9 |
HPE's for the ocean written in z-coordinates are obtained. The |
HPE's for the ocean written in z-coordinates are obtained. The |
10 |
non-Boussinesq equations for oceanic motion are: |
non-Boussinesq equations for oceanic motion are: |
11 |
\begin{eqnarray} |
\begin{eqnarray} |
12 |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}}% |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}} |
13 |
_{h}+\frac{1}{\rho }\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
_{h}+\frac{1}{\rho }\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
14 |
\label{eq-zns-hmom} \\ |
\\ |
15 |
\epsilon _{nh}\frac{Dw}{Dt}+g+\frac{1}{\rho }\frac{\partial p}{\partial z} |
\epsilon _{nh}\frac{Dw}{Dt}+g+\frac{1}{\rho }\frac{\partial p}{\partial z} |
16 |
&=&\epsilon _{nh}\mathcal{F}_{w} \label{eq-zns-hydro} \\ |
&=&\epsilon _{nh}\mathcal{F}_{w} \\ |
17 |
\frac{1}{\rho }\frac{D\rho }{Dt}+\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}% |
\frac{1}{\rho }\frac{D\rho }{Dt}+\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}} |
18 |
_{h}+\frac{\partial w}{\partial z} &=&0 \label{eq-zns-cont} \\ |
_{h}+\frac{\partial w}{\partial z} &=&0 \\ |
19 |
\rho &=&\rho (\theta ,S,p) \label{eq-zns-eos} \\ |
\rho &=&\rho (\theta ,S,p) \\ |
20 |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-zns-heat} \\ |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \\ |
21 |
\frac{DS}{Dt} &=&\mathcal{Q}_{s} \label{eq-zns-salt} |
\frac{DS}{Dt} &=&\mathcal{Q}_{s} |
22 |
|
\label{eq:non-boussinesq} |
23 |
\end{eqnarray} |
\end{eqnarray} |
24 |
These equations permit acoustics modes, inertia-gravity waves, |
These equations permit acoustics modes, inertia-gravity waves, |
25 |
non-hydrostatic motions, a geostrophic (Rossby) mode and a thermo-haline |
non-hydrostatic motions, a geostrophic (Rossby) mode and a thermo-haline |
41 |
reciprocal of the sound speed ($c_{s}$) squared. Substituting into \ref |
reciprocal of the sound speed ($c_{s}$) squared. Substituting into \ref |
42 |
{eq-zns-cont} gives: |
{eq-zns-cont} gives: |
43 |
\begin{equation} |
\begin{equation} |
44 |
\frac{1}{\rho c_{s}^{2}}\frac{Dp}{Dt}+\mathbf{\nabla }_{z}\cdot \vec{\mathbf{% |
\frac{1}{\rho c_{s}^{2}}\frac{Dp}{Dt}+\mathbf{\nabla }_{z}\cdot \vec{\mathbf{ |
45 |
v}}+\partial _{z}w\approx 0 \label{eq-zns-pressure} |
v}}+\partial _{z}w\approx 0 \label{eq-zns-pressure} |
46 |
\end{equation} |
\end{equation} |
47 |
where we have used an approximation sign to indicate that we have assumed |
where we have used an approximation sign to indicate that we have assumed |
49 |
Replacing \ref{eq-zns-cont} with \ref{eq-zns-pressure} yields a system that |
Replacing \ref{eq-zns-cont} with \ref{eq-zns-pressure} yields a system that |
50 |
can be explicitly integrated forward: |
can be explicitly integrated forward: |
51 |
\begin{eqnarray} |
\begin{eqnarray} |
52 |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}}% |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}} |
53 |
_{h}+\frac{1}{\rho }\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
_{h}+\frac{1}{\rho }\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
54 |
\label{eq-cns-hmom} \\ |
\label{eq-cns-hmom} \\ |
55 |
\epsilon _{nh}\frac{Dw}{Dt}+g+\frac{1}{\rho }\frac{\partial p}{\partial z} |
