Radial mixing in protoplanetary accretion disks. VI. Mixing by large-scale radial flows

@inproceedings{Keller2004RadialMI,
  title={Radial mixing in protoplanetary accretion disks. VI. Mixing by large-scale radial flows},
  author={Ch. A. Keller and H. Gail},
  year={2004}
}
The presence of crystalline dust materials in the outer, cold regions of protoplanetary accretion discs requires conditions for their formation, which are typical for the inner, warm regions of the disc. This suggests the existence of a mechanism that allows an efficient, outward-directed radial transport of material in accretion discs. Higher order analytical calculations, as well as numerical simulations reveal meridional flow structures in α -discs, which exhibit outflow of matter in regions… CONTINUE READING

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W. D. Addison-Wesley McComb
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