The universally growing mode in the solar atmosphere: Coronal heating by drift waves

Monthly Notices of the Royal Astronomical Society

Volumn 398, Issue 2, 2009, Pages 918-930

  Vranjes, J ^a   Poedts, S ^a  

^a CENTRE FOR PLASMA ASTROPHYSICS   (Belgium)

Author keywords

Sun: corona; Sun: oscillations

Indexed keywords

FREE ENERGY; HEATING; HEAVY IONS; MAGNETIC FIELDS; MAGNETOPLASMA; PLASMA WAVES; STOCHASTIC SYSTEMS;

BASIC THEORY; CORONAL HEATING; DENSITY GRADIENTS; DRIFT WAVES; MAGNETIC FIELD VECTORS; SOLAR ATMOSPHERE; STOCHASTIC HEATING; SUN : CORONA; SUN: OSCILLATIONS; WAVE THEORY;

PLASMA CONFINEMENT;

EID: 69549089719     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15180.x     Document Type: Article

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