3D Turbulent Reconnection: 20 Years After (2019)
- Authors:
- Autor USP: KOWAL, GRZEGORZ - EACH
- Unidade: EACH
- DOI: 10.1088/1742-6596/1332/1/012009
- Subjects: TURBULÊNCIA; ASTROFÍSICA; MAGNETOHIDRODINÂMICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Journal of Physics: Conference Series
- ISSN: 1742-6588
- Volume/Número/Paginação/Ano: v. 1332, n. 1, p. 01-21, art. 012009, nov. 2019
- Conference titles: Annual International Astrophysics Conference
- Status:
- Artigo publicado em periódico de acesso aberto (Gold Open Access)
- Versão do Documento:
- Versão publicada (Published version)
- Acessar versão aberta:
-
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: 08 abr. 2026. , 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 2026 abr. 08 ] 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 2026 abr. 08 ] Available from: https://doi.org/10.1088/1742-6596/1332/1/012009 - Particle acceleration in self-driven turbulent reconnection
- 3D turbulent reconnection: Theory, tests, and astrophysical implications
- Unveiling a new β scaling of the tearing instability in weakly collisional plasmas
- Colliding-Wind Binaries as a Source of TeV Cosmic Rays
- Generation and effects of electromotive force in turbulent stochastic reconnection
- Investigating turbulence effects on magnetic reconnection rates through 3D resistive magnetohydrodynamic simulations
- Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?
- 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
- Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets
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