RT info:eu-repo/semantics/article
T1 Ion dynamics effect on stark-broadened line shapes: A cross-comparison of various models
A1 Ferri, Sandrine
A1 Calisti, Annette
A1 Mossé, Caroline
A1 Rosato, Joël
A1 Talin, Bernard
A1 Alexiou, Spiros
A1 Gigosos Pérez, Marco Antonio
A1 González Delgado, Manuel Ángel
A1 González Herrero, Diego
A1 Lara, Natividad
A1 Gomez, Thomas
A1 Iglesias, Carlos
A1 Lorenzen, Sonja
A1 Mancini, Roberto
A1 Stambulchik, Evgeny
K1 Stark broadening
K1 Spectral line shapes
K1 Plasma
K1 33 Ciencias Tecnológicas
AB 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.
PB MDPI
SN 2218-2004
YR 2014
FD 2014
LK https://uvadoc.uva.es/handle/10324/56932
UL https://uvadoc.uva.es/handle/10324/56932
LA eng
NO Atoms, 2014, vol.2, n. 3, p. 299-318
NO Producción Científica
DS UVaDOC
RD 06-ago-2024