Comparison of the thin flux tube approximation with 3D MHD simulations

Astronomy and Astrophysics

Volumn 504, Issue 2, 2009, Pages 595-603

  Yelles Chaouche, L ^a,b   Solanki, S K ^a,c   Schussler M ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c Kyung Hee University   (South Korea)

Author keywords

Magnetohydrodynamics (MHD); Sun: magnetic fields; Sun: photosphere

Indexed keywords

COMPARATIVE ANALYSIS; EQUIPARTITION; FIELD DISTRIBUTION; FLUX CONCENTRATION; FLUX TUBES; LENGTH SCALE; MAGNETOHYDRODYNAMICS (MHD); MHD SIMULATION; NONMAGNETICS; PHOTOSPHERIC MAGNETIC FLUXES; RADIATIVE MHD; RADIUS OF CURVATURE; SECOND ORDERS; SIMULATED STRUCTURE; STRUCTURE AND DYNAMICS; SUN: MAGNETIC FIELDS; SUN: PHOTOSPHERE; TAYLOR EXPANSIONS; TOTAL PRESSURE;

CONCENTRATION (PROCESS); FLUID DYNAMICS; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC MATERIALS; MAGNETOHYDRODYNAMICS; MODEL CHECKING; SUN;

THREE DIMENSIONAL;

EID: 70349337607     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912390     Document Type: Article

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