Filtros : "Guerrero, G" Removido: "CAMPO MAGNÉTICO" Limpar

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  • 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: 25 ago. 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 ago. 25 ] 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 ago. 25 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
  • 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: 25 ago. 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 ago. 25 ]
    • 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 ago. 25 ]
  • 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: 25 ago. 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 ago. 25 ]
    • 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 ago. 25 ]
  • 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: 25 ago. 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 ago. 25 ] 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 ago. 25 ] Available from: https://doi.org/10.1088/0031-8949/86/01/018401

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