Multiscale Modeling of Heliospheric Plasmas
نویسنده
چکیده
A new MHD code has been developed for massively parallel computers using adaptive mesh refinement (AMR) and a new 8-wave Riemann solver. The code was implemented on a Cray T3D massively parallel computer with 512 PEs. In the first application, which modeled the expansion of the solar wind from the solar surface, the code achieved 13 GFLOPS.
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تاریخ انتشار 1997