Overshooting: Mixing length yields divergent results

被引:13
作者
Canuto, VM
Dubovikov, M
机构
[1] NASA Goddard Institute for Space Studies, New York, NY 10025
关键词
convection; hydrodynamics; stars; evolution; interiors; Sun; turbulence;
D O I
10.1086/310792
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Overshooting (OV) is the signature of the nonlocal nature of convection. To describe the latter, one needs five nonlocal, coupled differential equations to describe turbulent kinetic energies (total K and in the z-direction K-z), potential energy, convective flux, and rate of dissipation epsilon. We show analytically that if epsilon is assumed to be given by the local expression, epsilon = K(3/2)l(-1) (mixing length l = alpha H-p or l = z/a, since the region is small in extent), the remaining differential equations exhibit singularities (divergences) for specific values of a within the range of values usually employed. No solution can be found. Thus, OV results from such an approach are quite accidental, as they stem from an arbitrary fine tuning of a.
引用
收藏
页码:L161 / L163
页数:3
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