Conference item
Numerical Simulations of the MRI and Real Disks
- Abstract:
- Numerical MHD codes have become extraordinarily powerful tools with which to study accretion turbulence. They have been used primarily to extract values for the classical $\alpha$ parameter, and to follow complex evolutionary development. Energy transport, which is at the heart of classical disk theory, has yet to be explored in any detail. Further topics that should be explored by simulation include nonideal MHD, radiation physics, and outburst behavior related to the temperature sensitivity of the resistivity.
- Publication status:
- Published
Actions
Authors
- Host title:
- Astrophysics of Cataclysmic Variables and Related Objects
- Volume:
- 330
- Pages:
- 185-196
- Publication date:
- 2004-11-10
- ISBN:
- 1583811931
- Keywords:
- Pubs id:
-
pubs:333906
- UUID:
-
uuid:f3fe3d6c-2d09-4bd6-b514-014cfcb9c722
- Local pid:
-
pubs:333906
- Source identifiers:
-
333906
- Deposit date:
-
2014-12-26
- ARK identifier:
Terms of use
- Copyright date:
- 2004
- Notes:
-
To appear in The Astrophysics of Cataclysmic Variables and Related
Objects, ASP Conference Series. 12 pages, 2 figures, uses asp2004.sty
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