2026-05-05T20:48:33Zhttps://uvadoc.uva.es/oai/request

oai:uvadoc.uva.es:10324/569322025-02-13T13:33:09Zcom_10324_1159com_10324_931com_10324_894col_10324_1310

Ion dynamics effect on stark-broadened line shapes: A cross-comparison of various models Ferri, Sandrine Calisti, Annette Mossé, Caroline Rosato, Joël Talin, Bernard Alexiou, Spiros Gigosos Pérez, Marco Antonio González Delgado, Manuel Ángel González Herrero, Diego Lara, Natividad Gomez, Thomas Iglesias, Carlos Lorenzen, Sonja Mancini, Roberto Stambulchik, Evgeny Modeling the Stark broadening of spectral lines in plasmas is a complex problem. The problem has a long history, since it plays a crucial role in the interpretation of the observed spectral lines in laboratories and astrophysical plasmas. One difficulty is the characterization of the emitter’s environment. Although several models have been proposed over the years, there have been no systematic studies of the results, until now. Here, calculations from stochastic models and numerical simulations are compared for the Atoms 2014, 2 300 Lyman-α and -β lines in neutral hydrogen. Also discussed are results from the Helium-α and -β lines of Ar XVII. 2022-11-10T13:16:25Z 2022-11-10T13:16:25Z 2022-11-10T13:16:25Z 2014 info:eu-repo/semantics/article Atoms, 2014, vol.2, n. 3, p. 299-318 2218-2004 https://uvadoc.uva.es/handle/10324/56932 10.3390/atoms2030299 299 3 318 Atoms 2 2218-2004 eng https://www.mdpi.com/2218-2004/2/3/299 info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/3.0/ © 2014 The Author(s) Attribution 3.0 Unported MDPI