasma conditions shows that, in this case, the quasistatic approximation becomes more relevant.
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000007943 65320 $$2Author$$afusion reactor divertors
000007943 65320 $$2Author$$aplasma density
000007943 65320 $$2Author$$aplasma simulation
000007943 65320 $$2Author$$aspectral line breadth
000007943 65320 $$2Author$$aspectral line broadening
000007943 65320 $$2Author$$aStark effect
000007943 65320 $$2Author$$aTokamak devices
000007943 65320 $$2Author$$aZeeman effect
000007943 650_7 $$2WoSType$$aJ
000007943 7001_ $$0P:(DE-HGF)0$$aMarandet, Y.$$b1
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000007943 7001_ $$0P:(DE-HGF)0$$aFerri, S.$$b3
000007943 7001_ $$0P:(DE-HGF)0$$aMossé, C.$$b4
000007943 7001_ $$0P:(DE-HGF)0$$aGodbert-Mouret, L.$$b5
000007943 7001_ $$0P:(DE-HGF)0$$aKoubiti, M.$$b6
000007943 7001_ $$0P:(DE-HGF)0$$aStamm, R.$$b7
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000007943 8567_ $$uhttp://dx.doi.org/10.1103/PhysRevE.79.046408
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