Investigating turbulence effects on magnetic reconnection rates through 3D resistive magnetohydrodynamic simulations (2025)
- Authors:
- USP affiliated authors: KOWAL, GRZEGORZ - EACH ; VICENTIN, GIOVANI HEINZEN - IAG
- Unidades: EACH; IAG
- DOI: 10.3847/1538-4357/addc62
- Assunto: TERCEIRA DIMENSÃO
- Language: Inglês
- Imprenta:
- Publisher place: Philadelphia
- Date published: 2025
- Source:
- Título: The Astrophysical Journal: an international review of astronomy and astronomical physics
- ISSN: 1538-4357
- Volume/Número/Paginação/Ano: v. 987, n. 2, p. 01-18, 2025
- Status:
- Artigo publicado em periódico de acesso aberto (Gold Open Access)
- Versão do Documento:
- Versão publicada (Published version)
- Acessar versão aberta:
-
ABNT
VICENTIN, Giovani Heinzen et al. Investigating turbulence effects on magnetic reconnection rates through 3D resistive magnetohydrodynamic simulations. The Astrophysical Journal: an international review of astronomy and astronomical physics, v. 987, n. 2, p. 01-18, 2025Tradução . . Disponível em: http://dx.doi.org/10.3847/1538-4357/addc62. Acesso em: 08 abr. 2026. -
APA
Vicentin, G. H., Kowal, G., Pino, E. M. de G. D., & Lazarian, A. (2025). Investigating turbulence effects on magnetic reconnection rates through 3D resistive magnetohydrodynamic simulations. The Astrophysical Journal: an international review of astronomy and astronomical physics, 987( 2), 01-18. doi:10.3847/1538-4357/addc62 -
NLM
Vicentin GH, Kowal G, Pino EM de GD, Lazarian A. Investigating turbulence effects on magnetic reconnection rates through 3D resistive magnetohydrodynamic simulations [Internet]. The Astrophysical Journal: an international review of astronomy and astronomical physics. 2025 ; 987( 2): 01-18.[citado 2026 abr. 08 ] Available from: http://dx.doi.org/10.3847/1538-4357/addc62 -
Vancouver
Vicentin GH, Kowal G, Pino EM de GD, Lazarian A. Investigating turbulence effects on magnetic reconnection rates through 3D resistive magnetohydrodynamic simulations [Internet]. The Astrophysical Journal: an international review of astronomy and astronomical physics. 2025 ; 987( 2): 01-18.[citado 2026 abr. 08 ] Available from: http://dx.doi.org/10.3847/1538-4357/addc62 - 3D Turbulent Reconnection: 20 Years After
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- Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?
- Cosmic ray acceleration via turbulence-induced magnetic reconnection: from micro to macro scales
- Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales
- Global and local particle feedback on 3D PIC-RMHD simulations of astrophysical jets
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