Publication Abstracts
Canuto 1991
, 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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