Magnetic flux emergence into the solar photosphere and chromosphere

Astronomy and Astrophysics

Volumn 507, Issue 2, 2009, Pages 949-967

  Tortosa Andreu, A ^a   Moreno Insertis, F ^b  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD DE LA LAGUNA   (Spain)

Author keywords

Magnetohydrodynamics (MHD); Radiative transfer; Sun: chromosphere; Sun: granulation; Sun: magnetic fields; Sun: photosphere

Indexed keywords

FLUID PARTICLES; GRANULAR CONVECTION; HIGH TEMPERATURE; HORIZONTAL FIELDS; INTERGRANULAR; LAGRANGE; LAGRANGIAN; LOCAL THERMODYNAMIC EQUILIBRIUM; MAGNETIC ELEMENTS; MAGNETIC FLUX TUBE; MAGNETIZED PLASMAS; MAGNETOHYDRODYNAMICS (MHD); MECHANISM OF FORMATION; NON-RADIATIVE; NUMERICAL EXPERIMENTS; OHMIC DISSIPATION; SHOCK FRONTS; SIMULATION PREDICTION; SIMULATION RESULT; SOLAR PHOTOSPHERE; STATISTICAL SAMPLES; SUN: CHROMOSPHERE; SUN: MAGNETIC FIELD;

FLUID DYNAMICS; GRANULATION; HEATING; LAGRANGE MULTIPLIERS; MAGNETIC DOMAINS; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STRUCTURE; MAGNETOHYDRODYNAMICS; MAGNETOPLASMA; RADIATIVE TRANSFER; SIMULATORS; SUN;

EXPERIMENTS;

EID: 70450176328     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912394     Document Type: Article

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