The Kelvin-Helmholtz instability induced by the Magneto-rotational instability in the inner-edge region of an accretion disk ; MHD simulations with CIP-MOCCT method

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ADS bibcode: 2005AGUFMSA53B1182N
year: 2005
Listed Authors: Nakamura, K.; Tandokoro, R.; Fujimoto, M.; Ida, S.
Listed Institutions: Department of Earth and Planetary Sciences Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551 Japan; Department of Earth and Planetary Sciences Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551 Japan; Department of Earth and Planetary Sciences Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551 Japan; Department of Earth and Planetary Sciences Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551 Japan

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Tokyo Institute of Technology, Department of Earth and Planetary Science