Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? (2020)
- Authors:
- USP affiliated authors: KOWAL, GRZEGORZ - EACH ; GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidade: EACH
- DOI: 10.3847/1538-4357/ab7a13
- Subjects: TURBULÊNCIA; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Publisher place: Philadelphia
- Date published: 2020
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 892, n. 1, p. 01-15, mar. 2020
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
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: 28 dez. 2025. -
APA
Kowal, G., Gonçalves, D. A. F., 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, Gonçalves DAF, 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 2025 dez. 28 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13 -
Vancouver
Kowal G, Gonçalves DAF, 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 2025 dez. 28 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13 - Unveiling a new β scaling of the tearing instability in weakly collisional plasmas
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Informações sobre o DOI: 10.3847/1538-4357/ab7a13 (Fonte: oaDOI API)
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