Publication Abstracts
Canuto et al. 1984
, I. Goldman, and O. Hubickyj, 1984: A formula for the Shakura-Sunyaev turbulent viscosity parameter. Astrophys. J., 280, L55-L58, doi:10.1086/184269.
A formula for the Shakura-Sunyaev α-parameter is proposed in terms of the growth of the unstable modes driving turbulence. In the case of convective instability in a differentially rotating disk, α is given in terms of the parameters of the disk, namely T, R, ρ, and Ω.
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BibTeX Citation
@article{ca07000g,
author={Canuto, V. M. and Goldman, I. and Hubickyj, O.},
title={A formula for the Shakura-Sunyaev turbulent viscosity parameter},
year={1984},
journal={Astrophysical Journal},
volume={280},
pages={L55--L58},
doi={10.1086/184269},
}
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RIS Citation
TY - JOUR ID - ca07000g AU - Canuto, V. M. AU - Goldman, I. AU - Hubickyj, O. PY - 1984 TI - A formula for the Shakura-Sunyaev turbulent viscosity parameter JA - Astrophys. J. JO - Astrophysical Journal VL - 280 SP - L55 EP - L58 DO - 10.1086/184269 ER -
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