Kinetic cascade beyond magnetohydrodynamics of solar wind turbulence in two-dimensional hybrid simulations

Physics of Plasmas

Volumn 19, Issue 2, 2012, Pages

  Verscharen, D ^a,b   Marsch, E ^a   Motschmann, U ^b,c   Muller J ^b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b TECHNICAL UNIVERSITY OF BRAUNSCHWEIG   (Germany)

^c GERMAN AEROSPACE CENTER DLR   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

BACKGROUND FIELD; DISSIPATIVE EFFECTS; ENERGY CASCADE; HYBRID SIMULATION; KINETIC REGIME; KOLMOGOROV; MASSLESS ELECTRONS; N-WAVES; NORMAL MODES; PROPAGATION DIRECTION; RESONANT ABSORPTION; SOLAR-WIND TURBULENCE; SPECTRAL RANGE; TURBULENT SPECTRUM; TWO DIMENSIONAL MODEL; WAVE NUMBERS; WAVE VECTOR; WEAK TURBULENCE; WHISTLER WAVES; WIND CONDITIONS;

ELECTRON BEAMS; KINETICS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; PLASMA WAVES; SOLAR WIND; SPECTRUM ANALYSIS; TWO DIMENSIONAL;

SLOW WAVE STRUCTURES;

EID: 84857862004     PISSN: 1070664X     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.3682960     Document Type: Article

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