Astrophyscal fluid, Space, and Planets

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[1-32] Magnetohydrodynamic simulations for magnetic turbulence driven by the interaction between a relativistic shock wave and inhomogeneous media

*Kanji Morikawa¹, Yutaka Ohira¹, Takumi Ohmura^1,2 (1. The University of Tokyo, 2. National Astronomical Observatory of Japan)

Keywords:

magnetic turbulence,relativistic shock wave,dynamo,Magnetohydrodynamic simulation