ReP USP - Resultado da busca

Artigo de periodico
Diffusion of large-scale magnetic fields by reconnection in MHD turbulence (2021)
Santos-Lima, R ; Guerrero, G; Dal Pino, Elisabete Maria de Gouveia ; Lazarian, A.
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assunto: CAMPO MAGNÉTICO
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ABNT
SANTOS-LIMA, R et al. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, v. 503, p. 1290-1309, 2021Tradução . . Disponível em: https://academic.oup.com/mnras/article/503/1/1290/6144594. Acesso em: 07 jun. 2024.
APA
Santos-Lima, R., Guerrero, G., Dal Pino, E. M. de G., & Lazarian, A. (2021). Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, 503, 1290-1309. doi:10.1093/mnras/stab470
NLM
Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2024 jun. 07 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
Vancouver
Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2024 jun. 07 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
Artigo de periodico
What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? (2019)
Guerrero, G; Zaire, B; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia ; Kosovichev, A. G; Mansour, N. N
Source: The Astrophysical Journal. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR
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ABNT
GUERRERO, G et al. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?. The Astrophysical Journal, v. 880, n. 1, p. 6/1-6/20, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab224a. Acesso em: 07 jun. 2024.
APA
Guerrero, G., Zaire, B., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2019). What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? The Astrophysical Journal, 880( 1), 6/1-6/20. doi:10.3847/1538-4357/ab224a
NLM
Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jun. 07 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
Vancouver
Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jun. 07 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
Trabalho de evento
Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations (2017)
Guerrero, G; Smolarkiewicz, P. K; Gouveia dal Pino, Elisabete Maria de; Kososichev, A. G; Zaire, B; Mansour, N. N
Source: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Conference titles: IAU SYMPOSIUM. Unidade: IAG
Subjects: ESTRELAS, ASTROFÍSICA ESTELAR
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ABNT
GUERRERO, G et al. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982. Acesso em: 07 jun. 2024.
APA
Guerrero, G., Smolarkiewicz, P. K., Gouveia dal Pino, E. M. de, Kososichev, A. G., Zaire, B., & Mansour, N. N. (2017). Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations. In Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317003982
NLM
Guerrero G, Smolarkiewicz PK, Gouveia dal Pino EM de, Kososichev AG, Zaire B, Mansour NN. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jun. 07 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
Vancouver
Guerrero G, Smolarkiewicz PK, Gouveia dal Pino EM de, Kososichev AG, Zaire B, Mansour NN. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jun. 07 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
Artigo de periodico
Understanding solar torsional oscillations from global dynamo models (2016)
Guerrero, G; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia
Source: Astrophysical Journal Letters. Unidade: IAG
Subjects: SOL, CAMPO MAGNÉTICO
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ABNT
GUERRERO, G e SMOLARKIEWICZ, P. K e DAL PINO, Elisabete Maria de Gouveia. Understanding solar torsional oscillations from global dynamo models. Astrophysical Journal Letters, 2016Tradução . . Disponível em: https://arxiv.org/abs/1608.02278. Acesso em: 07 jun. 2024.
APA
Guerrero, G., Smolarkiewicz, P. K., & Dal Pino, E. M. de G. (2016). Understanding solar torsional oscillations from global dynamo models. Astrophysical Journal Letters. doi:10.3847/2041-8205/828/1/L3
NLM
Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 jun. 07 ] Available from: https://arxiv.org/abs/1608.02278
Vancouver
Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 jun. 07 ] Available from: https://arxiv.org/abs/1608.02278
Artigo de periodico
On the role of tachoclines in solar and stellar dynamos (2016)
Guerrero, G; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia; Kosovichev, A. G; Mansour, N. N
Source: Astrophysical Journal. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, CAMPO MAGNÉTICO
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ABNT
GUERRERO, G et al. On the role of tachoclines in solar and stellar dynamos. Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf. Acesso em: 07 jun. 2024.
