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

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. N. Zhukov, Y. Guo, D. Long, L. Harra, P. J. Smith, L. Rodriguez, C. Verbeeck, K. Barczynski and S. Parenti
Additional contact information
X. Cheng: Nanjing University
E. R. Priest: University of St. Andrews
H. T. Li: Nanjing University
J. Chen: Nanjing University
G. Aulanier: Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP)
L. P. Chitta: Max Planck Institute for Solar System Research
Y. L. Wang: Nanjing University
H. Peter: Max Planck Institute for Solar System Research
X. S. Zhu: Chinese Academy of Sciences
C. Xing: Nanjing University
M. D. Ding: Nanjing University
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
Y. Guo: Nanjing University
D. Long: Mullard Space Science Laboratory, University College London
L. Harra: PMOD/WRC
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

Nature Communications, 2023, vol. 14, issue 1, 1-1

Date: 2023
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DOI: 10.1038/s41467-023-38149-6

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