\epsilon _{nh}\frac{Dw}{Dt}+g+\frac{1}{\rho }\frac{\partial p}{\partial z} |
56 |
&=&\epsilon _{nh}\mathcal{F}_{w} \label{eq-cns-hydro} \\ |
&=&\epsilon _{nh}\mathcal{F}_{w} \label{eq-cns-hydro} \\ |
57 |
\frac{1}{\rho c_{s}^{2}}\frac{Dp}{Dt}+\mathbf{\nabla }_{z}\cdot \vec{\mathbf{% |
\frac{1}{\rho c_{s}^{2}}\frac{Dp}{Dt}+\mathbf{\nabla }_{z}\cdot \vec{\mathbf{ |
58 |
v}}_{h}+\frac{\partial w}{\partial z} &=&0 \label{eq-cns-cont} \\ |
v}}_{h}+\frac{\partial w}{\partial z} &=&0 \label{eq-cns-cont} \\ |
59 |
\rho &=&\rho (\theta ,S,p) \label{eq-cns-eos} \\ |
\rho &=&\rho (\theta ,S,p) \label{eq-cns-eos} \\ |
60 |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-cns-heat} \\ |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-cns-heat} \\ |
68 |
`Boussinesq assumption'. The only term that then retains the full variation |
`Boussinesq assumption'. The only term that then retains the full variation |
69 |
in $\rho $ is the gravitational acceleration: |
in $\rho $ is the gravitational acceleration: |
70 |
\begin{eqnarray} |
\begin{eqnarray} |
71 |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}}% |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}} |
72 |
_{h}+\frac{1}{\rho _{o}}\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
_{h}+\frac{1}{\rho _{o}}\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
73 |
\label{eq-zcb-hmom} \\ |
\label{eq-zcb-hmom} \\ |
74 |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho }{\rho _{o}}+\frac{1}{\rho _{o}}% |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho }{\rho _{o}}+\frac{1}{\rho _{o}} |
75 |
\frac{\partial p}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
\frac{\partial p}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
76 |
\label{eq-zcb-hydro} \\ |
\label{eq-zcb-hydro} \\ |
77 |
\frac{1}{\rho _{o}c_{s}^{2}}\frac{Dp}{Dt}+\mathbf{\nabla }_{z}\cdot \vec{% |
\frac{1}{\rho _{o}c_{s}^{2}}\frac{Dp}{Dt}+\mathbf{\nabla }_{z}\cdot \vec{ |
78 |
\mathbf{v}}_{h}+\frac{\partial w}{\partial z} &=&0 \label{eq-zcb-cont} \\ |
\mathbf{v}}_{h}+\frac{\partial w}{\partial z} &=&0 \label{eq-zcb-cont} \\ |
79 |
\rho &=&\rho (\theta ,S,p) \label{eq-zcb-eos} \\ |
\rho &=&\rho (\theta ,S,p) \label{eq-zcb-eos} \\ |
80 |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-zcb-heat} \\ |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-zcb-heat} \\ |
86 |
term appears as a Helmholtz term in the non-hydrostatic pressure equation). |
term appears as a Helmholtz term in the non-hydrostatic pressure equation). |
87 |
These are the \emph{truly} compressible Boussinesq equations. Note that the |
These are the \emph{truly} compressible Boussinesq equations. Note that the |
88 |
EOS must have the same pressure dependency as the linearized pressure term, |
EOS must have the same pressure dependency as the linearized pressure term, |
89 |
ie. $\left. \frac{\partial \rho }{\partial p}\right| _{\theta ,S}=\frac{1}{% |
ie. $\left. \frac{\partial \rho }{\partial p}\right| _{\theta ,S}=\frac{1}{ |
90 |
c_{s}^{2}}$, for consistency. |
c_{s}^{2}}$, for consistency. |
91 |
|
|
92 |
\subsubsection{`Anelastic' z-coordinate equations} |
\subsubsection{`Anelastic' z-coordinate equations} |
93 |
|
|
94 |
The anelastic approximation filters the acoustic mode by removing the |
The anelastic approximation filters the acoustic mode by removing the |
