Furukawa, M; Krishan, V; Hirota, M; Yoshida, Z
(The Japan Society of Plasma Science and Nuclear Fusion Research, 2006)
The temporal behavior of axisymmetric magneto-rotational instability in a thin accretion disk is analyzed via the Wentzel-Kramars-Brillouin (WKB) method. The height of the thin disk is used as a small parameter. It is found ...