The pulsar force-free magnetosphere linked to its striped wind: Time-dependent pseudo-spectral simulations

Monthly Notices of the Royal Astronomical Society

Volumn 424, Issue 1, 2012, Pages 605-619

  Petri J ^a  

^a UNIVERSITÉ DE STRASBOURG   (France)

Author keywords

Magnetic fields; Methods: numerical; MHD; Plasmas; Pulsars: general

Indexed keywords

CYLINDERS (SHAPES); ELECTRIC CHARGE; ELECTRIC LOSSES; ELECTRIC POTENTIAL; ELECTROMAGNETIC FIELDS; MAGNETOPLASMA; MAGNETOSPHERE; MAXWELL EQUATIONS; NUMERICAL METHODS; PULSARS; SPHERES;

LIGHT CYLINDER; MAGNETIC-FIELD; METHOD: NUMERICAL; NEUTRON STARS; PULSARS: GENERAL; RADIATION MECHANISM; SPECTRAL SIMULATIONS; SPHERICAL GEOMETRIES; STELLARS; TIME DEPENDENT;

MAGNETOHYDRODYNAMICS;

EID: 84863542081     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.21238.x     Document Type: Article

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