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ZHANG, Jian-Fu et al. Particle acceleration in self-driven turbulent reconnection. Journal of High Energy Astrophysics, v. No 2023, p. 01-10, 2023Tradução . . Disponível em: https://doi.org/10.1016/j.jheap.2023.08.001. Acesso em: 25 ago. 2024.
APA
Zhang, J. -F., Xu, S., Lazarian, A., & Kowal, G. (2023). Particle acceleration in self-driven turbulent reconnection. Journal of High Energy Astrophysics, No 2023, 01-10. doi:10.1016/j.jheap.2023.08.001
NLM
Zhang J-F, Xu S, Lazarian A, Kowal G. Particle acceleration in self-driven turbulent reconnection [Internet]. Journal of High Energy Astrophysics. 2023 ; No 2023 01-10.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1016/j.jheap.2023.08.001
Vancouver
Zhang J-F, Xu S, Lazarian A, Kowal G. Particle acceleration in self-driven turbulent reconnection [Internet]. Journal of High Energy Astrophysics. 2023 ; No 2023 01-10.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1016/j.jheap.2023.08.001
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TORREJÓN, Tania Elizabeth Medina e PINO, Elisabete Maria de Gouveia Dal e KOWAL, Grzegorz. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales. The Astrophysical Journal, v. 952, n. 2, p. 01-11, 2023Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/acd699. Acesso em: 25 ago. 2024.
APA
Torrejón, T. E. M., Pino, E. M. de G. D., & Kowal, G. (2023). Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales. The Astrophysical Journal, 952( 2), 01-11. doi:10.3847/1538-4357/acd699
NLM
Torrejón TEM, Pino EM de GD, Kowal G. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales [Internet]. The Astrophysical Journal. 2023 ; 952( 2): 01-11.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/acd699
Vancouver
Torrejón TEM, Pino EM de GD, Kowal G. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales [Internet]. The Astrophysical Journal. 2023 ; 952( 2): 01-11.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/acd699
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AMARAL, Bianca Basilio et al. Adesão às novas tecnologias na área da saúde: no exemplo das vacinas baseadas em MRNA para a Covid-19. 2022, Anais.. São Paulo: Escola de Artes, Ciências e Humanidades, 2022. p. 114-115. Disponível em: http://www5.each.usp.br/wp-content/uploads/2022/02/ANAIS-29%C2%BA-SIICUSP-EACH_USP.pdf. Acesso em: 25 ago. 2024.
APA
Amaral, B. B., Gonçalvez, L. H. F., Zanetti, M. C. G., Lima, M. F. B., Rocha, M. C., Lisboa, M. M., et al. (2022). Adesão às novas tecnologias na área da saúde: no exemplo das vacinas baseadas em MRNA para a Covid-19. In 29º SIICUSP-EACH 2021: Simpósio Internacional de Iniciação Científica e Tecnológica da USP: livro de resumos (p. 114-115). São Paulo: Escola de Artes, Ciências e Humanidades. Recuperado de http://www5.each.usp.br/wp-content/uploads/2022/02/ANAIS-29%C2%BA-SIICUSP-EACH_USP.pdf
NLM
Amaral BB, Gonçalvez LHF, Zanetti MCG, Lima MFB, Rocha MC, Lisboa MM, Teruya MM, Kowal G. Adesão às novas tecnologias na área da saúde: no exemplo das vacinas baseadas em MRNA para a Covid-19 [Internet]. 29º SIICUSP-EACH 2021: Simpósio Internacional de Iniciação Científica e Tecnológica da USP: livro de resumos. 2022 ; 114-115.[citado 2024 ago. 25 ] Available from: http://www5.each.usp.br/wp-content/uploads/2022/02/ANAIS-29%C2%BA-SIICUSP-EACH_USP.pdf
Vancouver
Amaral BB, Gonçalvez LHF, Zanetti MCG, Lima MFB, Rocha MC, Lisboa MM, Teruya MM, Kowal G. Adesão às novas tecnologias na área da saúde: no exemplo das vacinas baseadas em MRNA para a Covid-19 [Internet]. 29º SIICUSP-EACH 2021: Simpósio Internacional de Iniciação Científica e Tecnológica da USP: livro de resumos. 2022 ; 114-115.[citado 2024 ago. 25 ] Available from: http://www5.each.usp.br/wp-content/uploads/2022/02/ANAIS-29%C2%BA-SIICUSP-EACH_USP.pdf
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NOWAK, Natalia e KOWAL, Grzegorz e GONÇALVES, Diego Antonio Falceta. Generation and effects of electromotive force in turbulent stochastic reconnection. Physics of Plasmas, v. 28, n. 6, p. 062310-01 - 062310-12, 2021Tradução . . Disponível em: https://doi.org/10.1063/5.0045696. Acesso em: 25 ago. 2024.
