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Spectral line shapes in low frequency turbulent tokamak plasmas

Plasma Physics · Submitted 15 Dec 2004

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Turbulent fluctuations are found to affect line shapes through both the spatial and time averages introduced by the measurement process.

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arXiv IDphysics/0412091 (version 1)
Pith IDADVVZ2MM, Pith's permanent record of this paper and its review
CitationH. Capes, L. Godbert-Mouret, M. Koubiti, R. Stamm, Y. Marandet. "Spectral line shapes in low frequency turbulent tokamak plasmas." arXiv:physics/0412091 (2004). https://pith.science/paper/ADVVZ2MM
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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,804 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.25 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.10 · compares with prior results 0.08 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

In this paper we investigate the influence of low frequency turbulence on Doppler spectral line shapes in magnetized plasmas. Low frequency refers here to fluctuations whose typical time scale is much larger than those characterizing the atomic processes, such as radiative decay, collisions and charge exchange. This ordering is in particular relevant for drift wave turbulence, ubiquitous in edge plasmas of fusion devices. Turbulent fluctuations are found to affect line shapes through both the spatial and time averages introduced by the measurement process. The profile is expressed in terms of the fluid fields describing the plasma. Assuming the spectrometer acquisition time to be much larger than the turbulent time scale, an ordering generally fulfilled in experiments, allows to develop a statistical formalism. We proceed by investigating the effects of density, fluid velocity and temperature fluctuations alone on the Doppler profile of a spectral line emitted by a charge exchange population of neutrals. Line wings are found to be affected by ion temperature or fluid velocity fluctuations, and can in some cases exhibit a power-law behavior. This study gives some insights in the appearance of non-Boltzmann statistics, such as Levy statistics, when dealing with averaged experimental data.

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What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 In this paper we investigate the influence of low frequency turbulence on Doppler spectral line shapes in magnetized plasmas. contribution 0.99 0.82 0.05 asserted 0.52
s1 Low frequency refers here to fluctuations whose typical time scale is much larger than those characterizing the atomic processes, such as radiative decay, collisions and charge exchange. background 0.96 0.17 0.03 asserted 0.99
s2 This ordering is in particular relevant for drift wave turbulence, ubiquitous in edge plasmas of fusion devices. background 1.00 0.10 0.02 asserted 0.96
s3 Turbulent fluctuations are found to affect line shapes through both the spatial and time averages introduced by the measurement process. result 0.97 0.89 0.30 asserted 1.00
s4 The profile is expressed in terms of the fluid fields describing the plasma. method 0.86 0.76 0.05 asserted 1.00
s5 Assuming the spectrometer acquisition time to be much larger than the turbulent time scale, an ordering generally fulfilled in experiments, allows to develop a statistical formalism. method 0.99 0.48 0.04 asserted 0.87
s6 We proceed by investigating the effects of density, fluid velocity and temperature fluctuations alone on the Doppler profile of a spectral line emitted by a charge exchange population of neutrals. contribution 0.60 0.88 0.06 asserted 0.79
s7 Line wings are found to be affected by ion temperature or fluid velocity fluctuations, and can in some cases exhibit a power-law behavior. result 1.00 0.92 0.29 asserted 0.91
s8 This study gives some insights in the appearance of non-Boltzmann statistics, such as Levy statistics, when dealing with averaged experimental data. interpretation 0.99 0.78 0.31 hedged possibility 0.94

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.98.

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The paper
Original abstract

In this paper we investigate the influence of low frequency turbulence on Doppler spectral line shapes in magnetized plasmas. Low frequency refers here to fluctuations whose typical time scale is much larger than those characterizing the atomic processes, such as radiative decay, collisions and charge exchange. This ordering is in particular relevant for drift wave turbulence, ubiquitous in edge plasmas of fusion devices. Turbulent fluctuations are found to affect line shapes through both the spatial and time averages introduced by the measurement process. The profile is expressed in terms of the fluid fields describing the plasma. Assuming the spectrometer acquisition time to be much larger than the turbulent time scale, an ordering generally fulfilled in experiments, allows to develop a statistical formalism. We proceed by investigating the effects of density, fluid velocity and temperature fluctuations alone on the Doppler profile of a spectral line emitted by a charge exchange population of neutrals. Line wings are found to be affected by ion temperature or fluid velocity fluctuations, and can in some cases exhibit a power-law behavior. This study gives some insights in the appearance of non-Boltzmann statistics, such as Levy statistics, when dealing with averaged experimental data.

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