Large-Scale Internal Magnetic Field of the Sun

  • A. E. Dudorov
  • V. N. Krivodubskij
  • A. A. Ruzmaikin
  • T. V. Ruzmaikina
Conference paper
Part of the International Astronomical Union book series (IAUS, volume 138)

Abstract

The behaviour of the magnetic field during the formation and evolution of the Sun is investigated. It is shown that an internal poloidal magnetic field of the order of 104 – 105 G near the core of the Sun may be compatible with differential rotation and with torsional waves, travelling along the magnetic field lines (Dudorov et al., 1989).

Keywords

Magnetic Field Line Convection Zone Differential Rotation Toroidal Magnetic Field Torsional Wave 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© International Astronomical Union 1990

Authors and Affiliations

  • A. E. Dudorov
    • 1
  • V. N. Krivodubskij
    • 2
  • A. A. Ruzmaikin
    • 3
  • T. V. Ruzmaikina
    • 4
  1. 1.Astronomy Department of Moscow State UniversityMoscowUSSR
  2. 2.Kiev Shevchenko University Astronomical ObservatoryKievUSSR
  3. 3.IZMIRANTroitsk, Moscow regionUSSR
  4. 4.Institute of Physics of EarthMoscowUSSR

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