Magnetohydrodynamic Simulations of High-Beta Disks and Low-Beta Disks View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1999

AUTHORS

Takaaki Matsuzaki , Kazunari Shibata , Toshiki Tajima , Ryoji Matsumoto

ABSTRACT

We present results of three-dimensional MHD simulations of Keplerian accretion disks which indicate that accretion disks have two distinct states; a gas pressure dominated quasi-steady state and a magnetic pressure dominated cataclysmic state.

PAGES

235-236

Book

TITLE

Numerical Astrophysics

ISBN

978-94-010-6008-0
978-94-011-4780-4

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-011-4780-4_77

DOI

http://dx.doi.org/10.1007/978-94-011-4780-4_77

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1053397443


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