Statistics of reconnection-driven turbulence (2017)
- Authors:
- Autor USP: GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidade: EACH
- DOI: 10.3847/1538-4357/aa6001
- Subjects: TURBULÊNCIA; MAGNETOHIDRODINÂMICA
- Language: Inglês
- Imprenta:
- Publisher place: Philadelphia
- Date published: 2017
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 838, n. 2, p. 1-13, apr. 2017
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
KOWAL, Grzegorz et al. Statistics of reconnection-driven turbulence. The Astrophysical Journal, v. 838, n. 2, p. 1-13, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6001. Acesso em: 28 dez. 2025. -
APA
Kowal, G., Gonçalves, D. A. F., Lazarian, A., & Vishniac, E. T. (2017). Statistics of reconnection-driven turbulence. The Astrophysical Journal, 838( 2), 1-13. doi:10.3847/1538-4357/aa6001 -
NLM
Kowal G, Gonçalves DAF, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2025 dez. 28 ] Available from: https://doi.org/10.3847/1538-4357/aa6001 -
Vancouver
Kowal G, Gonçalves DAF, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2025 dez. 28 ] Available from: https://doi.org/10.3847/1538-4357/aa6001 - Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium
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Informações sobre o DOI: 10.3847/1538-4357/aa6001 (Fonte: oaDOI API)
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