Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations (2017)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.1017/S1743921317003982
- Subjects: ESTRELAS; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Publisher place: Cambridge
- Date published: 2017
- ISBN: 9781107170056
- Source:
- Conference titles: IAU SYMPOSIUM
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
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: 10 jan. 2026. -
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 2026 jan. 10 ] 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 2026 jan. 10 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982 - Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
- Prospect on intergalactic magnetic field measurements with gamma-ray instruments
- A magnetic reconnection model for explaining the multiwave length emission of the microquasars Cyg X-1 and Cyg X-3
- Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?
- Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: a major accretion disc contribution
- 3D hydrodynamical simulations of galactic winds: an application to the starburst galaxy M82
- The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays
- Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs
- Gamma-ray flux distribution and nonlinear behavior of four lat bright AGNs
- The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks
Informações sobre o DOI: 10.1017/S1743921317003982 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
