Construction of solar-wind-like magnetic fields.

Physical review letters · 2012 · Unclear · Insufficient evidence

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UnclearInsufficient evidencePaper 3180

Study snapshot

PublicationPhysical review letters · 2012

Study typeengineering

Reported directionUnclear

Evidence ratingInsufficient

Abstract

Fluctuations in the solar wind fields tend to not only have velocities and magnetic fields correlated in the sense consistent with Alfvén waves traveling from the Sun, but they also have the magnitude of the magnetic field remarkably constant despite their being broadband. This Letter provides, for the first time, a method for constructing fields with nearly constant magnetic field, zero divergence, and with any specified power spectrum for the fluctuations of the components of the field. Every wave vector, k, is associated with two polarizations; the relative phases of these can be chosen to minimize the variance of the field magnitude while retaining the "random" character of the fields. The method is applied to a case with one spatial coordinate that demonstrates good agreement with observed time series and power spectra of the magnetic field in the solar wind, as well as with the distribution of the angles of rapid changes ("discontinuities"), thus showing a deep connection between two seemingly unrelated issues. It is suggested that using this construction will lead to more realistic simulations of solar wind turbulence and of the propagation of energetic particles.

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AI evidence extraction

Structured fields below were generated from the paper’s abstract and metadata to make the evidence easier to inspect. Automated extraction may be incomplete or incorrect; verify important details against the original paper.

Study typeengineering

Effect directionunclear

PopulationNot supplied

Sample sizeNot supplied

ExposureNot supplied

Evidence strengthInsufficientConfidence: 74% · Peer reviewed: yes

Main findings

The paper presents a method to construct magnetic fields with nearly constant magnitude, zero divergence, and an arbitrary specified power spectrum for component fluctuations by choosing relative phases of two polarizations per wave vector to minimize variance in field magnitude. Applied in a one-spatial-coordinate case, the constructed fields show good agreement with observed solar-wind magnetic-field time series, power spectra, and the distribution of discontinuity angles.

Outcomes measured

Method for constructing magnetic fields with nearly constant magnitude
Zero-divergence magnetic field construction
Ability to specify any power spectrum for component fluctuations
Agreement with observed solar wind magnetic-field time series and power spectra
Agreement with distribution of angles of rapid changes ("discontinuities")

Limitations

No health/biological outcomes assessed
No exposure metrics (frequency, field strength, SAR, duration) reported in the abstract
Application described for a case with one spatial coordinate

View raw extracted JSON

{
  "study_type": "engineering",
  "exposure": {
    "band": null,
    "source": null,
    "frequency_mhz": null,
    "sar_wkg": null,
    "duration": null
  },
  "population": null,
  "sample_size": null,
  "outcomes": [
    "Method for constructing magnetic fields with nearly constant magnitude",
    "Zero-divergence magnetic field construction",
    "Ability to specify any power spectrum for component fluctuations",
    "Agreement with observed solar wind magnetic-field time series and power spectra",
    "Agreement with distribution of angles of rapid changes (\"discontinuities\")"
  ],
  "main_findings": "The paper presents a method to construct magnetic fields with nearly constant magnitude, zero divergence, and an arbitrary specified power spectrum for component fluctuations by choosing relative phases of two polarizations per wave vector to minimize variance in field magnitude. Applied in a one-spatial-coordinate case, the constructed fields show good agreement with observed solar-wind magnetic-field time series, power spectra, and the distribution of discontinuity angles.",
  "effect_direction": "unclear",
  "limitations": [
    "No health/biological outcomes assessed",
    "No exposure metrics (frequency, field strength, SAR, duration) reported in the abstract",
    "Application described for a case with one spatial coordinate"
  ],
  "evidence_strength": "insufficient",
  "confidence": 0.74,
  "peer_reviewed_likely": "yes",
  "keywords": [
    "solar wind",
    "magnetic fields",
    "Alfvén waves",
    "turbulence",
    "power spectrum",
    "zero divergence",
    "field construction",
    "discontinuities",
    "energetic particles",
    "simulation method"
  ],
  "suggested_hubs": []
}

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AI-extracted fields are generated from the abstract and metadata and may be incomplete or incorrect. This material is for informational purposes and is not medical advice.

Identifiers and source

DOI: 10.1103/physrevlett.109.231102
PubMed: 23368180

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