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Correlations of magnetic features and the torsional pattern

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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J. Muraközy, A. Ludmány

Solar and Stellar Astrophysics · Submitted 9 Jan 2014

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

The authors' main claim The bulges of the sunspot number and area distributions tend to be loacted within the 'forward' belts close to their poleward shearing borders.

how it is stated · asserted 0.71 read the record →

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arXiv ID1401.2078 (version 1)
Pith IDUSYXEKWW, Pith's permanent record of this paper and its review
CitationA. Ludm\'any, J. Murak\"ozy. "Correlations of magnetic features and the torsional pattern." arXiv:1401.2078 (2014). https://pith.science/paper/USYXEKWW
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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-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,268 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.10 · compares with prior results 0.16 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

The striking similarity between the cyclic equatorward migration of the torsional oscillation belts and the sunspot activity latitudes inspired several attempts to seek an explanation of the torsional phenomenon in terms of interactions between flux ropes and plasma motions. The aim of the present work is to examine the spatial and temporal coincidences of the torsional waves and the emergence of sunspot magnetic fields. The locations of the shearing latitudes have been compared with the distributions of certain sunspot parameters by using sunspot data of more than two cycles. The bulges of the sunspot number and area distributions tend to be loacted within the 'forward' belts close to their poleward shearing borders. A possible geometry of the magnetic and velocity field interacion is proposed.

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 striking similarity between the cyclic equatorward migration of the torsional oscillation belts and the sunspot activity latitudes inspired several attempts to seek an explanation of the torsional phenomenon in terms of interactions between flux ropes and plasma motions. background 1.00 0.06 0.04 asserted 0.99
s1 The aim of the present work is to examine the spatial and temporal coincidences of the torsional waves and the emergence of sunspot magnetic fields. contribution 1.00 0.58 0.04 asserted 0.58
s2 The locations of the shearing latitudes have been compared with the distributions of certain sunspot parameters by using sunspot data of more than two cycles. method 0.98 0.90 0.04 asserted 0.96
s3 The bulges of the sunspot number and area distributions tend to be loacted within the 'forward' belts close to their poleward shearing borders. result 1.00 0.84 0.59 asserted 0.71
s4 A possible geometry of the magnetic and velocity field interacion is proposed. interpretation 0.75 0.81 0.14 hedged possibility 0.94

What kind of paper the classifier reports this is: empirical study 1.00 · evidence from analysis of existing data 1.00.

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
not run
  • 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 striking similarity between the cyclic equatorward migration of the torsional oscillation belts and the sunspot activity latitudes inspired several attempts to seek an explanation of the torsional phenomenon in terms of interactions between flux ropes and plasma motions. The aim of the present work is to examine the spatial and temporal coincidences of the torsional waves and the emergence of sunspot magnetic fields. The locations of the shearing latitudes have been compared with the distributions of certain sunspot parameters by using sunspot data of more than two cycles. The bulges of the sunspot number and area distributions tend to be loacted within the 'forward' belts close to their poleward shearing borders. A possible geometry of the magnetic and velocity field interacion is proposed.

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