Erratum: Seismic sensitivity of Normal-mode Coupling to Lorentz stresses in the Sun [MNRAS, 470, 3, (2017), (2780-2790)] DOI: 10.1093/mnras/stx1342

Research output: Contribution to journalComment/debate

Abstract

The symbol er has been mistakenly replaced by Br in numerous instances in section 2 and appendix E. Since both er and Br are used frequently in paper and because they refer to very different quantities (er denotes the unit vector in the radial direction and Br the radial component of the magnetic field), the potential for misinterpretation is significant. Here we reproduce accurate versions of section 2 and appendix E of the manuscript (also see arxiv 1705.09431 for instance).

Original languageEnglish (US)
Pages (from-to)2764-2767
Number of pages4
JournalMonthly Notices of the Royal Astronomical Society
Volume472
Issue number3
DOIs
StatePublished - Jan 1 2017

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coupled modes
sun
magnetic field
sensitivity
magnetic fields

Keywords

  • Hydrodynamics
  • Sun: helioseismology
  • Sun: interior
  • Sun: oscillations
  • waves

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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title = "Erratum: Seismic sensitivity of Normal-mode Coupling to Lorentz stresses in the Sun [MNRAS, 470, 3, (2017), (2780-2790)] DOI: 10.1093/mnras/stx1342",
abstract = "The symbol er has been mistakenly replaced by Br in numerous instances in section 2 and appendix E. Since both er and Br are used frequently in paper and because they refer to very different quantities (er denotes the unit vector in the radial direction and Br the radial component of the magnetic field), the potential for misinterpretation is significant. Here we reproduce accurate versions of section 2 and appendix E of the manuscript (also see arxiv 1705.09431 for instance).",
keywords = "Hydrodynamics, Sun: helioseismology, Sun: interior, Sun: oscillations, waves",
author = "Shravan Hanasoge",
year = "2017",
month = "1",
day = "1",
doi = "10.1093/mnras/stx2214",
language = "English (US)",
volume = "472",
pages = "2764--2767",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "3",

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T1 - Erratum

T2 - Seismic sensitivity of Normal-mode Coupling to Lorentz stresses in the Sun [MNRAS, 470, 3, (2017), (2780-2790)] DOI: 10.1093/mnras/stx1342

AU - Hanasoge, Shravan

PY - 2017/1/1

Y1 - 2017/1/1

N2 - The symbol er has been mistakenly replaced by Br in numerous instances in section 2 and appendix E. Since both er and Br are used frequently in paper and because they refer to very different quantities (er denotes the unit vector in the radial direction and Br the radial component of the magnetic field), the potential for misinterpretation is significant. Here we reproduce accurate versions of section 2 and appendix E of the manuscript (also see arxiv 1705.09431 for instance).

AB - The symbol er has been mistakenly replaced by Br in numerous instances in section 2 and appendix E. Since both er and Br are used frequently in paper and because they refer to very different quantities (er denotes the unit vector in the radial direction and Br the radial component of the magnetic field), the potential for misinterpretation is significant. Here we reproduce accurate versions of section 2 and appendix E of the manuscript (also see arxiv 1705.09431 for instance).

KW - Hydrodynamics

KW - Sun: helioseismology

KW - Sun: interior

KW - Sun: oscillations

KW - waves

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U2 - 10.1093/mnras/stx2214

DO - 10.1093/mnras/stx2214

M3 - Comment/debate

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VL - 472

SP - 2764

EP - 2767

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -