Menu

Filtros : "Zaire, B" Limpar

Filtros

Limitar por data

  • 1

1 - 2 (2 registros)

  • 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

    Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR

    Acesso à fonteDOIComo citar
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas

    • 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: 27 jul. 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 jul. 27 ] 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 jul. 27 ] 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

    Fonte: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Nome do evento: IAU SYMPOSIUM. Unidade: IAG

    Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR

    Acesso à fonteAcesso à fonteDOIComo citar
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas

    • 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: 27 jul. 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 jul. 27 ] 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 jul. 27 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
  • 1

1 - 2 (2 registros)

Biblioteca Digital de Produção Intelectual da Universidade de São Paulo     2012 - 2024