Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/5713| Title: | WKB Analysis of Axisymmetric Magneto-Rotational Instability in a Thin Accretion Disk |
| Authors: | Furukawa, M Krishan, V Hirota, M Yoshida, Z |
| Keywords: | Magneto-rotational instability Accretion disk WKB analysis |
| Issue Date: | 2006 |
| Publisher: | The Japan Society of Plasma Science and Nuclear Fusion Research |
| Citation: | Plasma and Fusion Research, Vol. 1, pp. 001-1 - 001-2 |
| Abstract: | 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 that the oscillation of the envelope of the mode accelerates with time because of the density distribution in the direction of the disk height. |
| URI: | http://hdl.handle.net/2248/5713 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| WKB Analysis of Axisymmetric Magneto-Rotational Instability.pdf | 65.16 kB | Adobe PDF | ![]() View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.
