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Author Correction: Ultra-high-resolution observations of persistent null-point reconnection in the solar corona

Author

Listed:
  • X. Cheng

    (Nanjing University
    Max Planck Institute for Solar System Research
    Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education)

  • E. R. Priest

    (University of St. Andrews)

  • H. T. Li

    (Nanjing University
    Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education)

  • J. Chen

    (Nanjing University
    Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education)

  • G. Aulanier

    (Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP)
    Rosseland Centre for Solar Physics, Institute for Theoretical Astrophysics, Universitetet i Oslo)

  • L. P. Chitta

    (Max Planck Institute for Solar System Research)

  • Y. L. Wang

    (Nanjing University
    Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education)

  • H. Peter

    (Max Planck Institute for Solar System Research)

  • X. S. Zhu

    (Chinese Academy of Sciences)

  • C. Xing

    (Nanjing University
    Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP))

  • M. D. Ding

    (Nanjing University
    Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education)

  • S. K. Solanki

    (Max Planck Institute for Solar System Research)

  • D. Berghmans

    (Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium)

  • L. Teriaca

    (Max Planck Institute for Solar System Research)

  • R. Aznar Cuadrado

    (Max Planck Institute for Solar System Research)

  • A. N. Zhukov

    (Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium
    Skobeltsyn Institute of Nuclear Physics, Moscow State University)

  • Y. Guo

    (Nanjing University
    Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education)

  • D. Long

    (Mullard Space Science Laboratory, University College London)

  • L. Harra

    (PMOD/WRC
    ETH-Zürich)

  • P. J. Smith

    (Mullard Space Science Laboratory, University College London)

  • L. Rodriguez

    (Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium)

  • C. Verbeeck

    (Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium)

  • K. Barczynski

    (ETH-Zürich)

  • S. Parenti

    (Institut d’Astrophysique Spatiale, Université Paris-Saclay)

Abstract

No abstract is available for this item.

Suggested Citation

  • X. Cheng & E. R. Priest & H. T. Li & J. Chen & G. Aulanier & L. P. Chitta & Y. L. Wang & H. Peter & X. S. Zhu & C. Xing & M. D. Ding & S. K. Solanki & D. Berghmans & L. Teriaca & R. Aznar Cuadrado & A, 2023. "Author Correction: Ultra-high-resolution observations of persistent null-point reconnection in the solar corona," Nature Communications, Nature, vol. 14(1), pages 1-1, December.
    • Handle: RePEc:nat:natcom:v:14:y:2023:i:1:d:10.1038_s41467-023-38149-6
    DOI: 10.1038/s41467-023-38149-6
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