THREE-DIMENSIONAL MODELING OF COMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE IN THE LOCAL INTERSTELLAR MEDIUM
- Author
- CHERNYSHOV, A. A1 ; KARELSKY, K. V1 ; PETROSYAN, A. S1
[1] Theoretical Section, Space Research Institute of Russian Academy of Sciences, Profsoyuznaya 84/32, 117997, Moscow, Russian Federation - Source
The Astrophysical journal. 2008, Vol 686, Num 2, pp 1137-1144, 8 p ; 1 ; ref : 1/2 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- Russian
- Author keyword
- ISM: kinematics and dynamics MHD methods: numerical plasmas turbulence
- Keyword (fr)
- Cinématique Dynamique Modélisation Méthode numérique Plasma Turbulence MHD Voisinage solaire
- Keyword (en)
- Kinematics Dynamics Modelling Numerical method Plasma MHD turbulence Solar neighborhood
- Keyword (es)
- Método numérico Turbulencia MHD Vecindad solar
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20792342
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
10.1086/591642 
https://dx.doi.org/10.1086/591642
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