Publication Abstracts

Canuto 2011

Canuto, V.M., 2011: Stellar mixing: III. The case of a passive tracer. Astron. Astrophys., 528, A78, doi:10.1051/0004-6361/201015372.

In Papers I-II, we derived the expressions for the turbulent diffusivities of momentum, temperature T, and mean molecular weight μ. Since the scalar T-μ fields are active tracers (by influencing the density and thus the velocity field), whereas passive tracers such as 7Li are carried along by the flow without influencing it, it would be unjustified to use the diffusivities of the T-μ fields to represent the diffusivity of passive tracers. In this paper, we present the first derivation of a passive tracer diffusivity. Some key results are: a) In the general 3D case, the passive tracer diffusivity is a tensor given in algebraic form; b) the diffusivity tensor depends on shear, vorticity, T, and μ-gradients, thus including double diffusion and differential rotation; c) in the 1D version of the model, the passive tracer diffusivity is a scalar denoted by Kc; d) in doubly stable regimes, ∇μ > 0, ∇-∇ad < 0, Kc is nearly the same as those of the T-μ fields; e) in semi-convection regimes, ∇μ > 0, ∇-∇ad > 0, Kc is larger than that of the μ-field; f) in salt fingers regimes ∇μ < 0, ∇-∇ad < 0, Kc is smaller than that of the μ-field; and finally, g) in the only case we know of a direct measurement of a passive tracer diffusivity, the oceanographic North Atlantic Tracer Release Experiment (NATRE), the model reproduces the data quite closely.

Export citation: [ BibTeX ] [ RIS ]

BibTeX Citation

  author={Canuto, V. M.},
  title={Stellar mixing: III. The case of a passive tracer},
  journal={Astron. Astrophys.},

[ Close ]

RIS Citation

ID  - ca07320o
AU  - Canuto, V. M.
PY  - 2011
TI  - Stellar mixing: III. The case of a passive tracer
JA  - Astron. Astrophys.
VL  - 528
SP  - A78
DO  - 10.1051/0004-6361/201015372
ER  -

[ Close ]

• Return to 2011 Publications

• Return to Publications Homepage