Published April 4, 2001 | Version v1
Journal article

Stark broadening of N I, O I, N II, O II spectral lines for modelling the radiative transfer in thermal air plasmas

  • 1. Laboratoire EM2C UPR 288, CNRS and Ecole Centrale Paris, 92295 CHATENAY-MALABRY (France)

Description

Electron and ion Stark broadening parameters (widths and shifts) for all the lines of N I, O I, N II, and O II listed in the NIST database have been calculated following the semi-classical approach by Sahal-Brechot [Astron. and Astrophys. 1, 91 (1969)]. Calculations have been carried out systematically for air mixture plasmas in the temperature range 2 000 K-25 000 K under the assumption of chemical equilibrium at atmospheric pressure

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
559
Journal Issue
1
Journal Page Range
p. 166-168
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
15. ICSLS international conference on spectral line shapes
Dates
10-14 Jul 2000
Place
Berlin (Germany)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
35051620
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
ELECTRON TEMPERATURE; ELECTRONS; EXPERIMENTAL DATA; ION TEMPERATURE; LINE BROADENING; LINE WIDTHS; NITROGEN IONS; OXYGEN IONS; PLASMA; SEMICLASSICAL APPROXIMATION; STARK EFFECT
Descriptors DEC
CHARGED PARTICLES; DATA; ELEMENTARY PARTICLES; FERMIONS; INFORMATION; IONS; LEPTONS; NUMERICAL DATA

Optional Information

Notes
(c) 2001 American Institute of Physics.