95 |
time-dependency in the continuity (now pressure-) equation (\ref{eq-zcb-cont}% |
time-dependency in the continuity (now pressure-) equation (\ref{eq-zcb-cont} |
96 |
). This could be done simply by noting that $\frac{Dp}{Dt}\approx -g\rho _{o}% |
). This could be done simply by noting that $\frac{Dp}{Dt}\approx -g\rho _{o} |
97 |
\frac{Dz}{Dt}=-g\rho _{o}w$, but this leads to an inconsistency between |
\frac{Dz}{Dt}=-g\rho _{o}w$, but this leads to an inconsistency between |
98 |
continuity and EOS. A better solution is to change the dependency on |
continuity and EOS. A better solution is to change the dependency on |
99 |
pressure in the EOS by splitting the pressure into a reference function of |
pressure in the EOS by splitting the pressure into a reference function of |
104 |
Remembering that the term $\frac{Dp}{Dt}$ in continuity comes from |
Remembering that the term $\frac{Dp}{Dt}$ in continuity comes from |
105 |
differentiating the EOS, the continuity equation then becomes: |
differentiating the EOS, the continuity equation then becomes: |
106 |
\[ |
\[ |
107 |
\frac{1}{\rho _{o}c_{s}^{2}}\left( \frac{Dp_{o}}{Dt}+\epsilon _{s}\frac{% |
\frac{1}{\rho _{o}c_{s}^{2}}\left( \frac{Dp_{o}}{Dt}+\epsilon _{s}\frac{ |
108 |
Dp^{\prime }}{Dt}\right) +\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+% |
Dp^{\prime }}{Dt}\right) +\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+ |
109 |
\frac{\partial w}{\partial z}=0 |
\frac{\partial w}{\partial z}=0 |
110 |
\] |
\] |
111 |
If the time- and space-scales of the motions of interest are longer than |
If the time- and space-scales of the motions of interest are longer than |
112 |
those of acoustic modes, then $\frac{Dp^{\prime }}{Dt}<<(\frac{Dp_{o}}{Dt},% |
those of acoustic modes, then $\frac{Dp^{\prime }}{Dt}<<(\frac{Dp_{o}}{Dt}, |
113 |
\mathbf{\nabla }\cdot \vec{\mathbf{v}}_{h})$ in the continuity equations and |
\mathbf{\nabla }\cdot \vec{\mathbf{v}}_{h})$ in the continuity equations and |
114 |
$\left. \frac{\partial \rho }{\partial p}\right| _{\theta ,S}\frac{% |
$\left. \frac{\partial \rho }{\partial p}\right| _{\theta ,S}\frac{ |
115 |
Dp^{\prime }}{Dt}<<\left. \frac{\partial \rho }{\partial p}\right| _{\theta |
Dp^{\prime }}{Dt}<<\left. \frac{\partial \rho }{\partial p}\right| _{\theta |
116 |
,S}\frac{Dp_{o}}{Dt}$ in the EOS (\ref{EOSexpansion}). Thus we set $\epsilon |
,S}\frac{Dp_{o}}{Dt}$ in the EOS (\ref{EOSexpansion}). Thus we set $\epsilon |
117 |
_{s}=0$, removing the dependency on $p^{\prime }$ in the continuity equation |
_{s}=0$, removing the dependency on $p^{\prime }$ in the continuity equation |
118 |
and EOS. Expanding $\frac{Dp_{o}(z)}{Dt}=-g\rho _{o}w$ then leads to the |
and EOS. Expanding $\frac{Dp_{o}(z)}{Dt}=-g\rho _{o}w$ then leads to the |
119 |
anelastic continuity equation: |
anelastic continuity equation: |
120 |
\begin{equation} |
\begin{equation} |
121 |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{\partial w}{\partial z}-% |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{\partial w}{\partial z}- |
122 |
\frac{g}{c_{s}^{2}}w=0 \label{eq-za-cont1} |
\frac{g}{c_{s}^{2}}w=0 \label{eq-za-cont1} |
123 |
\end{equation} |
\end{equation} |
124 |
A slightly different route leads to the quasi-Boussinesq continuity equation |
