Simulations of magneto-convection in the solar photosphere. Equations, methods, and results of the MURaM code

Astronomy and Astrophysics

Volumn 429, Issue 1, 2005, Pages 335-351

  Vogler A ^a   Shelyag, S ^a   Schussler M ^a   Cattaneo, F ^b   Emonet, T ^b,c   Linde, T ^b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b UNIVERSITY OF CHICAGO   (United States)

^c UNIVERSITY OF CHICAGO   (United States)

Author keywords

Magnetohydrodynamics (MHD); Sun: faculae, plages; Sun: granulation; Sun: magnetic fields; Sun: photosphere

Indexed keywords

COMPUTER SIMULATION; HEAT CONVECTION; KINETIC ENERGY; MAGNETIZATION; MAGNETOHYDRODYNAMICS; MICROPOROSITY; NUMERICAL METHODS; SUN;

SUN: FACULAE, PLAGES; SUN: GRANULATION; SUN: MAGNETIC FIELDS; SUN: PHOTOSPHERE;

ASTROPHYSICS;

EID: 11144307487     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041507     Document Type: Article

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