Spectral Line Shapes in Plasmas Workshops
This is a home to the SLSP (Spectral Line Shapes in Plasmas) code comparison workshop series.
Motivation
Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space plasmas. Evidently, its reliable implementation requires sufficiently accurate calculations. The Stark broadening is the most computationally challenging contribution, with other factors (such as the Zeeman and Doppler effects) further complicating the calculations.
Except for limiting cases, line-shape calculations imply a usage of computer codes of varying complexity and requirements of computational resources. However, studies comparing different computational and analytical methods are almost nonexistent. This workshop purports to fill this gap. By detailed comparison of results for a selected set of case problems, it becomes possible to pinpoint sources of disagreements, infer limits of applicability, and assess accuracy.
Timeline
Discussion
Please use the forums for discussion.
Publications
2024
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Impact of penetrating collisions of plasma ions on spectral line shapes
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Line shape code comparison of the effect of periodic fields on hydrogen lines
2020
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Hydrogen line shapes in plasmas with large magnetic fields
2019
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Spectral Line Shapes in Plasmas II
2018
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ZEST: A fast code for simulating Zeeman–Stark line-shape functions
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Influence of helical trajectories of perturbers on Stark line shapes in magnetized plasmas
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The Fourth Workshop on Lineshape Code Comparison: Line merging
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Stark broadening of Cr III spectral lines: DO white dwarfs
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Broadening of the neutral helium 492-nm line in a corona discharge: Code comparisons and data fitting
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Matrix methods for solving Hartree-Fock equations in atomic structure calculations and line broadening
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C. Stollberg, E. Stambulchik, B. Duan, M. A. Gigosos, D. González Herrero, C. A. Iglesias, and C. MosséRevisiting Stark width and shift of He II Pα
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R. R. Sheeba, M. Koubiti, N. Bonifaci, F. Gilleron, C. Mossé, J.-C. Pain, J. Rosato, and E. StambulchikHβ line in a corona helium plasma: A multi-code line shape comparison
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The Third and Fourth Workshops on Spectral Line Shapes in Plasma Code Comparison: Isolated lines
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Beyond the linear Stark effect: A retrospective
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A new procedure to determine the plasma parameters from a genetic algorithm coupled with the spectral line-shape code PPP
2017
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Report on the third SLSP code comparison workshop
2014
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S. Alexiou, M. S. Dimitrijević, S. Sahal-Brechot, E. Stambulchik, B. Duan, D. González-Herrero, and M. A. GigososThe Second Workshop on Lineshape Code Comparison: Isolated Lines
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A. Calisti, A. Demura, M. A. Gigosos, D. González-Herrero, C. A. Iglesias, V. S. Lisitsa, and E. StambulchikInfluence of microfield directionality on line shapes
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S. Ferri, A. Calisti, C. Mossé, J. Rosato, B. Talin, S. Alexiou, M. A. Gigosos, M. Á. González, D. González-Herrero, N. Lara, T. Gomez, C. A. Iglesias, S. Lorenzen, R. C. Mancini, and E. StambulchikIon dynamics effect on Stark broadened line shapes: A cross comparison of various models
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Electron-impact widths and shifts of B III 2p–2s lines
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Hydrogen spectral line shape formation in the SOL of fusion reactor plasmas
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B. Omar, M. Á. González, M. A. Gigosos, T. S. Ramazanov, M. C. Jelbuldina, K. N. Dzhumagulova, M. C. Zammit, D. V. Fursa, and I. BraySpectral line shapes of He I line 3889 Å
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Ideal Coulomb plasma approximation in line shape models: Problematic issues
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Widths and shifts of isolated lines of neutral and ionized atoms perturbed by collisions with electrons and ions: An outline of the semiclassical perturbation (SCP) method and of the approximations used for the calculations
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Line-shape code comparison through modeling and fitting of experimental spectra of the C II 723-nm line emitted by the ablation cloud of a carbon pellet
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Spectral-kinetic coupling and effect of microfield rotation on Stark broadening in plasmas
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On the application of Stark broadening data determined with Semiclassical Perturbation approach
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Special Issue on Spectral Line Shapes in Plasmas
2013
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Review of the 1st Spectral Line Shapes in Plasmas code comparison workshop
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The effect of improved satellite line shapes on the argon Heβ spectral feature
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