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Fine Structures of Magnetic Field in Solar Quiet Region

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Abstract

In this paper, we present a time series of Fe i λ5250.2 Å photospheric filtergrams and corresponding magnetograms in a quiet region. The relationship between fine structures of granulation and magnetic fields is analyzed. It is found that although most bright filigree features in photospheric filtergrams are related to corresponding magnetic features, they are generally not cospatial. It is also found that some bright features and their corresponding photospheric magnetic fields show fast changes within several minutes.

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Authors and Affiliations

  1. Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing, 100080, China

    H. Zhang

  2. Stockholm Observatory, S-13336, Saltsjöbaden, Sweden

    G. Scharmer & M. Lofdahl

  3. Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, N-0315, Oslo 3, Norway

    Z. Yi

Authors
  1. H. Zhang
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  2. G. Scharmer
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  3. M. Lofdahl
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  4. Z. Yi
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Zhang, H., Scharmer, G., Lofdahl, M. et al. Fine Structures of Magnetic Field in Solar Quiet Region. Solar Physics 183, 283–290 (1998). https://doi.org/10.1023/A:1005007828403

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  • DOI: https://doi.org/10.1023/A:1005007828403

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