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Differential rotation as an axisymmetric resonant mode of convection

  • Part III Solar magnetism and large-scale flows
  • Conference paper
  • First Online:
The Sun and Cool Stars: activity, magnetism, dynamos

Part of the book series: Lecture Notes in Physics ((LNP,volume 380))

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References

  • Belvedere, G., Paternò, L.: 1977, Solar Phys. 54, 289

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  • Chan, K.L., Sofia, S., Mayr, H.G.: 1987, In The internal solar angular velocity, eds. B.R. Durney and S. Sofia, Reidel, Dordrecht, p. 347

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  • Durney, B.R., Roxburgh, I.W.: 1971, Solar Phys. 16, 3

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  • Dziembowski, W.A., Goode, P.R., Libbrecht, K.G.: 1989, Astrophys. J. 336, 53

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  • Rüdiger, G.: 1989, Differential rotation and stellar convection: Sun and solar-type stars, Gordon and Breach, New York

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  • Weiss, N.O.: 1965, Observatory 85, 37

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Author information

Authors and Affiliations

  1. Applied Research Corporation, Landover, MD, USA

    Kwing L. Chan

  2. Goddard Space Flight Center, Greenbelt, MD, USA

    Hans G. Mayr

Authors
  1. Kwing L. Chan
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  2. Hans G. Mayr
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Editor information

I. Tuominen D. Moss G. Rüdiger

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© 1991 Springer-Verlag

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Chan, K.L., Mayr, H.G. (1991). Differential rotation as an axisymmetric resonant mode of convection. In: Tuominen, I., Moss, D., Rüdiger, G. (eds) The Sun and Cool Stars: activity, magnetism, dynamos. Lecture Notes in Physics, vol 380. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53955-7_124

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  • DOI: https://doi.org/10.1007/3-540-53955-7_124

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-53955-1

  • Online ISBN: 978-3-540-46483-9

  • eBook Packages: Springer Book Archive

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