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Triple-Dipole Model on the Large-Scale Magnetic Structure of the Sun

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Magnetodynamic Phenomena in the Solar Atmosphere

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Abstract

It is necessary from a viewpoint of solar-terrestrial physics to study complex heliomagnetospheric structure and its solar cycle variation. The purpose of the present paper is to investigate large-scale structure of the solar magnetic fields, especially in relation to high-latitude prominences.

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Reference

  • Hara, H. (1995) Activity of high-latitude corona associated with low-latitude corona, Abstract of the spring meeting of Japanese Astronomical Society of Japan, S09w.

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Author information

Authors and Affiliations

  1. Tohoku U, Japan

    T. Saito (Emer. Prof)

  2. STE Lab, Nagoya Univ, Japan

    Y. Kozuka & M. Kojima

  3. Miyagi Univ. Education, Japan

    Y. Mori, M. Yasue & Y. Matsuura

Authors
  1. T. Saito
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  2. Y. Kozuka
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  3. M. Kojima
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  4. Y. Mori
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  5. M. Yasue
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  6. Y. Matsuura
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Editor information

Editors and Affiliations

  1. Science University of Tokyo, Japan

    Yutaka Uchida

  2. National Astronomical Observatory, Tokyo, Japan

    Takeo Kosugi

  3. University of Hawaii, Honolulu, HI, USA

    Hugh S. Hudson

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© 1996 Kluwer Academic Publishers

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Saito, T., Kozuka, Y., Kojima, M., Mori, Y., Yasue, M., Matsuura, Y. (1996). Triple-Dipole Model on the Large-Scale Magnetic Structure of the Sun. In: Uchida, Y., Kosugi, T., Hudson, H.S. (eds) Magnetodynamic Phenomena in the Solar Atmosphere. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0315-9_169

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  • DOI: https://doi.org/10.1007/978-94-009-0315-9_169

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6627-3

  • Online ISBN: 978-94-009-0315-9

  • eBook Packages: Springer Book Archive

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