Exact Stark analytical function for H{\alpha} line based on the FFM Model related with plasma parameters
A. Sarsa, A. Jim\'enez-Solano, M.S. Dimitrijevi\'c, C. Yubero

TL;DR
This paper presents a comprehensive analytical model for Stark broadening of the Hα line in plasmas, enabling accurate plasma parameter diagnostics across various conditions using spectral data and genetic algorithm optimization.
Contribution
The paper introduces a full splitting Stark broadening model for Hα line incorporating micro-field fluctuations, with parameters fitted via genetic algorithms for diverse plasma conditions.
Findings
Model accurately fits spectral data across plasma conditions
Parameters depend on electron density and temperature
Provides a tool for plasma diagnostics from experimental profiles
Abstract
Optical Emission Spectroscopy is a widely used technique for plasma diagnosis, with particular interest in hydrogen atomic emission due to its prevalence in plasmas. However, accurately determining plasma parameters like electron density, electron temperature, and gas temperature starting from the experimental profiles remains a challenge. This paper introduces a comprehensive model for Stark broadening of the H{\alpha} line in a wide range of plasma conditions, addressing the limitations of existing analytical expressions for line shapes. The proposed model encompasses the full splitting of the transition into fifteen Lorentzian profiles and electric micro-field fluctuations surrounding the emitting atoms due to collisions with charged particles. Starting from accurate spectral data obtained from realistic computer simulations, fitting parameters of the model, have been obtained by…
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