What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? (2019)
- Authors:
- Autor USP: DAL PINO, ELISABETE MARIA DE GOUVEIA - IAG
- Unidade: IAG
- DOI: 10.3847/1538-4357/ab224a
- Subjects: CAMPO MAGNÉTICO; ASTROFÍSICA SOLAR
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: The Astrophysical Journal
- ISSN: 2041-8213
- Volume/Número/Paginação/Ano: v. 880, n. 1, July, p. 6/1-6/20, 2019
- 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. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?. The Astrophysical Journal, v. 880, n. 1, p. 6/1-6/20, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab224a. Acesso em: 26 jul. 2024. -
APA
Guerrero, G., Zaire, B., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2019). What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? The Astrophysical Journal, 880( 1), 6/1-6/20. doi:10.3847/1538-4357/ab224a -
NLM
Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jul. 26 ] Available from: https://doi.org/10.3847/1538-4357/ab224a -
Vancouver
Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jul. 26 ] Available from: https://doi.org/10.3847/1538-4357/ab224a - Jet-ISM cloud interactions: 3D simulations of the HH 270/110 jet system
- Explosões assimétricas e jatos supersônicos
- Heating of T tauri disk winds by magnetic reconnection
- Evolution of the ISM of starburst galaxies and the formation of galactic superwinds
- Origin of jets and winds from stars and galaxies
- A mechanism for the superluminal ejections in microquasars: a jet/accretion disk symbiosis
- Exploring a different geometry for the solar tachocline in kinematic solar dynamo model
- On the production and acceleration of astrophysical jets: a comparative study
- Turbulent magnetic reconnection as a possible solution for the magnetic braking problem in protostellar disks
- Numerical study of turbulence of the intracluster medium using a collisionless MHD model
Informações sobre o DOI: 10.3847/1538-4357/ab224a (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas