Comparison between 2.5D and 3D simulations of coronal mass ejections
- Author
- JACOBS, C1 ; VAN DER HOIST, B1 ; POEDTS, S1
[1] Centrum voor Plasma-Astrofysica, K.U.Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium - Source
Astronomy and astrophysics (Berlin. Print). 2007, Vol 470, Num 1, pp 359-365, 7 p ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- Sun: coronal mass ejections (CMEs) magnetohydrodynamics (MHD) methods: numerical
- Keyword (fr)
- Couronne solaire Dimensionnalité Ejection masse coronale Espace interplanétaire Magnétohydrodynamique Modèle 3 dimensions Méthode numérique Nuage magnétique Onde choc interplanétaire Onde choc Simulation numérique Soleil Structure 3 dimensions Symétrie axiale
- Keyword (en)
- Solar corona Dimensionality Coronal mass ejection Interplanetary space Magnetohydrodynamics Three dimensional model Numerical method Magnetic cloud Interplanetary shock wave Shock waves Digital simulation Sun Three dimensional structure Axial symmetry
- Keyword (es)
- Dimensionalidad Eyección masa coronal Modelo 3 dimensiones Método numérico Nube magnetica Onda choque interplanetaria Estructura 3 dimensiones
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18886507
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
10.1051/0004-6361:20077305 
https://dx.doi.org/10.1051/0004-6361:20077305
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