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Chromospheric and coronal activities in the quiet sun originating from photospheric 5-minute oscillations

  • VII. Global Coronal Structure and Solar Activity
  • Conference paper
  • First Online:
Flare Physics in Solar Activity Maximum 22

Part of the book series: Lecture Notes in Physics ((LNP,volume 387))

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Abstract

We numerically investigated the non-linear response of the solar atmosphere to 5-min oscillations, assuming that atmospheric motions are restricted to flow along magnetic field lines. It was found that 5-min oscillations can generate shock waves along magnetic field lines with inclination angles of about 50 degrees from vertical in the chromosphere. It is suggested that coronal activities driven by the shock waves might be observable with the Soft X-ray Telescope on board Solar-A.

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Author information

Authors and Affiliations

  1. National Astronomical Observatory, Mitaka, 181, Tokyo, Japan

    Yoshinori Suematsu

  2. Department of Electric Engineering, Yonago National College of Technology, 4448 Hikona, Yonago, 683, Tottori, Japan

    Akitsugu Takeuchi

Authors
  1. Yoshinori Suematsu
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  2. Akitsugu Takeuchi
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Editor information

Yutaka Uchida Richard C. Canfield Tetsuya Watanabe Eijiro Hiei

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© 1991 Springer-Verlag

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Suematsu, Y., Takeuchi, A. (1991). Chromospheric and coronal activities in the quiet sun originating from photospheric 5-minute oscillations. In: Uchida, Y., Canfield, R.C., Watanabe, T., Hiei, E. (eds) Flare Physics in Solar Activity Maximum 22. Lecture Notes in Physics, vol 387. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0032647

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  • DOI: https://doi.org/10.1007/BFb0032647

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-54383-1

  • Online ISBN: 978-3-540-47596-5

  • eBook Packages: Springer Book Archive

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