The main features of a numerical code for astrophysical fluids and magneto-fluids named ECHO (Eulerian conservative high-order) are presented. Here the module for special and general relativistic MHD is discussed and applications of the code to astrophysical problems are summarized.
The ECHO code for astrophysical plasmas: special and general relativistic MHD / L. Del Zanna; S. Landi; O. Zanotti; N. Bucciantini; P. Londrillo. - In: NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. C, GEOPHYSICS AND SPACE PHYSICS. - ISSN 1826-9885. - STAMPA. - 32:(2009), pp. 109-113. [10.1393/ncc/i2009-10385-8]
The ECHO code for astrophysical plasmas: special and general relativistic MHD.
DEL ZANNA, LUCA;LANDI, SIMONE;
2009
Abstract
The main features of a numerical code for astrophysical fluids and magneto-fluids named ECHO (Eulerian conservative high-order) are presented. Here the module for special and general relativistic MHD is discussed and applications of the code to astrophysical problems are summarized.File in questo prodotto:
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