Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...484l.161c&link_type=abstract
Astrophysical Journal Letters v.484, p.L161
Astronomy and Astrophysics
Astronomy
11
Convection, Hydrodynamics, Turbulence, Sun: Evolution, Stars: Evolution, Stars: Interiors
Scientific paper
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 Kz), 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 = K3/2l-1 (mixing length l = alpha Hp 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.
Canuto Vittorio M.
Dubovikov M.
No associations
LandOfFree
Overshooting: Mixing Length Yields Divergent Results does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Overshooting: Mixing Length Yields Divergent Results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Overshooting: Mixing Length Yields Divergent Results will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1878132