RECOVERING PHOTOSPHERIC VELOCITIES FROM VECTOR MAGNETOGRAMS BY USING A THREE-DIMENSIONAL, FULLY MAGNETOHYDRODYNAMIC MODEL
- Author
- WANG, A. H1 ; WU, S. T1 ; YANG LIU2 ; HATHAWAY, D3
[1] Center for Space Plasma and Aeronomic Research and Department of Mechanical and Aerospace Engineering, University of Alabama, Huntsville, AL 35899, United States
[2] W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085, United States
[3] George C. Marshall Space Flight Center/National Aeronautical and Space Administration, Huntsville, AL 35812, United States - Source
The Astrophysical journal. 2008, Vol 674, Num 1 ; L57-L60 ; 2 ; ref : 1/4 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
- English
- Author keyword
- MHD Sun : activity Sun : atmospheric motions Sun: magnetic fields
- Keyword (fr)
- Champ magnétique Magnétogramme Modèle MHD Mouvement atmosphérique Soleil
- Keyword (en)
- Magnetic fields Magnetogram MHD model Atmospheric movements Sun
- Keyword (es)
- Magnetograma Modelo MHD
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20082022
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
10.1086/528844 
https://dx.doi.org/10.1086/528844
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