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Artigo de periodico
Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration (2019)
Páez, A.; Jatenco-Pereira, Vera ; Gonçalves, Diego Antonio Falceta ; Opher, M.
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: PLASMA, ONDAS DE CHOQUE, CAMPO MAGNÉTICO, SOL
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
PÁEZ, A. et al. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration. The Astrophysical Journal, v. 879, n. 2, p. 01-09, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab2460. Acesso em: 02 ago. 2024.
APA
Páez, A., Jatenco-Pereira, V., Gonçalves, D. A. F., & Opher, M. (2019). Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration. The Astrophysical Journal, 879( 2), 01-09. doi:10.3847/1538-4357/ab2460
NLM
Páez A, Jatenco-Pereira V, Gonçalves DAF, Opher M. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration [Internet]. The Astrophysical Journal. 2019 ; 879( 2): 01-09.[citado 2024 ago. 02 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
Vancouver
Páez A, Jatenco-Pereira V, Gonçalves DAF, Opher M. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration [Internet]. The Astrophysical Journal. 2019 ; 879( 2): 01-09.[citado 2024 ago. 02 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
Trabalho de evento
Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo (2011)
Santos-Lima, R; Gouveia dal Pino, Elisabete Maria de; Lazarian, A.; Kowal, G.; Falceta Gonçalves, Diego Antonio
Source: Advances in plasma astrophysics: Proceedings. Conference titles: IAU Symposium. Unidades: IAG, EACH
Subjects: CAMPO MAGNÉTICO, MEIO INTERGALÁTICO, PLASMA, MAGNETOHIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS-LIMA, R et al. Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311007563. Acesso em: 02 ago. 2024.
APA
Santos-Lima, R., Gouveia dal Pino, E. M. de, Lazarian, A., Kowal, G., & Falceta Gonçalves, D. A. (2011). Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo. In Advances in plasma astrophysics: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311007563
NLM
Santos-Lima R, Gouveia dal Pino EM de, Lazarian A, Kowal G, Falceta Gonçalves DA. Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311007563
Vancouver
Santos-Lima R, Gouveia dal Pino EM de, Lazarian A, Kowal G, Falceta Gonçalves DA. Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311007563
Trabalho de evento
MHD turbulence-Star Formation Connection: from pc to kpc scales (2011)
Gouveia dal Pino, Elisabete Maria de; Santos-Lima, R; Lazarian, A; Leão, M. R. M; Falceta Gonçalves, Diego Antonio; Kowal, G
Source: Advances in plasma astrophysics: Proceedings. Conference titles: IAU Symposium. Unidades: IAG, EACH
Subjects: FORMAÇÃO DE ESTRELAS, PLASMA, TURBULÊNCIA, MAGNETOHIDRODINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GOUVEIA DAL PINO, Elisabete Maria de et al. MHD turbulence-Star Formation Connection: from pc to kpc scales. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S174392131100723X. Acesso em: 02 ago. 2024.
APA
Gouveia dal Pino, E. M. de, Santos-Lima, R., Lazarian, A., Leão, M. R. M., Falceta Gonçalves, D. A., & Kowal, G. (2011). MHD turbulence-Star Formation Connection: from pc to kpc scales. In Advances in plasma astrophysics: Proceedings. Paris: International Astronomical Union. doi:10.1017/S174392131100723X
NLM
Gouveia dal Pino EM de, Santos-Lima R, Lazarian A, Leão MRM, Falceta Gonçalves DA, Kowal G. MHD turbulence-Star Formation Connection: from pc to kpc scales [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S174392131100723X
Vancouver
Gouveia dal Pino EM de, Santos-Lima R, Lazarian A, Leão MRM, Falceta Gonçalves DA, Kowal G. MHD turbulence-Star Formation Connection: from pc to kpc scales [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S174392131100723X

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