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Convection And Its Stability In The Equatorial Regions Of The Convection Zone

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Solar Photosphere: Structure, Convection, and Magnetic Fields

Part of the book series: International Astronomical Union ((IAUS,volume 138))

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Abstract

The problem of the existence, evolution, and stability of spatial structures in convection is of considerable importance to astrophysics as well as to geophysical hydrodynamics. The Boussinesq approximation will be used because the considered motions in stars are sufficiently slow.

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References

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© 1990 International Astronomical Union

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Klyachkin, A.V. (1990). Convection And Its Stability In The Equatorial Regions Of The Convection Zone. In: Stenflo, J.O. (eds) Solar Photosphere: Structure, Convection, and Magnetic Fields. International Astronomical Union, vol 138. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1061-4_36

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  • DOI: https://doi.org/10.1007/978-94-009-1061-4_36

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-0530-9

  • Online ISBN: 978-94-009-1061-4

  • eBook Packages: Springer Book Archive

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