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A Model of the Magnetic Field Long-Term Evolution at the Coronal Base and Polar Heliospheric Regions

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The 3-D Heliosphere at Solar Maximum
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Abstract

The long-term evolution of the polar magnetic field at the coronal base induced by the first Rossby mode demonstrates the reversal of the line-of-sight magnetic field component in polar caps and what is more the same line-of-sight magnetic polarities in both caps (“the line-of-sight solar magnetic monopole”) at the moment of reversal.

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© 2001 Springer Science+Business Media Dordrecht

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Pisanko, Y.V. (2001). A Model of the Magnetic Field Long-Term Evolution at the Coronal Base and Polar Heliospheric Regions. In: Marsden, R.G. (eds) The 3-D Heliosphere at Solar Maximum. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3230-7_27

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  • DOI: https://doi.org/10.1007/978-94-017-3230-7_27

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5723-5

  • Online ISBN: 978-94-017-3230-7

  • eBook Packages: Springer Book Archive

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