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Radiative magnetohydrodynamic simulations of solar pores

Author
CAMERON, R1 ; SCHÜSSLER, M1 ; VÖGLER, A2 ; ZAKHAROV, V1
[1] Max-Planck-Institut fur Sonnensystemforschung Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
[2] Sterrekundig Instituut, Utrecht University, Postbus 80 000, 3508 TA Utrecht, Netherlands
Source

Astronomy and astrophysics (Berlin. Print). 2007, Vol 474, Num 1, pp 261-272, 12 p ; ref : 3/4 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: activity Sun: magnetic fields Sun: magnetohydrodynamics (MHD) Sun: photosphere
Keyword (fr)
Champ magnétique Champ écoulement Condition aux limites Continuum Dynamique Energétique Flux magnétique Granulation solaire Intensité Magnétohydrodynamique Modèle 3 dimensions Modèle MHD Morphologie Pénombre Simulation numérique Soleil Structure interne Structure magnétique Structure petite échelle Tache solaire
Keyword (en)
Magnetic fields Flow pattern Boundary conditions Continuum Dynamics Energetics Magnetic flux Solar granulation Intensity Magnetohydrodynamics Three dimensional model MHD model Morphology Penumbra Digital simulation Sun Internal structure Magnetic structure Small scale structure Sunspots
Keyword (es)
Continuo Energética Intensidad Modelo 3 dimensiones Modelo MHD Estructura interna Estructura pequeña escala
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19138509

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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