3D turbulent reconnection: Theory, tests, and astrophysical implications (2020)
- Authors:
- Autor USP: KOWAL, GRZEGORZ - EACH
- Unidade: EACH
- DOI: 10.1063/1.5110603
- Subjects: TURBULÊNCIA; ASTROFÍSICA; MAGNETOHIDRODINÂMICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Physics of Plasmas
- ISSN: 1070-664X
- Volume/Número/Paginação/Ano: v. 27, n. 1, p. 01-63, art. 012305, jan. 2020
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: hybrid
- Licença: cc-by
-
ABNT
LAZARIAN, Alex et al. 3D turbulent reconnection: Theory, tests, and astrophysical implications. Physics of Plasmas, v. 27, n. ja 2020, p. 01-63, 2020Tradução . . Disponível em: https://doi.org/10.1063/1.5110603. Acesso em: 04 nov. 2024. -
APA
Lazarian, A., Eyink, G. L., Jafari, A., Kowal, G., Li, H., Xu, S., & Vishniac, E. T. (2020). 3D turbulent reconnection: Theory, tests, and astrophysical implications. Physics of Plasmas, 27( ja 2020), 01-63. doi:10.1063/1.5110603 -
NLM
Lazarian A, Eyink GL, Jafari A, Kowal G, Li H, Xu S, Vishniac ET. 3D turbulent reconnection: Theory, tests, and astrophysical implications [Internet]. Physics of Plasmas. 2020 ; 27( ja 2020): 01-63.[citado 2024 nov. 04 ] Available from: https://doi.org/10.1063/1.5110603 -
Vancouver
Lazarian A, Eyink GL, Jafari A, Kowal G, Li H, Xu S, Vishniac ET. 3D turbulent reconnection: Theory, tests, and astrophysical implications [Internet]. Physics of Plasmas. 2020 ; 27( ja 2020): 01-63.[citado 2024 nov. 04 ] Available from: https://doi.org/10.1063/1.5110603 - Particle acceleration in self-driven turbulent reconnection
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Informações sobre o DOI: 10.1063/1.5110603 (Fonte: oaDOI API)
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