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Validation of heliospheric modeling algorithms through pulsar observations I: Interplanetary scintillation-based tomography

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C. Tiburzi, B. V. Jackson, L. Cota, G. M. Shaifullah, R. A. Fallows, M. Tokumaru, P. Zucca

Solar and Stellar Astrophysics · Submitted 12 Jun 2023

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

The authors' main claim This work represents a completely independent comparison and validation of these techniques to provide this measurement, and it strengthens confidence in the use of both in space-weather analyses applications.

how it is stated · asserted 0.99 read the record →

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arXiv ID2306.07451 (version 1)
Pith IDJ6CWG6GB, Pith's permanent record of this paper and its review
CitationB. V. Jackson, C. Tiburzi, G. M. Shaifullah, L. Cota, M. Tokumaru, P. Zucca, R. A. Fallows. "Validation of heliospheric modeling algorithms through pulsar observations I: Interplanetary scintillation-based tomography." arXiv:2306.07451 (2023). https://pith.science/paper/J6CWG6GB
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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, 3,024 input tokens.

What the abstract itself states, as probabilities: claims first 0.11 · states limitation 0.07 · human participants 0.02 · controlled comparison 0.26 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.96 · mentions code or data availability 0.03.

The abstract, sentence by sentence

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

Solar-wind 3-D reconstruction tomography based on interplanetary scintillation (IPS) studies provides fundamental information for space-weather forecasting models, and gives the possibility to determine heliospheric column densities. Here we compare the time series of Solar-wind column densities derived from long-term observations of pulsars, and the Solar-wind reconstruction provided by the UCSD IPS tomography. This work represents a completely independent comparison and validation of these techniques to provide this measurement, and it strengthens confidence in the use of both in space-weather analyses applications.

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 Solar-wind 3-D reconstruction tomography based on interplanetary scintillation (IPS) studies provides fundamental information for space-weather forecasting models, and gives the possibility to determine heliospheric column densities. background 1.00 0.08 0.05 asserted 0.91
s1 Here we compare the time series of Solar-wind column densities derived from long-term observations of pulsars, and the Solar-wind reconstruction provided by the UCSD IPS tomography. contribution 0.72 0.88 0.06 asserted 0.96
s2 This work represents a completely independent comparison and validation of these techniques to provide this measurement, and it strengthens confidence in the use of both in space-weather analyses applications. interpretation 0.88 0.67 0.76 asserted 0.99

What kind of paper the classifier reports this is: empirical study 0.91 · evidence from analysis of existing data 0.87.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • 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

Solar-wind 3-D reconstruction tomography based on interplanetary scintillation (IPS) studies provides fundamental information for space-weather forecasting models, and gives the possibility to determine heliospheric column densities. Here we compare the time series of Solar-wind column densities derived from long-term observations of pulsars, and the Solar-wind reconstruction provided by the UCSD IPS tomography. This work represents a completely independent comparison and validation of these techniques to provide this measurement, and it strengthens confidence in the use of both in space-weather analyses applications.

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References
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1 arXiv paper cite this in 1 sentence

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

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