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

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dc.creatorBalbus, Steven A.
dc.creatorHawley, John F.
dc.date2006-08-21
dc.date.accessioned2026-07-07T10:39:50Z
dc.date.available2026-07-07T10:39:50Z
dc.descriptionWe 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.
dc.description22 pages, 4 figures. To appear Apj Dec 1 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0608429
dc.identifierhttp://arxiv.org/abs/astro-ph/0608429
dc.identifierAstrophys.J.652:1020-1027,2006
dc.identifierdoi:10.1086/508320
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181166
dc.subjectAstrophysics
dc.titleAn Exact, Three-Dimensional, Time-Dependent Wave Solution in Local Keplerian Flow
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