An anisotropic turbulent model for solar coronal heating

Astronomy and Astrophysics

Volumn 490, Issue 1, 2008, Pages 325-337

  Bigot, B ^a,b   Galtier, S ^a,c   Politano, H ^b  

^a UNIVERSITÉ PARIS SUD   (France)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c INSTITUT UNIVERSITAIRE DE FRANCE   (France)

Author keywords

Magnetohydrodynamics (MHD); Sun: corona; Turbulence

Indexed keywords

AERODYNAMIC HEATING; ANISOTROPY; HEATING; HEATING RATE; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; MODEL STRUCTURES; SOLAR HEATING; TURBULENCE;

A-PRIORI; ACTIVE REGIONS; CORONAL HEATING; CORONAL HOLES; CORONAL STRUCTURES; EXACT RESULTS; HEATING EFFICIENCY; MAGNETIC LOOPS; MAGNETIC-FIELD LINES; MAGNETOHYDRODYNAMICS (MHD); SELF-CONSISTENT MODELING; SMALL-SCALE DYNAMICS; SOLAR CORONAL HEATING; SUN: CORONA; TURBULENT MODELS; TURBULENT STATE; TURBULENT VELOCITY; WAVE TURBULENCE;

TURBULENCE MODELS;

EID: 53849090667     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079227     Document Type: Article

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