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Rotation of large scale patterns on the solar surface as determined from filament and millimeter data

  • 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))

Abstract

The rotation of large scale solar magnetic field patterns was studied using quiescent filaments and low temperature regions observed at 37 GHz as tracers.

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References

  • Adams, W.M., Tang, F.: 1977, Solar Phys. 55, 499

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  • Brajša, R., Vršnak, B., Ruždjak, V., Schroll, A.: 1989,Hvar Obs. Bull. 13, 449

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  • Vršnak, B., Pohjolainen, S., Teräsranta, H., Urpo, S., Brajša, R., Ruždjak, V., Schroll, A., Jurač, S.: 1991, these Proceedings

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Authors and Affiliations

  1. Metsähovi Radio Research Station, 02540, Kylmälä, Finland

    S. Pohjolainen, H. Teräsranta & S. Urpol

  2. Hvar Observatory, 58450, Hvar, Yugoslavia

    B. Vršnak, R. Brajša, V. Ruždjak & S. Jurač

  3. Sonnenobservatorium Kanzelhöhe, 9520, Sattendorf, Austria

    A. Schroll

Authors
  1. S. Pohjolainen
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  2. B. Vršnak
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  3. H. Teräsranta
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  4. S. Urpol
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  5. R. Brajša
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  6. V. Ruždjak
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  7. S. Jurač
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  8. A. Schroll
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Editor information

I. Tuominen D. Moss G. Rüdiger

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© 1991 Springer-Verlag

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Pohjolainen, S. et al. (1991). Rotation of large scale patterns on the solar surface as determined from filament and millimeter data. 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_142

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  • DOI: https://doi.org/10.1007/3-540-53955-7_142

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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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