Optical Emission Spectroscopy (OES) is perhaps the most flexible plasma diagnostic technique, from the hardware point of view. Non-invasive collection of light and its spectral analysis can be done on virtually any plasma device at any plasma condition. Utilization of the spectral information for the measurement of plasma parameters is much less straightforward. Light emission at optical or VUV wavelengths originates from unstable atomic/molecular electronic states. These are someway excited in the plasma and then undergo a collision/radiative kinetics during their short lifetime. In non-equilibrium plasmas, then, a correct interpretation of the OES outcomes is possible only if the excitation and loss kinetics is well known, together with the relaxation properties of the vibrational and rotational manifolds of molecules. Furthermore, inferring plasma parameters is possible only if particular conditions are fulfilled. It is therefore of paramount importance to address the issue of how to recognize and assess the dominant, if any, process producing the molecular excitation to a radiative state. Starting from a survey of the most common excitation mechanisms, not always the mere electron impact with the ground state, and of the collision kinetics of excited states, we shall address the measurements by OES analysis of the translational and vibrational temperatures, of the electric field in a gas discharge, of the concentration of species, in a variety of non-equilibrium plasma conditions, from low to high pressure, including plasma processing devices, negative ions sources and cold edge plasmas. With a focus on common mistakes arising from the misuse of bad assumptions in the analysis of spectra.
A critical overview of Optical Emission Spectroscopy for plasma diagnostics
Dilecce G.
Conference:
5th European Conference on Plasma Diagnostics - ECPD 2023,
, Rethymmo, Crete, Greece , 23-27 April 2023
Year:
2023
ISTP Authors: Giorgio Dilecce
Keywords: Optical Emission Spectroscopy, plasma diagnostics
Research Activitie: Key note o lezione magistrale
Related products
-
Journal of instrumentation 17 (4), pp. C04017-1 - C04017-9 Year: 2022 DOI: 10.1088/1748-0221/17/04/C04017
Characterization of Cs-free negative ion production in the ion source SPIDER by cavity ring-down spectroscopy
Barbisan M.; Agnello R.; Casati G.; Pasqualotto R.; Sartori E.; Serianni G.
-
2022 Space Propulsion - 8th Edition of the Space Propulsion Conference - SP22 - 3AF, , Estoril, Portugal , 9-13 May 2022 Year: 2022
PIC model of an air-breathing low power Hall thruster
Taccogna F.; Cichocki F.; Minelli P.
-
IEEE transactions on plasma science (Online) 50 (11), pp. 3995 - 4001 Year: 2022 DOI: 10.1109/TPS.2022.3190561
Development of a Collisional Radiative Model for Hydrogen-Cesium Plasmas and Its Application to SPIDER
Pouradier Duteil B.; Sartori E.; Zaniol B.; Barbisan M.; Poggi C.; Spolaore M.; Serianni G.
-
Fusion engineering and design (Print) 192 pp. 113591-1 - 113591-8 Year: 2023 DOI: 10.1016/j.fusengdes.2023.113591
Design and characterization of the polychromators for JT-60SA Thomson scattering systems
D’Isa F.A.; Davis S.; Fassina A.; Giudicotti L.; Manfredi M.; Montagnani G.; Nigro A.; Palombi L.; Ricciarini S.; Tojo H.; Verrecchia M.; Pasqualotto R.
English
Italiano