Symmetry breaking in stellar dynamos
- Autor
- JENNINGS, R. L; WEISS, N. O
Univ. Cambridge, dep. applied mathematics theoretical physics, Cambridge CB3 9EW, United Kingdom - Fuente
Monthly Notices of the Royal Astronomical Society. 1991, Vol 252, Num 2, pp 249-260 ; ref : 58 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- Blackwell Science, Oxford
- País de la publicación
- United Kingdom
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Bifurcation Brisure symétrie Champ magnétique Circulation méridienne Etoile type avancé Génération Modèle théorique Simulation numérique Soleil Théorie dynamo Théorie linéaire
- Palabra clave (in)
- Bifurcation Symmetry breaking Magnetic field Meridional circulation Late type star Generation Theoretical model Numerical simulation Sun Dynamo theory Linear theory
- Palabra clave (es)
- Bifurcación Ruptura simetría Campo magnético Circulación meridiana Estrella tipo avanzada Generación Modelo teórico Simulación numérica Sol Teoría dinamo Teoría lineal
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10L Magnetic and electric fields. Polarization of starlight
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 4957552
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1093/mnras/252.2.249 
https://dx.doi.org/10.1093/mnras/252.2.249
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