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Filtros : "EACH" "Boston University, Astronomy Department" Removidos: "Indexado no: BDENF" "ARTIGO DE JORNAL-RESENHA" "Universidade Federal da Bahia (UFBA)" "RUSP" Limpar

Filtros

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.
Fonte: The Astrophysical Journal. Unidades: IAG, EACH
Assuntos: 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: 15 maio 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 maio 15 ] 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 maio 15 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
Artigo de periodico
Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces (2017)
Murcia, Miguel Andres Paez; Pereira, Vera Jatenco Silva; Gonçalves, Diego Antonio Falceta; opher, merav
Fonte: The Astrophysical Journal: an international review of astronomy and astronomical physics. Unidades: EACH, IAG
Assuntos: VENTO SOLAR, SOL, CAMPO MAGNÉTICO, ATIVIDADE SOLAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MURCIA, Miguel Andres Paez et al. Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces. The Astrophysical Journal: an international review of astronomy and astronomical physics, v. 851, p. 01-09, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa9753. Acesso em: 15 maio 2024.
APA
Murcia, M. A. P., Pereira, V. J. S., Gonçalves, D. A. F., & opher, merav. (2017). Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces. The Astrophysical Journal: an international review of astronomy and astronomical physics, 851, 01-09. doi:10.3847/1538-4357/aa9753
NLM
Murcia MAP, Pereira VJS, Gonçalves DAF, opher merav. Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces [Internet]. The Astrophysical Journal: an international review of astronomy and astronomical physics. 2017 ; 851 01-09.[citado 2024 maio 15 ] Available from: https://doi.org/10.3847/1538-4357/aa9753
Vancouver
Murcia MAP, Pereira VJS, Gonçalves DAF, opher merav. Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces [Internet]. The Astrophysical Journal: an international review of astronomy and astronomical physics. 2017 ; 851 01-09.[citado 2024 maio 15 ] Available from: https://doi.org/10.3847/1538-4357/aa9753

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