Emergence of magnetic flux from the convection zone into the corona

Astronomy and Astrophysics

Volumn 426, Issue 3, 2004, Pages 1047-1063

  Archontis, V ^a   Moreno Insertis, F ^a,b   Galsgaard, K ^c,d   Hood, A ^c   O'Shea, E ^a  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD DE LA LAGUNA   (Spain)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

^d UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

Magnetohydrodynamics (MHD); Methods: numerical; Stars: activity; Sun: corona; Sun: interior; Sun: magnetic fields

Indexed keywords

ASTROPHYSICS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; NUMERICAL METHODS; PLASMAS; SATELLITES; SUN; VISCOSITY;

METHODS: NUMERICAL; STARS: ACTIVITY; SUN: CORONA; SUN: INTERIORS; SUN: MAGNETIC FIELDS;

MAGNETIC FLUX;

EID: 13744250530     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035934     Document Type: Article

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