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Fossil magnetic fields and activity of young stars

  • Part II Current stellar dynamo theory
  • Conference paper
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Part of the book series: Lecture Notes in Physics ((LNP,volume 380))

Abstract

The strength of fossil magnetic fields in young stars is estimated. The interaction of a fossil magnetic field with convection in stellar envelopes is investigated. The influence of such a magnetic field, transformed to a small scale, on the activity of young stars is discussed.

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References

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I. Tuominen D. Moss G. Rüdiger

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© 1991 Springer-Verlag

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Dudorov, A.E., Gorbenko, E.E. (1991). Fossil magnetic fields and activity of young stars. 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_121

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  • DOI: https://doi.org/10.1007/3-540-53955-7_121

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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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