A Model of Self-sustaining Magnetic Dynamo in Accretion Disks
- 10.2991/mcei-17.2017.66How to use a DOI?
- accretion;accretion disks;magnetic reconnection;magnetic field;magnetic dynamo
This paper put forward a model of magnetic dynamo which similar to the model of C.A.Tout and J.E.Pringle, it explains the movement way of magnetic dynamo in accretion disks and the main principle also are the instability of the Parker, the instability of the Balbus-Hawley and the reconnection. The difference is that the Petschek reconnection is substituted into Sweet-Parker reconnection, it can also form a self-sustaining magnetic dynamo.
- © 2017, the Authors. Published by Atlantis Press.
- Open Access
- This is an open access article distributed under the CC BY-NC license (http://creativecommons.org/licenses/by-nc/4.0/).
Cite this article
TY - CONF AU - Hongliang Zhao AU - Bo Jiang AU - Li Wang PY - 2017/12 DA - 2017/12 TI - A Model of Self-sustaining Magnetic Dynamo in Accretion Disks BT - Proceedings of the 2017 7th International Conference on Mechatronics, Computer and Education Informationization (MCEI 2017) PB - Atlantis Press SP - 304 EP - 308 SN - 2352-538X UR - https://doi.org/10.2991/mcei-17.2017.66 DO - 10.2991/mcei-17.2017.66 ID - Zhao2017/12 ER -