Publication Abstracts

Canuto 1991

Canuto, V.M., 1991: Turbulent convection: A new model. In The Sun and Cool Stars: Activity, Magnetism, Dynamos. I. Tuominen, D. Moss, and G. Rüdiger, Eds., Lecture Notes in Physics, vol. 380. Springer, pp. 27-32, doi:10.1007/3-540-53955-7_100.

We use the latest models of turbulence to compute a new expression for the turbulent convective flux, Fc. The new values of Fc are up to ten times larger than those given by the mixing length theory, MLT. Astrophysical considerations indicate that the new model fares better with observational data than the MLT.

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BibTeX Citation

@inbook{ca03810n,
  author={Canuto, V. M.},
  editor={Tuominen, I. and Moss, D. and Rüdiger, G.},
  title={Turbulent convection: A new model},
  booktitle={The Sun and Cool Stars: Activity, Magnetism, Dynamos},
  year={1991},
  volume={380},
  pages={27--32},
  publisher={Springer},
  address={Berlin},
  series={Lecture Notes in Physics},
  doi={10.1007/3-540-53955-7_100},
}

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RIS Citation

TY  - CHAP
ID  - ca03810n
AU  - Canuto, V. M.
ED  - Tuominen, I.
ED  - Moss, D.
ED  - Rüdiger, G.
PY  - 1991
TI  - Turbulent convection: A new model
BT  - The Sun and Cool Stars: Activity, Magnetism, Dynamos
T3  - Lecture Notes in Physics
VL  - 380
SP  - 27
EP  - 32
DO  - 10.1007/3-540-53955-7_100
PB  - Springer
CY  - Berlin
ER  -

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