APA
Nowak, N., Kowal, G., & Gonçalves, D. A. F. (2021). Generation and effects of electromotive force in turbulent stochastic reconnection. Physics of Plasmas, 28( 6), 062310-01 - 062310-12. doi:10.1063/5.0045696
NLM
Nowak N, Kowal G, Gonçalves DAF. Generation and effects of electromotive force in turbulent stochastic reconnection [Internet]. Physics of Plasmas. 2021 ; 28( 6): 062310-01 - 062310-12.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1063/5.0045696
Vancouver
Nowak N, Kowal G, Gonçalves DAF. Generation and effects of electromotive force in turbulent stochastic reconnection [Internet]. Physics of Plasmas. 2021 ; 28( 6): 062310-01 - 062310-12.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1063/5.0045696
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MEDINA-TORREJON, Tania et al. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets. Astrophysical Journal, v. 908, n. 2, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abd6c2. Acesso em: 25 ago. 2024.
APA
Medina-Torrejon, T., Dal Pino, E. de G., Kadowaki, L. H. S., Kowal, G., Singh, C. B., & Mizuno, Y. (2021). Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets. Astrophysical Journal, 908( 2). doi:10.3847/1538-4357/abd6c2
NLM
Medina-Torrejon T, Dal Pino E de G, Kadowaki LHS, Kowal G, Singh CB, Mizuno Y. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets [Internet]. Astrophysical Journal. 2021 ; 908( 2):[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/abd6c2
Vancouver
Medina-Torrejon T, Dal Pino E de G, Kadowaki LHS, Kowal G, Singh CB, Mizuno Y. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets [Internet]. Astrophysical Journal. 2021 ; 908( 2):[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/abd6c2
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KOWAL, Grzegorz e FALCETA GONÇALVES, Diego Antonio. Colliding-Wind Binaries as a Source of TeV Cosmic Rays. Frontiers in Astronomy and Space Sciences, v. 8, p. 01-11, 2021Tradução . . Disponível em: https://doi.org/10.3389/fspas.2021.667805. Acesso em: 25 ago. 2024.
APA
Kowal, G., & Falceta Gonçalves, D. A. (2021). Colliding-Wind Binaries as a Source of TeV Cosmic Rays. Frontiers in Astronomy and Space Sciences, 8, 01-11. doi:10.3389/fspas.2021.667805
NLM
Kowal G, Falceta Gonçalves DA. Colliding-Wind Binaries as a Source of TeV Cosmic Rays [Internet]. Frontiers in Astronomy and Space Sciences. 2021 ; 8 01-11.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3389/fspas.2021.667805
Vancouver
Kowal G, Falceta Gonçalves DA. Colliding-Wind Binaries as a Source of TeV Cosmic Rays [Internet]. Frontiers in Astronomy and Space Sciences. 2021 ; 8 01-11.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3389/fspas.2021.667805
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LAZARIAN, Alex et al. 3D turbulent reconnection: Theory, tests, and astrophysical implications. Physics of Plasmas, v. 27, n. ja 2020, p. 01-63, 2020Tradução . . Disponível em: https://doi.org/10.1063/1.5110603. Acesso em: 25 ago. 2024.
APA
Lazarian, A., Eyink, G. L., Jafari, A., Kowal, G., Li, H., Xu, S., & Vishniac, E. T. (2020). 3D turbulent reconnection: Theory, tests, and astrophysical implications. Physics of Plasmas, 27( ja 2020), 01-63. doi:10.1063/1.5110603
NLM
Lazarian A, Eyink GL, Jafari A, Kowal G, Li H, Xu S, Vishniac ET. 3D turbulent reconnection: Theory, tests, and astrophysical implications [Internet]. Physics of Plasmas. 2020 ; 27( ja 2020): 01-63.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1063/1.5110603
Vancouver
Lazarian A, Eyink GL, Jafari A, Kowal G, Li H, Xu S, Vishniac ET. 3D turbulent reconnection: Theory, tests, and astrophysical implications [Internet]. Physics of Plasmas. 2020 ; 27( ja 2020): 01-63.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1063/1.5110603
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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: 25 ago. 2024.
