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Influence of Random Irregularities on Quasi-Thermal Noise Spectrum of Plasma

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N. A. Zabotin, Yu. V. Chugunov, E. A. Mareev, A. G. Bronin

Plasma Physics · Submitted 11 Apr 2000

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

The authors' main claim Presence of random irregularities change dispersion law in plasma what cause the change in the shape of quasi-thermal noise spectrum.

how it is stated · asserted 1.00 read the record →

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arXiv IDphysics/0004021 (version 2)
Pith ID4YIMGFQN, Pith's permanent record of this paper and its review
CitationA. G. Bronin, E. A. Mareev, N. A. Zabotin, Yu. V. Chugunov. "Influence of Random Irregularities on Quasi-Thermal Noise Spectrum of Plasma." arXiv:physics/0004021 (2000). https://pith.science/paper/4YIMGFQN
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,535 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.36 · randomized assignment 0.02 · states quantitative result 0.06 · compares with prior results 0.15 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

The influence of random irregularities of electron density on quasi-thermal noise spectra in plasma is considered in the paper. Quasi-thermal noise spectrum of plasma in state near the thermal equilibrium is determined by effective dielectric constant tensor. Presence of random irregularities change dispersion law in plasma what cause the change in the shape of quasi-thermal noise spectrum. Numerical estimation of noise spectra are fulfilled for both conditions of ionospheric and solar wind plasma.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The influence of random irregularities of electron density on quasi-thermal noise spectra in plasma is considered in the paper. contribution 0.84 0.66 0.09 asserted 0.84
s1 Quasi-thermal noise spectrum of plasma in state near the thermal equilibrium is determined by effective dielectric constant tensor. background 1.00 0.18 0.07 asserted 1.00
s2 Presence of random irregularities change dispersion law in plasma what cause the change in the shape of quasi-thermal noise spectrum. result 0.54 0.54 0.69 asserted 1.00
s3 Numerical estimation of noise spectra are fulfilled for both conditions of ionospheric and solar wind plasma. method 0.44 0.91 0.09 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.58 · evidence from simulation or computation 0.97.

What was examined, and what was not

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  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
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  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

The influence of random irregularities of electron density on quasi-thermal noise spectra in plasma is considered in the paper. Quasi-thermal noise spectrum of plasma in state near the thermal equilibrium is determined by effective dielectric constant tensor. Presence of random irregularities change dispersion law in plasma what cause the change in the shape of quasi-thermal noise spectrum. Numerical estimation of noise spectra are fulfilled for both conditions of ionospheric and solar wind plasma.

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