Coupling from the photosphere to the chromosphere and the corona

Space Science Reviews

Volumn 144, Issue 1-4, 2009, Pages 317-350

  Wedemeyer Bohm S ^a   Lagg, A ^b   Nordlund, A ^c  

^a UNIVERSITY OF OSLO   (Norway)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

Chromosphere; Convection; Corona; Magnetohydrodynamics; Photosphere; Radiative transfer; Sun

Indexed keywords

ATMOSPHERIC LAYERS; CHROMOSPHERE; CONVECTION; CONVECTION ZONES; CORONA; DYNAMIC SYSTEMS; MAGNETIC FIELD CONFIGURATIONS; MULTI-SCALE; NUMERICAL SIMULATIONS; PHOTOSPHERE; PHYSICAL PROCESS; QUIET SUNS; SOLAR CONVECTIONS; SPATIAL SCALE;

FLUID DYNAMICS; GRANULATION; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; RADIATIVE TRANSFER;

SUN;

EID: 63949085827     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-008-9447-8     Document Type: Article

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