A kinetic description of the dissipative quasi-parallel solar wind termination shock

Astronomy and Astrophysics

Volumn 487, Issue 2, 2008, Pages 723-729

  Verscharen, D ^a   Fahr, H J ^a  

^a UNIVERSITY OF BONN   (Germany)

Author keywords

Magnetohydrodynamics (MHD); Plasmas; Shock waves; Solar wind

Indexed keywords

ATOMS; DIFFERENCE EQUATIONS; DIFFERENTIAL EQUATIONS; DIFFERENTIATION (CALCULUS); DISTRIBUTION FUNCTIONS; ELECTRIC FIELD EFFECTS; ELECTRIC FIELDS; ELECTROLYSIS; ELECTROMAGNETIC FIELD THEORY; ELECTROMAGNETIC FIELDS; FLOW INTERACTIONS; FOKKER PLANCK EQUATION; IONS; MAGNETIC FIELD EFFECTS; MAGNETOHYDRODYNAMICS; PARTICLE INTERACTIONS; PLASMA DIAGNOSTICS; PLASMA WAVES; PLASMAS; SEDIMENTATION; SOLAR WIND; WAVE PLASMA INTERACTIONS;

ELECTROSTATIC PLASMA WAVES; FOKKER-PLANCK; HUGONIOT; ION DISTRIBUTIONS; JUMP CONDITIONS; KINETIC ANALYSES; KINETIC APPROACH; KINETIC DESCRIPTION; MAGNETOHYDRODYNAMICS (MHD); MAIN PROCESS; RANKINE; SHOCK REGION; SHOCK WAVES; SOLAR-WIND IONS; SPATIAL SIZE; STOCHASTIC DIFFERENTIAL EQUATIONS; TERMINATION SHOCKS; TWO-STREAM INSTABILITY; WAVE-PARTICLE INTERACTIONS;

PLASMA STABILITY;

EID: 48849097286     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809950     Document Type: Article

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