Beyond ideal MHD: Towards a more realistic modelling of relativistic astrophysical plasmas

Monthly Notices of the Royal Astronomical Society

Volumn 394, Issue 4, 2009, Pages 1727-1740

  Palenzuela, Carlos ^a   Lehner, Luis ^b   Reula, Oscar ^c   Rezzolla, Luciano ^a,b  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b LOUISIANA STATE UNIVERSITY   (United States)

^c UNIVERSIDAD NACIONAL DE CÓRDOBA   (Argentina)

Author keywords

Methods; MHD; Numerical; Plasmas; Relativity

Indexed keywords

ASTROPHYSICS; MAGNETOPLASMA; MAGNETOSPHERE; NUMERICAL METHODS; RUNGE KUTTA METHODS;

ASTROPHYSICAL PLASMA; MAGNETIC-FIELD; METHOD; NUMERICAL; NUMERICAL SOLUTION; QUASI-STATIONARY; REALISTIC MODEL; RELATIVISTICS; RESISTIVE EFFECTS; STATIONARY PROCESS;

MAGNETOHYDRODYNAMICS;

EID: 67849131204     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14454.x     Document Type: Article

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