Smoothed Particle Magnetohydrodynamics - IV. Using the vector potential

Monthly Notices of the Royal Astronomical Society

Volumn 401, Issue 3, 2010, Pages 1475-1499

  Price, Daniel J ^a  

^a MONASH UNIVERSITY   (Australia)

Author keywords

Magnetic fields; Methods: numerical; MHD; Shock waves; Stars: formation

Indexed keywords

ENTROPY; EQUATIONS OF MOTION; MAGNETOHYDRODYNAMICS; NUMERICAL METHODS; VECTORS;

DIVERGENCE CONSTRAINT; EQUATION OF MOTION; MAGNETIC-FIELD; METHOD: NUMERICAL; NUMERICAL SOLUTION; SHOCK-WAVES; SMOOTHED PARTICLE HYDRODYNAMICS METHODS; STARS FORMATION; THREE DIMENSIONS; VECTOR POTENTIAL;

SHOCK WAVES;

EID: 73949112418     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15763.x     Document Type: Article

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