Source: Solar Active Regions and 3D Magnetic Structure. Conference titles: IAU, Joint Discussion. Unidade: IAG
Subjects: SOL, CAMPO MAGNÉTICO
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GUERRERO, G e DAL PINO, Elisabete Maria de Gouveia. The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. 2006, Anais.. Paris: International Astronomical Union, 2006. . Acesso em: 10 set. 2024.APA
Guerrero, G., & Dal Pino, E. M. de G. (2006). The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. In Solar Active Regions and 3D Magnetic Structure. Paris: International Astronomical Union.NLM
Guerrero G, Dal Pino EM de G. The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. Solar Active Regions and 3D Magnetic Structure. 2006 ;[citado 2024 set. 10 ]Vancouver
Guerrero G, Dal Pino EM de G. The effects of the shape and width ofthe tachocline on the butterfly diagram of the solar cycle. Solar Active Regions and 3D Magnetic Structure. 2006 ;[citado 2024 set. 10 ]
