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Diamagnetic current does not produce an instability in the solar corona - MaRDI portal

Diamagnetic current does not produce an instability in the solar corona (Q3639195)

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Diamagnetic current does not produce an instability in the solar corona
scientific article

    Statements

    title
    Diamagnetic current does not produce an instability in the solar corona (English)
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    author
    J. Vranješ
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    Stefaan Poedts
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    publication date
    29 October 2009
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    zbMATH Keywords
    Sun: corona
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    waves
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    instabilities
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    Identifiers

    zbMATH DE Number
    5622865
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    OpenAlex ID
    W2112449393
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    Wikidata QID
    Q60722965
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