A slightly different route leads to the quasi-Boussinesq continuity equation |
125 |
where we use the scaling $\frac{\partial \rho ^{\prime }}{\partial t}+% |
where we use the scaling $\frac{\partial \rho ^{\prime }}{\partial t}+ |
126 |
\mathbf{\nabla }_{3}\cdot \rho ^{\prime }\vec{\mathbf{v}}<<\mathbf{\nabla }% |
\mathbf{\nabla }_{3}\cdot \rho ^{\prime }\vec{\mathbf{v}}<<\mathbf{\nabla } |
127 |
_{3}\cdot \rho _{o}\vec{\mathbf{v}}$ yielding: |
_{3}\cdot \rho _{o}\vec{\mathbf{v}}$ yielding: |
128 |
\begin{equation} |
\begin{equation} |
129 |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{1}{\rho _{o}}\frac{% |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{1}{\rho _{o}}\frac{ |
130 |
\partial \left( \rho _{o}w\right) }{\partial z}=0 \label{eq-za-cont2} |
\partial \left( \rho _{o}w\right) }{\partial z}=0 \label{eq-za-cont2} |
131 |
\end{equation} |
\end{equation} |
132 |
Equations \ref{eq-za-cont1} and \ref{eq-za-cont2} are in fact the same |
Equations \ref{eq-za-cont1} and \ref{eq-za-cont2} are in fact the same |
135 |
\frac{1}{\rho _{o}}\frac{\partial \rho _{o}}{\partial z}=\frac{-g}{c_{s}^{2}} |
\frac{1}{\rho _{o}}\frac{\partial \rho _{o}}{\partial z}=\frac{-g}{c_{s}^{2}} |
136 |
\end{equation} |
\end{equation} |
137 |
Again, note that if $\rho _{o}$ is evaluated from prescribed $\theta _{o}$ |
Again, note that if $\rho _{o}$ is evaluated from prescribed $\theta _{o}$ |
138 |
and $S_{o}$ profiles, then the EOS dependency on $p_{o}$ and the term $\frac{% |
and $S_{o}$ profiles, then the EOS dependency on $p_{o}$ and the term $\frac{ |
139 |
g}{c_{s}^{2}}$ in continuity should be referred to those same profiles. The |
g}{c_{s}^{2}}$ in continuity should be referred to those same profiles. The |
140 |
full set of `quasi-Boussinesq' or `anelastic' equations for the ocean are |
full set of `quasi-Boussinesq' or `anelastic' equations for the ocean are |
141 |
then: |
then: |
142 |
\begin{eqnarray} |
\begin{eqnarray} |
143 |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}}% |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}} |
144 |
_{h}+\frac{1}{\rho _{o}}\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
_{h}+\frac{1}{\rho _{o}}\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
145 |
\label{eq-zab-hmom} \\ |
\label{eq-zab-hmom} \\ |
146 |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho }{\rho _{o}}+\frac{1}{\rho _{o}}% |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho }{\rho _{o}}+\frac{1}{\rho _{o}} |
147 |
\frac{\partial p}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
\frac{\partial p}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
148 |
\label{eq-zab-hydro} \\ |
\label{eq-zab-hydro} \\ |
149 |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{1}{\rho _{o}}\frac{% |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{1}{\rho _{o}}\frac{ |
150 |
\partial \left( \rho _{o}w\right) }{\partial z} &=&0 \label{eq-zab-cont} \\ |
\partial \left( \rho _{o}w\right) }{\partial z} &=&0 \label{eq-zab-cont} \\ |
151 |
\rho &=&\rho (\theta ,S,p_{o}(z)) \label{eq-zab-eos} \\ |
\rho &=&\rho (\theta ,S,p_{o}(z)) \label{eq-zab-eos} \\ |
152 |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-zab-heat} \\ |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-zab-heat} \\ |