APA
Guerrero, G., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2016). On the role of tachoclines in solar and stellar dynamos. Astrophysical Journal. doi:10.3847/0004-637X/819/2/104
NLM
Guerrero G, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. On the role of tachoclines in solar and stellar dynamos [Internet]. Astrophysical Journal. 2016 ;[citado 2024 jun. 07 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf
Vancouver
Guerrero G, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. On the role of tachoclines in solar and stellar dynamos [Internet]. Astrophysical Journal. 2016 ;[citado 2024 jun. 07 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf
Trabalho de evento-resumo
Effects of tachocline in solar-stellar dynamo simulations (2015)
Kosovichev, Alexander; Guerrero, G; Smolarkiewicz, P; Dal Pino, Elisabete Maria de Gouveia; Mansour, N. N
Source: Meeting Abstracts. Conference titles: IAU General Assembly. Unidade: IAG
Subjects: SOL, ESTRELAS, DÍNAMOS
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ABNT
KOSOVICHEV, Alexander et al. Effects of tachocline in solar-stellar dynamo simulations. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 07 jun. 2024.
APA
Kosovichev, A., Guerrero, G., Smolarkiewicz, P., Dal Pino, E. M. de G., & Mansour, N. N. (2015). Effects of tachocline in solar-stellar dynamo simulations. In Meeting Abstracts. Paris: International Astronomical Union.
NLM
Kosovichev A, Guerrero G, Smolarkiewicz P, Dal Pino EM de G, Mansour NN. Effects of tachocline in solar-stellar dynamo simulations. Meeting Abstracts. 2015 ;[citado 2024 jun. 07 ]
Vancouver
Kosovichev A, Guerrero G, Smolarkiewicz P, Dal Pino EM de G, Mansour NN. Effects of tachocline in solar-stellar dynamo simulations. Meeting Abstracts. 2015 ;[citado 2024 jun. 07 ]
Trabalho de evento-resumo
Solving the problem of magnetic flux transport during star formation (2015)
Santos de Lima, R; Dal Pino, Elisabete Maria de Gouveia; Guerrero, G; Leao, M; Lazarian, A
Source: Meeting Abstracts. Conference titles: IAU General Assembly. Unidade: IAG
Subjects: FORMAÇÃO DE ESTRELAS, MEIO INTERESTELAR
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ABNT
SANTOS DE LIMA, R et al. Solving the problem of magnetic flux transport during star formation. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 07 jun. 2024.
APA
Santos de Lima, R., Dal Pino, E. M. de G., Guerrero, G., Leao, M., & Lazarian, A. (2015). Solving the problem of magnetic flux transport during star formation. In Meeting Abstracts. Paris: International Astronomical Union.
NLM
Santos de Lima R, Dal Pino EM de G, Guerrero G, Leao M, Lazarian A. Solving the problem of magnetic flux transport during star formation. Meeting Abstracts. 2015 ;[citado 2024 jun. 07 ]
Vancouver
Santos de Lima R, Dal Pino EM de G, Guerrero G, Leao M, Lazarian A. Solving the problem of magnetic flux transport during star formation. Meeting Abstracts. 2015 ;[citado 2024 jun. 07 ]
Artigo de periodico
Magnetic flux transport by turbulent reconnection in astrophysical flows (2012)
Dal Pino, Elisabete Maria de Gouveia; Leão, M. R. M; Santos-Lima, R; Guerrero, G; Lazarian, A
Source: Physica Scripta. Unidade: IAG
Subjects: TURBULÊNCIA, MAGNETOHIDRODINÂMICA, MAGNETISMO, ASTROFÍSICA
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ABNT
DAL PINO, Elisabete Maria de Gouveia et al. Magnetic flux transport by turbulent reconnection in astrophysical flows. Physica Scripta, v. 86, p. 018401/1-018401/6, 2012Tradução . . Disponível em: https://doi.org/10.1088/0031-8949/86/01/018401. Acesso em: 07 jun. 2024.
