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Artigo de periodico
Magnetic flux transport by turbulent reconnection in astrophysical flows (2012)
Dal Pino, Elisabete Maria de Gouveia; Leão, M. R. M; Santos-Lima, R; Guerrero, G; Lazarian, A
Source: Physica Scripta. Unidade: IAG
Subjects: TURBULÊNCIA, MAGNETOHIDRODINÂMICA, MAGNETISMO, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DAL PINO, Elisabete Maria de Gouveia et al. Magnetic flux transport by turbulent reconnection in astrophysical flows. Physica Scripta, v. 86, p. 018401/1-018401/6, 2012Tradução . . Disponível em: https://doi.org/10.1088/0031-8949/86/01/018401. Acesso em: 30 abr. 2024.
APA
Dal Pino, E. M. de G., Leão, M. R. M., Santos-Lima, R., Guerrero, G., & Lazarian, A. (2012). Magnetic flux transport by turbulent reconnection in astrophysical flows. Physica Scripta, 86, 018401/1-018401/6. doi:10.1088/0031-8949/86/01/018401
NLM
Dal Pino EM de G, Leão MRM, Santos-Lima R, Guerrero G, Lazarian A. Magnetic flux transport by turbulent reconnection in astrophysical flows [Internet]. Physica Scripta. 2012 ; 86 018401/1-018401/6.[citado 2024 abr. 30 ] Available from: https://doi.org/10.1088/0031-8949/86/01/018401
Vancouver
Dal Pino EM de G, Leão MRM, Santos-Lima R, Guerrero G, Lazarian A. Magnetic flux transport by turbulent reconnection in astrophysical flows [Internet]. Physica Scripta. 2012 ; 86 018401/1-018401/6.[citado 2024 abr. 30 ] Available from: https://doi.org/10.1088/0031-8949/86/01/018401
Artigo de periodico
Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? (2020)
Kowal, Grzegorz ; Falceta Gonçalves, Diego Antonio ; Lazarian, Alex ; Vishniac, Ethan T
Source: The Astrophysical Journal. Unidade: EACH
Subjects: TURBULÊNCIA, ASTROFÍSICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
KOWAL, Grzegorz et al. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?. The Astrophysical Journal, v. 892, n. 1, p. 01-15, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab7a13. Acesso em: 30 abr. 2024.
APA
Kowal, G., Falceta Gonçalves, D. A., Lazarian, A., & Vishniac, E. T. (2020). Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? The Astrophysical Journal, 892( 1), 01-15. doi:10.3847/1538-4357/ab7a13
NLM
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? [Internet]. The Astrophysical Journal. 2020 ; 892( 1): 01-15.[citado 2024 abr. 30 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
Vancouver
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? [Internet]. The Astrophysical Journal. 2020 ; 892( 1): 01-15.[citado 2024 abr. 30 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
Artigo de periodico
3D turbulent reconnection: Theory, tests, and astrophysical implications (2020)
Lazarian, Alex ; Eyink, Gregory L.; Jafari, Amir ; Kowal, Grzegorz ; Li, Hui ; Xu, Siyao ; Vishniac, Ethan T
Source: Physics of Plasmas. Unidade: EACH
Subjects: TURBULÊNCIA, ASTROFÍSICA, MAGNETOHIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 30 abr. 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 abr. 30 ] 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 abr. 30 ] Available from: https://doi.org/10.1063/1.5110603
Trabalho de evento-anais periodico
3D Turbulent Reconnection: 20 Years After (2019)
Lazarian, Alex ; Kowal, Grzegorz ; Xu, Siyao ; Jafari, Amir
Source: Journal of Physics: Conference Series. Conference titles: Annual International Astrophysics Conference. Unidade: EACH
Subjects: TURBULÊNCIA, ASTROFÍSICA, MAGNETOHIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LAZARIAN, Alex et al. 3D Turbulent Reconnection: 20 Years After. Journal of Physics: Conference Series. Bristol: Escola de Artes, Ciências e Humanidades, Universidade de São Paulo. Disponível em: https://doi.org/10.1088/1742-6596/1332/1/012009. Acesso em: 30 abr. 2024. , 2019
APA
Lazarian, A., Kowal, G., Xu, S., & Jafari, A. (2019). 3D Turbulent Reconnection: 20 Years After. Journal of Physics: Conference Series. Bristol: Escola de Artes, Ciências e Humanidades, Universidade de São Paulo. doi:10.1088/1742-6596/1332/1/012009
NLM
Lazarian A, Kowal G, Xu S, Jafari A. 3D Turbulent Reconnection: 20 Years After [Internet]. Journal of Physics: Conference Series. 2019 ; no 2019( 1): 01-21.[citado 2024 abr. 30 ] Available from: https://doi.org/10.1088/1742-6596/1332/1/012009
Vancouver
Lazarian A, Kowal G, Xu S, Jafari A. 3D Turbulent Reconnection: 20 Years After [Internet]. Journal of Physics: Conference Series. 2019 ; no 2019( 1): 01-21.[citado 2024 abr. 30 ] Available from: https://doi.org/10.1088/1742-6596/1332/1/012009

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