Посилання:Initial conditions for turbulent mixing simulations / T. Kaman, J. Glimm, D.H. Sharp // Condensed Matter Physics. — 2010. — Т. 13, № 4. — С. 43401:1-7. — Бібліогр.: 15 назв. — англ.
Підтримка:It is a pleasure to thank D. Youngs for helpful comments and for sharing unpublished experimental data. This research was supported in part by the U.S. Department of Energy grants DE–FC02–06–ER25770,DE–FG07–07ID14889, DE–FC52–08NA28614 and DE–AC07–05ID14517. This work is supported by the Army Research Organization grant W911NF0910306. This manuscript has been co-authored by Brookhaven Science Associates, LLC, under Contract No. DE–AC02–98CH10886 with the U.S. Department of Energy. The United States Government retains, and the publisher, by accepting this article for publication, acknowledges, a world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for the United States Government purposes. This work has a Los Alamos Laboratory preprint number LA–UR 10–03424 and a Stony Brook University preprint number SUNYSB–AMS–10–03.
In the context of the classical Rayleigh-Taylor hydrodynamical instability, we examine the much debated question of models for initial conditions and the possible influence of unrecorded long wave length contributions to the instability growth rate α.
У контексті класичної гідродинамічної нестійкості Релея - Тейлора вивчено дискусійне питання моделей для початкових умов і можливий вплив незафіксованих далекосяжних вкладів на швидкість росту нестійкості альфа.