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Author Correction: Ultra-high-resolution observations of persistent null-point reconnection in the solar corona.
Cheng, X; Priest, E R; Li, H T; Chen, J; Aulanier, G; Chitta, L P; Wang, Y L; Peter, H; Zhu, X S; Xing, C; Ding, M D; Solanki, S K; Berghmans, D; Teriaca, L; Aznar Cuadrado, R; Zhukov, A N; Guo, Y; Long, D; Harra, L; Smith, P J; Rodriguez, L; Verbeeck, C; Barczynski, K; Parenti, S.
Afiliación
  • Cheng X; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China. xincheng@nju.edu.cn.
  • Priest ER; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany. xincheng@nju.edu.cn.
  • Li HT; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China. xincheng@nju.edu.cn.
  • Chen J; School of Mathematics and Statistics, University of St. Andrews, Fife, KY16 9SS, Scotland, UK.
  • Aulanier G; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.
  • Chitta LP; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China.
  • Wang YL; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.
  • Peter H; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China.
  • Zhu XS; Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP), 4 place Jussieu, 75005, Paris, France.
  • Xing C; Rosseland Centre for Solar Physics, Institute for Theoretical Astrophysics, Universitetet i Oslo, P.O. Box 1029, Blindern, 0315, Oslo, Norway.
  • Ding MD; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany.
  • Solanki SK; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.
  • Berghmans D; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China.
  • Teriaca L; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany.
  • Aznar Cuadrado R; State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China.
  • Zhukov AN; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.
  • Guo Y; Sorbonne Université, Observatoire de Paris - PSL, École Polytechnique, IP Paris, CNRS, Laboratory for Plasma Physics (LPP), 4 place Jussieu, 75005, Paris, France.
  • Long D; School of Astronomy and Space Science, Nanjing University, 210093, Nanjing, China.
  • Harra L; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 210093, Nanjing, China.
  • Smith PJ; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany.
  • Rodriguez L; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, 1180, Brussels, Belgium.
  • Verbeeck C; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany.
  • Barczynski K; Max Planck Institute for Solar System Research, 37077, Göttingen, Germany.
  • Parenti S; Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium, Ringlaan -3- Av. Circulaire, 1180, Brussels, Belgium.
Nat Commun ; 14(1): 2372, 2023 Apr 25.
Article en En | MEDLINE | ID: mdl-37185588
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Texto completo: 1 Base de datos: MEDLINE Idioma: En Revista: Nat Commun Asunto de la revista: BIOLOGIA / CIENCIA Año: 2023 Tipo del documento: Article País de afiliación: China
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Texto completo: 1 Base de datos: MEDLINE Idioma: En Revista: Nat Commun Asunto de la revista: BIOLOGIA / CIENCIA Año: 2023 Tipo del documento: Article País de afiliación: China