159 |
technically, to also remove the dependence of $\rho $ on $p_{o}$. This would |
technically, to also remove the dependence of $\rho $ on $p_{o}$. This would |
160 |
yield the ``truly'' incompressible Boussinesq equations: |
yield the ``truly'' incompressible Boussinesq equations: |
161 |
\begin{eqnarray} |
\begin{eqnarray} |
162 |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}}% |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}} |
163 |
_{h}+\frac{1}{\rho _{c}}\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
_{h}+\frac{1}{\rho _{c}}\mathbf{\nabla }_{z}p &=&\vec{\mathbf{\mathcal{F}}} |
164 |
\label{eq-ztb-hmom} \\ |
\label{eq-ztb-hmom} \\ |
165 |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho }{\rho _{c}}+\frac{1}{\rho _{c}}% |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho }{\rho _{c}}+\frac{1}{\rho _{c}} |
166 |
\frac{\partial p}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
\frac{\partial p}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
167 |
\label{eq-ztb-hydro} \\ |
\label{eq-ztb-hydro} \\ |
168 |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{\partial w}{\partial z} |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{\partial w}{\partial z} |
193 |
This then yields what we can call the semi-compressible Boussinesq |
This then yields what we can call the semi-compressible Boussinesq |
194 |
equations: |
equations: |
195 |
\begin{eqnarray} |
\begin{eqnarray} |
196 |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}}% |
\frac{D\vec{\mathbf{v}}_{h}}{Dt}+f\hat{\mathbf{k}}\times \vec{\mathbf{v}} |
197 |
_{h}+\frac{1}{\rho _{c}}\mathbf{\nabla }_{z}p^{\prime } &=&\vec{\mathbf{% |
_{h}+\frac{1}{\rho _{c}}\mathbf{\nabla }_{z}p^{\prime } &=&\vec{\mathbf{ |
198 |
\mathcal{F}}} \label{eq-zpe-hmom} \\ |
\mathcal{F}}} \label{eq:ocean-mom} \\ |
199 |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho ^{\prime }}{\rho _{c}}+\frac{1}{\rho |
\epsilon _{nh}\frac{Dw}{Dt}+\frac{g\rho ^{\prime }}{\rho _{c}}+\frac{1}{\rho |
200 |
_{c}}\frac{\partial p^{\prime }}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
_{c}}\frac{\partial p^{\prime }}{\partial z} &=&\epsilon _{nh}\mathcal{F}_{w} |
201 |
\label{eq-zpe-hydro} \\ |
\label{eq:ocean-wmom} \\ |
202 |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{\partial w}{\partial z} |
\mathbf{\nabla }_{z}\cdot \vec{\mathbf{v}}_{h}+\frac{\partial w}{\partial z} |
203 |
&=&0 \label{eq-zpe-cont} \\ |
&=&0 \label{eq:ocean-cont} \\ |
204 |
\rho ^{\prime } &=&\rho (\theta ,S,p_{o}(z))-\rho _{c} \label{eq-zpe-eos} \\ |
\rho ^{\prime } &=&\rho (\theta ,S,p_{o}(z))-\rho _{c} \label{eq:ocean-eos} \\ |
205 |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq-zpe-heat} \\ |
\frac{D\theta }{Dt} &=&\mathcal{Q}_{\theta } \label{eq:ocean-theta} \\ |
206 |
\frac{DS}{Dt} &=&\mathcal{Q}_{s} \label{eq-zpe-salt} |
\frac{DS}{Dt} &=&\mathcal{Q}_{s} \label{eq:ocean-salt} |
207 |
\end{eqnarray} |
\end{eqnarray} |
208 |
Note that the hydrostatic pressure of the resting fluid, including that |
Note that the hydrostatic pressure of the resting fluid, including that |
209 |
associated with $\rho _{c}$, is subtracted out since it has no effect on the |
associated with $\rho _{c}$, is subtracted out since it has no effect on the |