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Massively Parallel Simulations of Solar Flares and Plasma Turbulence

Some of the outstanding problems in spaceand astrophysical plasmasystems include solar flares and hydroor magnetohydrodynamic turbulence (e.g. in the interstellar medium). Both fields demand for high resolution and thus numerical simulations need an efficient parallel implementation. We will describe the physics behind these problems and present the numerical frameworks for solving these problems on massive parallel computers.