APA
Dal Pino, E. M. de G., Leão, M. R. M., Santos-Lima, R., Guerrero, G., & Lazarian, A. (2012). Magnetic flux transport by turbulent reconnection in astrophysical flows. Physica Scripta, 86, 018401/1-018401/6. doi:10.1088/0031-8949/86/01/018401
NLM
Dal Pino EM de G, Leão MRM, Santos-Lima R, Guerrero G, Lazarian A. Magnetic flux transport by turbulent reconnection in astrophysical flows [Internet]. Physica Scripta. 2012 ; 86 018401/1-018401/6.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1088/0031-8949/86/01/018401
Vancouver
Dal Pino EM de G, Leão MRM, Santos-Lima R, Guerrero G, Lazarian A. Magnetic flux transport by turbulent reconnection in astrophysical flows [Internet]. Physica Scripta. 2012 ; 86 018401/1-018401/6.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1088/0031-8949/86/01/018401
Trabalho de evento-anais periodico
Flux transport solar dynamo models, current problems and possible solutions (2009)
Guerrero, G; Dal Pino, Elisabete Maria de Gouveia
Source: Revista Mexicana de Astronomía y Astrofísica. Conference titles: Magnetic Fields in the Universe II: from Laboratory and Stars to the Primordial Universe. Unidade: IAG
Subjects: SOL, CAMPO MAGNÉTICO
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ABNT
GUERRERO, G e DAL PINO, Elisabete Maria de Gouveia. Flux transport solar dynamo models, current problems and possible solutions. Revista Mexicana de Astronomía y Astrofísica. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 07 jun. 2024. , 2009
APA
Guerrero, G., & Dal Pino, E. M. de G. (2009). Flux transport solar dynamo models, current problems and possible solutions. Revista Mexicana de Astronomía y Astrofísica. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
NLM
Guerrero G, Dal Pino EM de G. Flux transport solar dynamo models, current problems and possible solutions. Revista Mexicana de Astronomía y Astrofísica. 2009 ; 36 CD252-CD261.[citado 2024 jun. 07 ]
Vancouver
Guerrero G, Dal Pino EM de G. Flux transport solar dynamo models, current problems and possible solutions. Revista Mexicana de Astronomía y Astrofísica. 2009 ; 36 CD252-CD261.[citado 2024 jun. 07 ]
Artigo de periodico
Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model (2008)
Guerrero, G; Dal Pino, Elisabete Maria de Gouveia
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: SOL (ATIVIDADE), CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR
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ABNT
GUERRERO, G e DAL PINO, Elisabete Maria de Gouveia. Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model. Astronomy & Astrophysics, v. 485, p. 267-273, 2008Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:200809351. Acesso em: 07 jun. 2024.
APA
Guerrero, G., & Dal Pino, E. M. de G. (2008). Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model. Astronomy & Astrophysics, 485, 267-273. doi:10.1051/0004-6361:200809351
NLM
Guerrero G, Dal Pino EM de G. Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model [Internet]. Astronomy & Astrophysics. 2008 ; 485 267-273.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361:200809351
Vancouver
Guerrero G, Dal Pino EM de G. Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model [Internet]. Astronomy & Astrophysics. 2008 ; 485 267-273.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361:200809351
Artigo de periodico
How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? (2007)
Guerrero, G; Dal Pino, Elisabete Maria de Gouveia
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: SOL, CAMPO MAGNÉTICO
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ABNT
GUERRERO, G e DAL PINO, Elisabete Maria de Gouveia. How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo?. Astronomy & Astrophysics, v. 464, p. 341\2013349, 2007Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065834. Acesso em: 07 jun. 2024.
APA
Guerrero, G., & Dal Pino, E. M. de G. (2007). How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? Astronomy & Astrophysics, 464, 341\2013349. doi:10.1051/0004-6361:20065834
NLM
Guerrero G, Dal Pino EM de G. How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? [Internet]. Astronomy & Astrophysics. 2007 ; 464 341\2013349.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361:20065834
Vancouver
Guerrero G, Dal Pino EM de G. How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? [Internet]. Astronomy & Astrophysics. 2007 ; 464 341\2013349.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361:20065834
Trabalho de evento-resumo
The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle (2006)
Guerrero, G; Dal Pino, Elisabete Maria de Gouveia
Source: Solar Active Regions and 3D Magnetic Structure. Conference titles: IAU, Joint Discussion. Unidade: IAG
Subjects: SOL, CAMPO MAGNÉTICO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GUERRERO, G e DAL PINO, Elisabete Maria de Gouveia. The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. 2006, Anais.. Paris: International Astronomical Union, 2006. . Acesso em: 07 jun. 2024.
APA
Guerrero, G., & Dal Pino, E. M. de G. (2006). The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. In Solar Active Regions and 3D Magnetic Structure. Paris: International Astronomical Union.
NLM
Guerrero G, Dal Pino EM de G. The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. Solar Active Regions and 3D Magnetic Structure. 2006 ;[citado 2024 jun. 07 ]
Vancouver
Guerrero G, Dal Pino EM de G. The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. Solar Active Regions and 3D Magnetic Structure. 2006 ;[citado 2024 jun. 07 ]

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