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The large-scale magnetic field in the global solar cycle: observational aspects

  • 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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Abstract

The global solar cycle is considered as an interaction of 3 types of activity: at low-latitude (sunspots), at high-latitude (polar faculae) and the weak magnetic field. The properties of single and 3-fold reversals of the polar magnetic field are considered. The variation spectrum of the large-scale magnetic field of the Sun is analyzed in the range of 1-30 nHz. A dependence between the rate of a poleward meridional flow and phase of the global cycle is discussed.

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Author information

Authors and Affiliations

  1. Kislovodsk Solar Station, 357741, Kislovodsk, USSR

    V. I. Makarov

  2. Indian Institute of Astrophysics, 560034, Bangalore, India

    K. R. Sivaraman

Authors
  1. V. I. Makarov
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  2. K. R. Sivaraman
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Editor information

I. Tuominen D. Moss G. Rüdiger

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© 1991 Springer-Verlag

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Makarov, V.I., Sivaraman, K.R. (1991). The large-scale magnetic field in the global solar cycle: observational aspects. 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_129

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  • DOI: https://doi.org/10.1007/3-540-53955-7_129

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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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