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The Sun and Cool Stars: activity, magnetism, dynamos pp 271–274Cite as

The longer term evolution of magnetic field and mass flow in a decaying active region

  • Part III Solar magnetism and large-scale flows
  • Conference paper
  • First Online:

  • 145 Accesses

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

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Authors and Affiliations

  1. Beijing Astronomical Observatory, Chinese Academy of Sciences, P. R. China

    Hongqi Zhang & Guoxiang Ai

  2. Big Bear Solar Observatory, California Institute of Technology, USA

    Haimin Wang, Harold Zirin & Alan Patterson

Authors
  1. Hongqi Zhang
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  2. Guoxiang Ai
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  3. Haimin Wang
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  4. Harold Zirin
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  5. Alan Patterson
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Editor information

I. Tuominen D. Moss G. Rüdiger

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© 1991 Springer-Verlag

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Zhang, H., Ai, G., Wang, H., Zirin, H., Patterson, A. (1991). The longer term evolution of magnetic field and mass flow in a decaying active region. 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_139

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  • DOI: https://doi.org/10.1007/3-540-53955-7_139

  • Published:

  • 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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