Exploring a deep meridional flow hypothesis for a circulation dominated solar dynamo model (2005)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Subjects: ATIVIDADE SOLAR; MAGNETOHIDRODINÂMICA; CAMPO MAGNÉTICO
- Language: Inglês
- Imprenta:
- Publisher place: College Park
- Date published: 2005
- Source:
- Título: AIP Conference Proceedings
- Volume/Número/Paginação/Ano: v. 784, p. 574-581, 2005
- Conference titles: Conference on Magnetic Fields in the Universe: from Laboratory and Stars to Primordial Structures
-
ABNT
GUERRERO, G. A e MUÑOZ, J. D e DAL PINO, Elisabete Maria de Gouveia. Exploring a deep meridional flow hypothesis for a circulation dominated solar dynamo model. AIP Conference Proceedings. College Park: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 02 nov. 2024. , 2005 -
APA
Guerrero, G. A., Muñoz, J. D., & Dal Pino, E. M. de G. (2005). Exploring a deep meridional flow hypothesis for a circulation dominated solar dynamo model. AIP Conference Proceedings. College Park: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. -
NLM
Guerrero GA, Muñoz JD, Dal Pino EM de G. Exploring a deep meridional flow hypothesis for a circulation dominated solar dynamo model. AIP Conference Proceedings. 2005 ; 784 574-581.[citado 2024 nov. 02 ] -
Vancouver
Guerrero GA, Muñoz JD, Dal Pino EM de G. Exploring a deep meridional flow hypothesis for a circulation dominated solar dynamo model. AIP Conference Proceedings. 2005 ; 784 574-581.[citado 2024 nov. 02 ] - The effects of magnetic fields on radiative cooling jets
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- Cosmic magnetic fields: from stars to the primordial universe
- Probing magneto-centrifugal scenarios for jet production
- On the production and acceleration of astrophysical jets: a comparative study
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