An Exact, Three-Dimensional, Time-Dependent Wave Solution in Local Keplerian Flow

Details An Exact, Three-Dimensional, Time-Dependent Wave Solution in Local Keplerian Flow An Exact, Three-Dimensional, Time-Dependent Wave Solution in Local Keplerian Flow

2006-08-21

arxiv.org/abs/astro-ph/0608429v1

Astrophys.J.652:1020-1027,2006

Astronomy and Astrophysics

Astrophysics

22 pages, 4 figures. To appear Apj Dec 1 2006

Scientific paper

10.1086/508320

We present an exact three-dimensional wave solution to the shearing sheet
equations of motion. The existence of this solution argues against transient
amplification as a route to turbulence in unmagnetized disks. Moreover, because
the solution covers an extensive dynamical range in wavenumber space, it is an
excellent test of the dissipative properties of numerical codes.

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