Stark-broadened hydrogen line profiles predicted by the model microfield method for calculating electron number densities

Citation
Bw. Acon et al., Stark-broadened hydrogen line profiles predicted by the model microfield method for calculating electron number densities, SPECT ACT B, 56(5), 2001, pp. 527-539
Citations number
54
Categorie Soggetti
Spectroscopy /Instrumentation/Analytical Sciences
Journal title
SPECTROCHIMICA ACTA PART B-ATOMIC SPECTROSCOPY
ISSN journal
05848547 → ACNP
Volume
56
Issue
5
Year of publication
2001
Pages
527 - 539
Database
ISI
SICI code
0584-8547(20010531)56:5<527:SHLPPB>2.0.ZU;2-C
Abstract
This report is the first account on the application of theoretical Stark-br oadening profiles predicted by the model microfield method (MMM) to estimat e electron number density (n(e)) in several laboratory plasmas. The determi nation of n(e) is accomplished by least-squares fitting of the entire emiss ion profile or the wing portions of the emission profile of the H-beta line (486.13 nm) to the theoretical Stark-broadened profiles. Experimental prof iles obtained for the H-beta line from argon and helium inductively coupled plasmas (ICP), a glow discharge, and a high-voltage spark are used to test the new MMM profiles. Results are contrasted with data predicted by the tr aditional 'Unified Theory'. Compared to the 'Unified Theory', the MMM profi les are more accurate in the line center and span over a wide range of temp erature (2500-80000 K) and electron number densities (1 x 10(10)-1 x 10(17) cm(-3)). (C) 2001 Elsevier Science B.V. All rights reserved.