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The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Magnetohydrodynamics Simulation Module for the Global Solar Corona.
Hayashi, K; Hoeksema, J T; Liu, Y; Bobra, M G; Sun, X D; Norton, A A.
Afiliação
  • Hayashi K; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA USA ; National Astronomical Observatory of China, Chinese Academy of Sciences, Beijing, China.
  • Hoeksema JT; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA USA.
  • Liu Y; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA USA.
  • Bobra MG; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA USA.
  • Sun XD; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA USA.
  • Norton AA; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA USA.
Sol Phys ; 290(5): 1507-1529, 2015.
Article em En | MEDLINE | ID: mdl-26069350
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Sol Phys Ano de publicação: 2015 Tipo de documento: Article
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Sol Phys Ano de publicação: 2015 Tipo de documento: Article