Exploring solar dynamo models with a bipolytropic density profile for a deep meridional flow (2004)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- Assunto: MEIO INTERGALÁTICO
- Language: Inglês
- Imprenta:
- Source:
- Título: Abstract Book
- Conference titles: Magnetic Fields in the Universe : from Laboratory and Stars to Primordial Structures
-
ABNT
GUERRERO, Gustavo e MUÑOZ, José D e GOUVEIA DAL PINO, Elisabete Maria de. Exploring solar dynamo models with a bipolytropic density profile for a deep meridional flow. 2004, Anais.. s.n.: s.l., 2004. . Acesso em: 14 out. 2024. -
APA
Guerrero, G., Muñoz, J. D., & Gouveia dal Pino, E. M. de. (2004). Exploring solar dynamo models with a bipolytropic density profile for a deep meridional flow. In Abstract Book. s.n.: s.l. -
NLM
Guerrero G, Muñoz JD, Gouveia dal Pino EM de. Exploring solar dynamo models with a bipolytropic density profile for a deep meridional flow. Abstract Book. 2004 ;[citado 2024 out. 14 ] -
Vancouver
Guerrero G, Muñoz JD, Gouveia dal Pino EM de. Exploring solar dynamo models with a bipolytropic density profile for a deep meridional flow. Abstract Book. 2004 ;[citado 2024 out. 14 ] - The effects of magnetic fields on radiative cooling jets
- Origin of the superluminal ejections in microquasars by violent magnetic reconnection
- Star formation in 'beta' pictoris triggered by a supernova
- Astrophysical jets and outflows
- Plasmas e altas energias
- Three-dimensional numerical simulations of rotating jets
- Numerical simulations of young stellar jets: from one tenth to parsec scales
- 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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