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Stellar Turbulence pp 51–52Cite as

Observed solar spectral line asymmetries and wavelength shifts due to convection

  • 1. The Physical Origin of Turbulence
  • Conference paper
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Part of the book series: Lecture Notes in Physics ((LNP,volume 114))

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  1. S-222 24, Lund, Sweden

    Dainis Dravins

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  1. Dainis Dravins
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David F. Gray Jeffery L. Linsky

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© 1980 Springer-Verlag

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Dravins, D. (1980). Observed solar spectral line asymmetries and wavelength shifts due to convection. In: Gray, D.F., Linsky, J.L. (eds) Stellar Turbulence. Lecture Notes in Physics, vol 114. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-09737-6_10

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  • DOI: https://doi.org/10.1007/3-540-09737-6_10

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-09737-2

  • Online ISBN: 978-3-540-38554-7

  • eBook Packages: Springer Book Archive

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