APA
Kowal, G., Falceta Gonçalves, D. A., 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, Falceta Gonçalves DA, 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 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
Vancouver
Kowal G, Falceta Gonçalves DA, 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 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
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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: 25 ago. 2024. , 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 2024 ago. 25 ] 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 2024 ago. 25 ] Available from: https://doi.org/10.1088/1742-6596/1332/1/012009
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ACHARYYA, A. et al. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout. Astroparticle Physics, v. 111, p. 35-53, 2019Tradução . . Disponível em: https://doi.org/10.1016/j.astropartphys.2019.04.001. Acesso em: 25 ago. 2024.
APA
Acharyya, A., Souza, V. de, Vecchi, M., Dal Pino, E. M. de G., & Kowal, G. (2019). Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout. Astroparticle Physics, 111, 35-53. doi:10.1016/j.astropartphys.2019.04.001
NLM
Acharyya A, Souza V de, Vecchi M, Dal Pino EM de G, Kowal G. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout [Internet]. Astroparticle Physics. 2019 ; 111 35-53.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1016/j.astropartphys.2019.04.001
Vancouver
Acharyya A, Souza V de, Vecchi M, Dal Pino EM de G, Kowal G. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout [Internet]. Astroparticle Physics. 2019 ; 111 35-53.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1016/j.astropartphys.2019.04.001
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GOUVEIA DAL PINO, Elisabete Maria de et al. Magnetic reconnection on jet-accretion disk systems. Proceedings of Science. Trieste - Italy: Scuola Internazionale Superiore di Studi Avanzati - SISSA. . Acesso em: 25 ago. 2024. , 2017
APA
Gouveia dal Pino, E. M. de, Dell Valle, M. V., Kadowaki, L., Khiali, B., Kowal, G., Mizuno, Y., & Singh, C. B. (2017). Magnetic reconnection on jet-accretion disk systems. Proceedings of Science. Trieste - Italy: Scuola Internazionale Superiore di Studi Avanzati - SISSA.
NLM
Gouveia dal Pino EM de, Dell Valle MV, Kadowaki L, Khiali B, Kowal G, Mizuno Y, Singh CB. Magnetic reconnection on jet-accretion disk systems. Proceedings of Science. 2017 ; 269 1-13.[citado 2024 ago. 25 ]
Vancouver
Gouveia dal Pino EM de, Dell Valle MV, Kadowaki L, Khiali B, Kowal G, Mizuno Y, Singh CB. Magnetic reconnection on jet-accretion disk systems. Proceedings of Science. 2017 ; 269 1-13.[citado 2024 ago. 25 ]
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CAPRONI, Anderson et al. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, v. 838, n. 2, p. 1-9, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6002. Acesso em: 25 ago. 2024.
APA
Caproni, A., Lanfranchi, G. A., Baio, G. H. C., Kowal, G., & Falceta Gonçalves, D. A. (2017). Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, 838( 2), 1-9. doi:10.3847/1538-4357/aa6002
NLM
Caproni A, Lanfranchi GA, Baio GHC, Kowal G, Falceta Gonçalves DA. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
Vancouver
Caproni A, Lanfranchi GA, Baio GHC, Kowal G, Falceta Gonçalves DA. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
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SANTOS-LIMA, Reinaldo et al. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback. Monthly Notices of the Royal Astronomical Society, v. 465, n. 4, p. 4866-4871, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw3050. Acesso em: 25 ago. 2024.
APA
Santos-Lima, R., Dal Pino, E. M. de G., Falceta Gonçalves, D. A., Nakwacki, M. S., & Kowal, G. (2017). Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback. Monthly Notices of the Royal Astronomical Society, 465( 4), 4866-4871. doi:10.1093/mnras/stw3050
NLM
Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA, Nakwacki MS, Kowal G. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 465( 4): 4866-4871.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stw3050
Vancouver
Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA, Nakwacki MS, Kowal G. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 465( 4): 4866-4871.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stw3050
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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: 25 ago. 2024.
APA
Kowal, G., Falceta Gonçalves, D. A., 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, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6001
Vancouver
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2024 ago. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6001
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NAKWACKI, Maria Soledad et al. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society, v. 455, n. 4, p. 3702-3723, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2586. Acesso em: 25 ago. 2024.
APA
Nakwacki, M. S., Kowal, G., Santos-Lima, R., Dal Pino, E. M. de G., & Falceta Gonçalves, D. A. (2016). Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society, 455( 4), 3702-3723. doi:10.1093/mnras/stv2586
NLM
Nakwacki MS, Kowal G, Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455( 4): 3702-3723.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stv2586
Vancouver
Nakwacki MS, Kowal G, Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455( 4): 3702-3723.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stv2586
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DAL PINO, Elisabete Maria de Gouveia e KOWAL, Grzegorz. Particle acceleration by magnetic reconnection. Magnetic fields in diffuse media. Tradução . Heidelberg: Springer, 2015. . . Acesso em: 25 ago. 2024.
