Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: SOL, CAMPO MAGNÉTICO
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ABNT
GUERRERO, G e DAL PINO, Elisabete Maria de Gouveia. How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo?. Astronomy & Astrophysics, v. 464, p. 341\2013349, 2007Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065834. Acesso em: 16 nov. 2024.APA
Guerrero, G., & Dal Pino, E. M. de G. (2007). How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? Astronomy & Astrophysics, 464, 341\2013349. doi:10.1051/0004-6361:20065834NLM
Guerrero G, Dal Pino EM de G. How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? [Internet]. Astronomy & Astrophysics. 2007 ; 464 341\2013349.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361:20065834Vancouver
Guerrero G, Dal Pino EM de G. How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? [Internet]. Astronomy & Astrophysics. 2007 ; 464 341\2013349.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361:20065834
