The gravity wave drag parameterization used at NMC is a fairly crude approximation of gravity waves forced by flow over topography. The surface flux parameterization follows Pierrehumbert (1987). With respect to the vertical deposition of momentum, we favor the saturation flux method (Lindzen, 1981) of depositing the momentum vertically after studying comparisons with a linear deposition. As described below, critical layers, the degree of instability and other processes contribute to the vertical momentum deposition within the saturation flux method. An attempt is made to include these contributions.
In interior layers of the atmosphere, if no absorption occurs, the stress is constant with height and no momentum deposition occurs. At the highest sigma layer, any remaining stress is deposited. Otherwise the stress is not absorbed with height until either 1) a critical level is encountered at which point the momentum flux vanishes or 2) the gravity waves break and generate turbulence from shear or convective instability or 3) from wave saturation. Once the gravity wave begins to break the wave saturation hypothesis of Lindzen (1981) is invoked. That is, the waveinduced turbulent dissipation prevents the displacement amplitude from exceeding its critical value, in this case 1 - 1/(4Ri), where Ri is the Richardson number. The Froude number, Fr, and the Richardson number of the mean state of the atmosphere, Ri, are related to the wave modified Richardson number, Rm, as Rm = Ri - Ri Fr. If the critical value of the wave-modified Richardson number is chosen to be 1/4, the above criteria results. This is discussed in more detail below, in terms of application to the NMC spectral model.
The drag due to sub-grid scale momentum flux appears as an additional body force on the right hand side of the momentum equation of the model. The starting point is the momentum eqn from page . The velocity tendency equation is modified by the vertical derivative of the gravity wave induced stress:
where is surface pressure.
The prognostic equations for momentum, in the NMC spectral model, (see Sela, 1982, 1987) are in the form of tendencies of vorticity and divergence. The relevant part for this section can be represented as:
where A and B are the velocity tendencies and include the vertical diffusion of momentum. The vertical flux of momentum due to gravity wave drag is incorporated in the model by modifying A and B to become:
in eqn. (6.2).
The vertical derivative of the stress is written in difference form as
where SI(k) is the index for model sigma interface levels and SL(k) is the index for the model sigma layers.
Based on linear, two-dimensional non-rotating, stably stratified flow over a ridge, gravity wave motions are set up which propagate away from the mountain. The flux measured from a low level in the atmosphere is defined to be the base level flux. It is taken to be the first 1/3 of the atmosphere but this choice is arbitrary. The vertical momentum flux or gravity wave stress in a grid box due to a single mountain is given as in PH:
where is a grid increment, N is the Brunt Viasala frequency given as
The environmental variables are calculated from a mass weighted vertical average over the base layer. In eqn. (6.5) G(Fr) is a monotonically increasing function of Froude number, , where U is the wind speed calculated as a mass weighted vertical average in the base layer, and , is the vertical displacement caused by the orography variance. An effective mountain length, where m is the number of mountains in a grid box, can then be defined to obtain the form of the base level stress used in the computation as shown in eqn. (6.7).
giving the stress in a grid box. PH gives the form for the function G as
where is an order unity non-dimensional saturation flux set to 1.0 and 'a' is a function
of the mountain aspect ratio. Typical values of U=10m/s, N=, = 100km, and a =
1 give a flux of 1 Pascal. If this flux goes to zero linearly with height, then the deceleration
would be about 10m/s, which is consistent with numerous observations (see Table 1 in PH).
In Fig. 6.1, the universal flux function, G, is shown as a function of Froude number and
mountain shape parameters . A value of 1.0 for 'a' has been used in the
When breaking occurs for some layer in the free atmosphere, the stress at the next lower layer is known, beginning with the base level flux described in (6.7). It should be noted that this representation of the stress (6.7), under a binomial expansion for small Froude number, is identical to that used in the free atmosphere in PSS:
with , where is an inverse length scale parameter given as in the PSS formulation.
Following Helfand et. al. (1987) and PSS wave breaking occurs at the level where the amplification of the wave causes the local Froude number to exceed the critical value
where is the critical vertical displacement amplitude for a wave in the free atmosphere which is about to break. This means that a shear instability is assumed to occur at Ri<1/4. PH points out that a criteria for shear instability is difficult to determine and convective breaking (Ri<0) criterion is usually satisfied before that of shear breaking. Both of the above criteria are used in the present parameterization. However, if Ri<0 occurs in the base level, then no deposition takes place.
Once it is determined that some wave breaking is to occur, the vertical structure of the stress is reduced so that the wave-induced turbulent dissipation prevents the displacement amplitude, , from exceeding its critical value. This is measured by the ratio of the critical and locally calculated Froude numbers described above. The gravity wave momentum flux should be reduced by a factor when the Froude number exceeds its critical value. Using (6.9) we can rewrite the Froude number at interface in terms of the stress of the interface layer below the one under consideration, , as
As a result the vertical profile of the momentum flux is built up from the base level stress as a function of local values of N, U and the particle displacement. The gravity wave drag-induced velocity tendency change is computed as the vertical divergence of the momentum flux as described above in eqns. (6.3, 6.4).
Another option independently allows for a linear interpolation of the vertical stress profile to begin at an arbitrary layer LCAP and extend to the model top sigma layer. This option allows a linear profile to be imposed in part or entirely throughout the atmosphere. Linear profiles of the vertical stress function have been used with success on the NMC Nested Grid Model, and at other NWP centers.
The scheme is composed of subroutines, V3GWD, where basic values and base level stress are calculated, as well as the base level stress and velocity tendencies, and GWDRAG which receives the input from V3GWD and returns the vertical structure of the stress. The changes to the velocity tendency are calculated from the vertical stress profile calculated in GWDRAG. Within the base layer, no gravity wave deposition is allowed if a critical layer or instability takes place. The base layer is assigned as the layers below 667mb. The parameter KBPS indicates the sigma level where the saturation flux hypothesis is to be used. Below this level a linear stress profile is fit to the bottom stress value. The current default value for KBPS is 2. The parameter LCAP is used to replace the saturation flux hypothesis with a linear profile extending from sigma layer LCAP to the top of the model atmosphere. Changes to the control variables NUM and CON may be used to alter the parameterization (see Chapter 8). Fig. 6.2 shows sigma interfaces and levels of the current 18 layer model. The base level averages of variables on sigma layers and interfaces have been treated separately. The result is that stress is defined on an interface while the velocity tendency is in sigma layers. The variables, symbols in the subroutine calls are shown in Table 6.1.
List of variables and symbols passed between the subroutines.
Sigma coordinate approximate pressure (mb) Interface Layer
19 _______________ 000
(KDIM) 18 --------------- T, u, v, A, B 021
18 _______________ , Ri, Vg, Fr 050
. . . .
. . . .
. . . .
KSM _______________ , Ri, Vg, Fr
KSM --------------- T, u, v, A, B
. . . .
. . . .
4 _______________ , Ri, Vg, Fr 948
3 --------------- T, u, v, A, B 960
3 _______________ , Ri, Vg, Fr 973
2 --------------- T, u, v, A, B 981 (KBPS)
2 _______________ , Ri, Vg, Fr 990
1 --------------- T, u, v, A, B 995
1 _______________ , Ri, Vg, Fr 1000
Figure 6.2: Model vertical structure as it applies to the gravity wave drag parameterization
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