Study on the relation of the solar coronal rotation with magnetic field structures.

Xiang, N B; Zhao, X H; Deng, L H; Li, F Y; Zheng, S

Xiang, N B; Zhao, X H; Deng, L H; Li, F Y; Zheng, S.

Afiliación

Xiang NB; Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China. nanbin@ynao.ac.cn.
Zhao XH; State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China. nanbin@ynao.ac.cn.
Deng LH; State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China. xhzhao@spaceweather.ac.cn.
Li FY; School of Mathematics and Computer Science, Yunnan Minzu University, Kunming, 650504, China. linhua.deng@ymu.edu.cn.
Zheng S; State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China.

Sci Rep ; 13(1): 21089, 2023 Nov 30.

Article en En | MEDLINE | ID: mdl-38036637

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Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Sci Rep Año: 2023 Tipo del documento: Article País de afiliación: China Pais de publicación: Reino Unido

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