Erratum

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

Shravan Hanasoge

    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

    Fingerprint

    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

    @article{2c9326633d4c4e4e8e054e8cd74bfe6d,
    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",

    }

    TY - JOUR

    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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    UR - http://www.scopus.com/inward/citedby.url?scp=85030545946&partnerID=8YFLogxK

    U2 - 10.1093/mnras/stx2214

    DO - 10.1093/mnras/stx2214

    M3 - Comment/debate

    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 -