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Analytical solutions for time-dependent kinematic three-dimensional magnetic reconnection.
Chen, Yalan; Wang, Yi; Wei, Fengsi; Feng, Xueshang; Zhou, Zilu; Wang, Boyi; Zuo, Pingbing; Jiang, Chaowei; Xu, Xiaojun; Song, Xiaojian; Gu, Yaxin; Wang, Ludi; Xu, Xiaoheng; Bian, Xinkai.
Afiliação
  • Chen Y; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Wang Y; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Wei F; Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China.
  • Feng X; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Zhou Z; Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China.
  • Wang B; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Zuo P; Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China.
  • Jiang C; State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, 999078, China.
  • Xu X; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Song X; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Gu Y; Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China.
  • Wang L; Shenzhen Key Laboratory of Numerical Prediction for Space Storm, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, China.
  • Xu X; Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China.
  • Bian X; State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, 999078, China.
PLoS One ; 18(5): e0286138, 2023.
Article em En | MEDLINE | ID: mdl-37253032
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Física / Campos Magnéticos Idioma: En Revista: PLoS One Assunto da revista: CIENCIA / MEDICINA Ano de publicação: 2023 Tipo de documento: Article País de afiliação: China
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Física / Campos Magnéticos Idioma: En Revista: PLoS One Assunto da revista: CIENCIA / MEDICINA Ano de publicação: 2023 Tipo de documento: Article País de afiliação: China