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Asymptotic Analyses for Atmospheric Flows and ... - FU Berlin, FB MI

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778 ZAMM · Z. angew. Math. Mech. 80 (2000) 11-12<br />

Small scale dynamics:<br />

On the small scales comparable to h sc it is found that<br />

∇ ⃗x p (0) = ∇ ⃗ξ p (0) = ∇ ⃗x p (1) ≡ 0 so that p (0) = p(z,t) , p (1) = p (1) ( ⃗ ξ,z,t) . (49)<br />

Consistent with observations, temporal variations of the background pressure p are suppressed, so that p = p(z).<br />

Next one recovers the pseudo-incompressible flow equations <strong>for</strong> stratified flows from (37), except <strong>for</strong> one<br />

modification concerning the influence of long wavelength pressure gradients. The horizontal momentum equation<br />

now reads<br />

⃗u t + ⃗u ·∇ ⃗x ⃗u + w⃗u z + 1 ρ ∇ ⃗x p (2) = ⃗ D Ro<br />

u − 1 ρ ∇ ⃗ ξ<br />

p (1) , (50)<br />

where we have included the Coriolis terms in ⃗ D Ro<br />

u<br />

to abbreviate the notation. One may expect to find the fully<br />

three-dimensional anelastic approximation from (39), plus the long wave pressure gradient term as in (50), if<br />

variations of the potential temperature are assumed to be of order O(M 2 ) only. This case was not discussed in [5].<br />

The only new effect on the small scales is thus the pressure gradient term 1 ρ ∇ ξ ⃗ p (1) , which is responsible <strong>for</strong><br />

a bulk acceleration of the fluid. Notice that the ⃗x-dependence of the second order pressure p (2) is determined by a<br />

small scale divergence constraint analogous to (37) 2 .<br />

Large scale dynamics:<br />

In a st<strong>and</strong>ard fashion, the relevant equation <strong>for</strong> the dynamics on the 1 M l refscale<br />

are obtained by horizontally averaging over the small scale coordinate ⃗x. The ⃗x-averaging operator will be<br />

abbreviated by 〈·〉. The large scale dynamics involves three variables, namely the long wave pressure mode p (1) ,<br />

the averaged vertical component of vorticity ζ = ⃗ k ·∇ ⃗ξ<br />

×〈⃗u (0) 〉, <strong>and</strong> the averaged first order vertical velocity<br />

w (1) = 〈w (1) 〉. The long wavelength dynamical equations <strong>for</strong> the considered regime read<br />

( ∂2<br />

∂t 2 − c2 ∇ ⃗ξ 2 ) p (1) = (1− c 2 ∂ ∂z ) ∂ ∂t (ρ w(1) ) − c 2 ζ + Q p (1) ,<br />

N 2 c 2 (ρ w (1) ) = −(1 + c 2 ∂ ∂z ) ∂ ∂t<br />

p (1) + Q ρw (1) ,<br />

(51)<br />

∂<br />

∂t ζ = 1<br />

c 2 ∂<br />

∂t p(1) + ∂ ∂z (ρ w(1) ) + Q ζ<br />

.<br />

Here Q i are inhomogeneous terms that combine the effects of small scale averages of nonlinear terms, <strong>and</strong> of the<br />

momentum <strong>and</strong> energy inhomogeneities ⃗ D v ,D p from (1). The system in (51) supports internal gravity waves, long<br />

wave acoustics, <strong>and</strong> the Lamb wave. It represents the link between the multiple length scale asymptotics from [5]<br />

<strong>and</strong> classical analyses <strong>for</strong> small perturbations from a state of rest.<br />

We notice also that the in the stationary limit (∂/∂t ≡ 0) the first equation in (51) reduces to the pressure<br />

Poisson equation from the quasi-geostrophic theory obtained by applying the horizontal divergence ∇ ||<br />

· (·) to<br />

the geostrophic balance equation (6). Thus we verify that the Coriolis effects achieve dominant importance <strong>for</strong><br />

quasi-steady flow on the larger ⃗ ξ-scale as announced earlier.

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