On the Alpha-model of Turbulence
Publications of the Department of Astronomy, Tome 13 (1985), p. 27
Voir la notice de l'article provenant de la source eLibrary of Mathematical Institute of the Serbian Academy of Sciences and Arts
One considers the structure of stellar discs with an $\alpha$-model of turbulence. One obtains the equation of the energetic balance for turbulent pulsations and shows that $\alpha(r)$ as, in the central and peripheral parts of the disc, a monotonous, slowly increasing and bounded function. Quick changes occur in the narrow band of the disc near the star's surlace.
@article{PDA_1985_13_a3,
author = {T. Angelov},
title = {On the {Alpha-model} of {Turbulence}},
journal = {Publications of the Department of Astronomy},
pages = {27 },
publisher = {mathdoc},
volume = {13},
year = {1985},
language = {en},
url = {http://geodesic.mathdoc.fr/item/PDA_1985_13_a3/}
}
T. Angelov. On the Alpha-model of Turbulence. Publications of the Department of Astronomy, Tome 13 (1985), p. 27 . http://geodesic.mathdoc.fr/item/PDA_1985_13_a3/