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- W1984398910 abstract "Abstract It is known that a turbulent, two-dimensional fluid at high Reynolds number under a suitable restoring force can evolve toward larger scales, that is, to waves and zonal jets. A two-dimensional disk of turbulent fluid gravitationally bound to a central mass is considered as a model for a pre-planetary disk. It is found that for general conditions, azimuthal zonal jets can form in the disk. Planetesimals are assumed to accrete between these jets. Their radial separation distances, s(r), should be roughly s(r)∼ π{[e/(1 - e 2)]}1/2 r, where e is orbital eccentricity, and r is semimajor radius. In the corotating reference frame, jets alternate in direction, forming counterstreaming pairs. For eccentricities comparable to Solar System planetary orbital eccentricities, jet pair separations roughly double with each successive jet pair. The predicted spacings are in better agreement with observation than predicitions by the Titius-Bode(TB) Rule. This model predicts that TB-like spacing should be common in extra-solar planetary systems." @default.
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- W1984398910 date "1994-12-01" @default.
- W1984398910 modified "2023-09-25" @default.
- W1984398910 title "A turbulent fluid model for the evolution of zonal jets in a pre-planetary nebular disk" @default.
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- W1984398910 doi "https://doi.org/10.1080/03091929408226579" @default.
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