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Magnetic tubes in overshooting compressible convection

  • Part I Convectin and Turbulence as the Basis of Magnetic Activity
  • Conference paper
  • First Online:
The Sun and Cool Stars: activity, magnetism, dynamos

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

Abstract

A magnetic tube is introduced into turbulent compressible penetrative convection. After being strongly advected, most of the magnetic flux is stored in the overshoot region. With rotation there are meridional travelling waves.

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References

  • Brandenburg, A., Nordlund, Å., Pulkkinen, P., Stein, R.F., Tuominen, I.: 1990, Astron. Astrophys. 232, 277

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  • Hurlburt, N.E., Toomre, J., Massaguer, J.M.: 1986, Astrophys. J. 311, 563

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Authors and Affiliations

  1. D.A.M.T.P., Silver St., CB3 9EW, Cambridge, UK

    R. L. Jennings

  2. Observatory and Astrophysics Laboratory, University of Helsinki, Finland

    A. Brandenburg & I. Tuominen

  3. Copenhagen University Observatory, DK-1350, Copenhagen K, Denmark

    Å. Nordlund

  4. Department of Physics and Astronomy, Michigan State University, USA

    R. F. Stein

Authors
  1. R. L. Jennings
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  2. A. Brandenburg
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  3. Å. Nordlund
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  4. R. F. Stein
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  5. I. Tuominen
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Editor information

I. Tuominen D. Moss G. Rüdiger

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© 1991 Springer-Verlag

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Jennings, R.L., Brandenburg, A., Nordlund, Å., Stein, R.F., Tuominen, I. (1991). Magnetic tubes in overshooting compressible 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_111

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  • DOI: https://doi.org/10.1007/3-540-53955-7_111

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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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