Supersonic solar wind ion flows downstream of the termination shock explained by a two-fluid shock model

Astronomy and Astrophysics

Volumn 490, Issue 3, 2008, Pages

  Fahr, H J ^a   Chalov, S V ^b  

^a UNIVERSITY OF BONN   (Germany)

^b INSTITUTE FOR PROBLEMS IN MECHANICS   (Russian Federation)

Author keywords

Hydrodynamics; Shock waves; Solar wind

Indexed keywords

DIGITAL SIGNAL PROCESSING; ELECTROLYSIS; FLUID DYNAMICS; HYDRODYNAMICS; IONS; MACH NUMBER; MAGNETIC FIELD EFFECTS; MAGNETOHYDRODYNAMICS; PLASMA FLOW; PLASMAS; RIVERS; SOLAR ENERGY; SOLAR WIND;

DOWNSTREAM; DOWNSTREAM FLOWS; FLUID SHOCKS; ION FLOWS; ION PRESSURES; SHOCK STRUCTURES; TERMINATION SHOCKS; TWO-FLUID MODELS; UPSTREAM FLOWS;

WIND POWER;

EID: 54949141197     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810679     Document Type: Article

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