On the Alpha-model of Turbulence
Publications of the Department of Astronomy, Tome 13 (1985) no. 1
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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_1_a3,
author = {T. Angelov},
title = {On the {Alpha-model} of {Turbulence}},
journal = {Publications of the Department of Astronomy},
pages = {27 - 30},
year = {1985},
volume = {13},
number = {1},
url = {http://geodesic.mathdoc.fr/item/PDA_1985_13_1_a3/}
}
T. Angelov. On the Alpha-model of Turbulence. Publications of the Department of Astronomy, Tome 13 (1985) no. 1. http://geodesic.mathdoc.fr/item/PDA_1985_13_1_a3/