Length-scale estimates for the LANS- α equations in terms of the Reynolds number
Foias, Holm and Titi [C. Foias, D.D. Holm, E.S. Titi, The three dimensional viscous Camassa–Holm equations and their relation to the Navier–Stokes equations and turbulence theory, J. Dynam. Differential Equations 14 (2002) 1–35] have settled the problem of existence and uniqueness for the 3D LANS- α...
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Veröffentlicht in: | Physica. D 2006-08, Vol.220 (1), p.69-78 |
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Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
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Zusammenfassung: | Foias, Holm and Titi [C. Foias, D.D. Holm, E.S. Titi, The three dimensional viscous Camassa–Holm equations and their relation to the Navier–Stokes equations and turbulence theory, J. Dynam. Differential Equations 14 (2002) 1–35] have settled the problem of existence and uniqueness for the 3D LANS-
α
equations on periodic box
[
0
,
L
]
3
. There still remains the problem, first introduced by Doering and Foias [C.R. Doering, C. Foias, Energy dissipation in body-forced turbulence, J. Fluid Mech. 467 (2002) 289–306] for the Navier–Stokes equations, of obtaining estimates in terms of the Reynolds number
R
e
, whose character depends on the fluid response, as opposed to the Grashof number, whose character depends on the forcing.
R
e
is defined as
R
e
=
U
ℓ
/
ν
where
U
is a bounded spatio-temporally averaged Navier–Stokes velocity field and
ℓ
the characteristic scale of the forcing. It is found that the inverse Kolmogorov length is estimated by
ℓ
λ
k
−
1
≤
c
(
ℓ
/
α
)
1
/
4
R
e
5
/
8
. Moreover, the estimate of Foias, Holm and Titi for the fractal dimension of the global attractor, in terms of
R
e
, comes out to be
d
F
(
A
)
≤
c
V
α
V
ℓ
1
/
2
(
L
2
λ
1
)
9
/
8
R
e
9
/
4
where
V
α
=
(
L
/
(
ℓ
α
)
1
/
2
)
3
and
V
ℓ
=
(
L
/
ℓ
)
3
. It is also shown that there exists a series of time-averaged inverse squared length scales whose members,
〈
κ
n
,
0
2
〉
, are estimated as
(
n
≥
1
)
ℓ
2
〈
κ
n
,
0
2
〉
≤
c
n
,
α
V
α
n
−
1
n
R
e
11
4
−
7
4
n
(
ln
R
e
)
1
n
+
c
1
R
e
(
ln
R
e
)
.
The upper bound on the first member of the hierarchy
〈
κ
1
,
0
2
〉
coincides with the inverse squared Taylor micro-scale to within log-corrections. |
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ISSN: | 0167-2789 1872-8022 |
DOI: | 10.1016/j.physd.2006.06.012 |