APA
Dal Pino, E. M. de G., & Kowal, G. (2015). Particle acceleration by magnetic reconnection. In Magnetic fields in diffuse media. Heidelberg: Springer.
NLM
Dal Pino EM de G, Kowal G. Particle acceleration by magnetic reconnection. In: Magnetic fields in diffuse media. Heidelberg: Springer; 2015. [citado 2024 ago. 25 ]
Vancouver
Dal Pino EM de G, Kowal G. Particle acceleration by magnetic reconnection. In: Magnetic fields in diffuse media. Heidelberg: Springer; 2015. [citado 2024 ago. 25 ]
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FALCETA GONÇALVES, Diego Antonio et al. The onset of large-scale turbulence in the interstellar medium of spiral galaxies. Monthly Notices of the Royal Astronomical Society, v. 446, n. ja 2015, p. 973-989, 2015Tradução . . Disponível em: https://doi.org/10.1093/mnras/stu2127. Acesso em: 25 ago. 2024.
APA
Falceta Gonçalves, D. A., Bonnell, I., Kowal, G., Lépine, J. R. D., & Braga, C. A. de S. (2015). The onset of large-scale turbulence in the interstellar medium of spiral galaxies. Monthly Notices of the Royal Astronomical Society, 446( ja 2015), 973-989. doi:10.1093/mnras/stu2127
NLM
Falceta Gonçalves DA, Bonnell I, Kowal G, Lépine JRD, Braga CA de S. The onset of large-scale turbulence in the interstellar medium of spiral galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 446( ja 2015): 973-989.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stu2127
Vancouver
Falceta Gonçalves DA, Bonnell I, Kowal G, Lépine JRD, Braga CA de S. The onset of large-scale turbulence in the interstellar medium of spiral galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 446( ja 2015): 973-989.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stu2127
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FALCETA GONÇALVES, Diego Antonio e KOWAL, Grzegorz. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media. The Astrophysical Journal, v. 808, n. 1, p. 1-15, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/65. Acesso em: 25 ago. 2024.
APA
Falceta Gonçalves, D. A., & Kowal, G. (2015). Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media. The Astrophysical Journal, 808( 1), 1-15. doi:10.1088/0004-637X/808/1/65
NLM
Falceta Gonçalves DA, Kowal G. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media [Internet]. The Astrophysical Journal. 2015 ; 808( 1): 1-15.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1088/0004-637X/808/1/65
Vancouver
Falceta Gonçalves DA, Kowal G. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media [Internet]. The Astrophysical Journal. 2015 ; 808( 1): 1-15.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1088/0004-637X/808/1/65
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POIDEVIN, Frédérick et al. Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog. 2015, Anais.. Cambridge: Cambridge University Press, 2015. Disponível em: https://doi.org/10.1017/S1743921314011600. Acesso em: 25 ago. 2024.
APA
Poidevin, F., Falceta-Gonçalves, D., Kowal, G., Dal Pino, E. M. de G., & Magalhães, A. M. (2015). Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog. In IAU Highlights of Astronomy, v. 16. Cambridge: Cambridge University Press. doi:10.1017/S1743921314011600
NLM
Poidevin F, Falceta-Gonçalves D, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog [Internet]. IAU Highlights of Astronomy, v. 16. 2015 ;[citado 2024 ago. 25 ] Available from: https://doi.org/10.1017/S1743921314011600
Vancouver
Poidevin F, Falceta-Gonçalves D, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog [Internet]. IAU Highlights of Astronomy, v. 16. 2015 ;[citado 2024 ago. 25 ] Available from: https://doi.org/10.1017/S1743921314011600
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ABNT
SILVA, Gustavo Rocha da et al. Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows. Monthly Notices of the Royal Astronomical Society, v. 446, n. ja 2015, p. 104-119, 2015Tradução . . Disponível em: https://doi.org/10.1093/mnras/stu2104. Acesso em: 25 ago. 2024.
APA
Silva, G. R. da, Falceta Gonçalves, D. A., Kowal, G., & Dal Pino, E. M. de G. (2015). Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows. Monthly Notices of the Royal Astronomical Society, 446( ja 2015), 104-119. doi:10.1093/mnras/stu2104
NLM
Silva GR da, Falceta Gonçalves DA, Kowal G, Dal Pino EM de G. Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 446( ja 2015): 104-119.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stu2104
Vancouver
Silva GR da, Falceta Gonçalves DA, Kowal G, Dal Pino EM de G. Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 446( ja 2015): 104-119.[citado 2024 ago. 25 ] Available from: https://doi.org/10.1093/mnras/stu2104