Modeling of Stark-Broadened Lines in a Fluctuating Edge Plasma

被引:4
|
作者
Rosato, J. [1 ]
Marandet, Y. [1 ]
Peiffer, A. [1 ]
Capes, H. [1 ]
Godbert-Mouret, L. [1 ]
Koubiti, M. [1 ]
Stamm, R. [1 ]
机构
[1] Aix Marseille Univ, CNRS, PIIM UMR 7345, F-13397 Marseille 20, France
关键词
Spectroscopy; turbulence; plasma diagnostic; SHAPES;
D O I
10.1002/ctpp.201410045
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
A line shape model that accounts for low-frequency fluctuations is applied to the Balmer series of the hydrogen isotopes (atomic transitions n -> 2). The plasma fluid parameters (density, temperature, etc.) are described as random variables characterized by a prescribed joint probability density function. A special emphasis is devoted to Stark broadened lines, which are sensitive to the plasma density. It is shown that fluctuations can lead to a significant increase of the line width if the fluctuation level Delta N-e/< N-e > (with < N-e > and Delta N-e being respectively the density averaged along the line-of-sight and its RMS value) is large. (C) 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
引用
收藏
页码:565 / 569
页数:5
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