Finite non-linear waves: Difference between revisions

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Created page with "Category:Compressible flow Category:Unsteady waves Category:Inviscid flow __TOC__ \section{Finite Nonlinear Waves} \noindent Starting point: the governing flow equations on partial differential form\\ \noindent Continuity equation: \begin{equation} \frac{\partial \rho}{\partial t}+u\frac{\partial \rho}{\partial x}+\rho\frac{\partial u}{\partial x}=0 \label{eq:pde:cont} \end{equation}\\ \noindent Momentum equation: \begin{equation} \frac{\partial u}{\pa..."
 
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\section{Finite Nonlinear Waves}
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Starting point: the governing flow equations on partial differential form


\noindent Starting point: the governing flow equations on partial differential form\\
Continuity equation:


\noindent Continuity equation:
{{NumEqn|<math>
 
\begin{equation}
\frac{\partial \rho}{\partial t}+u\frac{\partial \rho}{\partial x}+\rho\frac{\partial u}{\partial x}=0
\frac{\partial \rho}{\partial t}+u\frac{\partial \rho}{\partial x}+\rho\frac{\partial u}{\partial x}=0
\label{eq:pde:cont}
</math>}}
\end{equation}\\


\noindent Momentum equation:
Momentum equation:


\begin{equation}
{{NumEqn|<math>
\frac{\partial u}{\partial t}+u\frac{\partial u}{\partial x}+\frac{1}{\rho}\frac{\partial p}{\partial x}=0
\frac{\partial u}{\partial t}+u\frac{\partial u}{\partial x}+\frac{1}{\rho}\frac{\partial p}{\partial x}=0
\label{eq:pde:mom}
</math>}}
\end{equation}\\


\noindent Any thermodynamic property can be expressed as a function of two other thermodynamic properties. This means that we can get density as a function of pressure and entropy: $\rho=\rho(p,s)$ and therefore\\
Any thermodynamic property can be expressed as a function of two other thermodynamic properties. This means that we can get density as a function of pressure and entropy: <math>\rho=\rho(p,s)</math> and therefore


\begin{equation*}
{{NumEqn|<math>
d\rho=\left(\frac{\partial \rho}{\partial p}\right)_s dp+\left(\frac{\partial \rho}{\partial s}\right)_p ds
d\rho=\left(\frac{\partial \rho}{\partial p}\right)_s dp+\left(\frac{\partial \rho}{\partial s}\right)_p ds
\end{equation*}\\
</math>}}


\noindent Assuming isentropic flow $ds=0$ gives\\
Assuming isentropic flow <math>ds=0</math> gives


\begin{equation*}
{{NumEqn|<math>
d\rho=\left(\frac{\partial \rho}{\partial p}\right)_s dp
d\rho=\left(\frac{\partial \rho}{\partial p}\right)_s dp
\end{equation*}\\
</math>}}


\begin{equation}
{{NumEqn|<math>
\begin{aligned}
\begin{aligned}
&\frac{\partial \rho}{\partial t}=\left(\frac{\partial \rho}{\partial p}\right)_s\frac{\partial p}{\partial t}=\frac{1}{a^2}\frac{\partial p}{\partial t}\\
&\frac{\partial \rho}{\partial t}=\left(\frac{\partial \rho}{\partial p}\right)_s\frac{\partial p}{\partial t}=\frac{1}{a^2}\frac{\partial p}{\partial t}\\
Line 41: Line 48:
&\frac{\partial \rho}{\partial x}=\left(\frac{\partial \rho}{\partial p}\right)_s\frac{\partial p}{\partial x}=\frac{1}{a^2}\frac{\partial p}{\partial x}
&\frac{\partial \rho}{\partial x}=\left(\frac{\partial \rho}{\partial p}\right)_s\frac{\partial p}{\partial x}=\frac{1}{a^2}\frac{\partial p}{\partial x}
\end{aligned}
\end{aligned}
\label{eq:rhotop}
</math>}}
\end{equation}\\


\noindent Now, insert \ref{eq:rhotop} in \ref{eq:pde:cont} gives\\
Now, insert \ref{eq:rhotop} in \ref{eq:pde:cont} gives


\begin{equation}
{{NumEqn|<math>
\frac{\partial p}{\partial t}+u\frac{\partial p}{\partial x}+\rho a^2\frac{\partial u}{\partial x}=0
\frac{\partial p}{\partial t}+u\frac{\partial p}{\partial x}+\rho a^2\frac{\partial u}{\partial x}=0
\label{eq:pde:cont:b}
</math>}}
\end{equation}\\


\noindent Dividing \ref{eq:pde:cont:b} by $\rho a$ gives\\
Dividing \ref{eq:pde:cont:b} by <math>\rho a</math> gives


\begin{equation}
{{NumEqn|<math>
\frac{1}{\rho a}\left(\frac{\partial p}{\partial t}+u\frac{\partial p}{\partial x}\right)+a\frac{\partial u}{\partial x}=0
\frac{1}{\rho a}\left(\frac{\partial p}{\partial t}+u\frac{\partial p}{\partial x}\right)+a\frac{\partial u}{\partial x}=0
\label{eq:pde:cont:c}
</math>}}
\end{equation}\\


\noindent A slightly modified form of the momentum equation is obtained by multiplying and dividing the last term by $a$\\
A slightly modified form of the momentum equation is obtained by multiplying and dividing the last term by <math>a</math>


\begin{equation}
{{NumEqn|<math>
\frac{\partial u}{\partial t}+u\frac{\partial u}{\partial x}+\frac{1}{\rho a}\left(a\frac{\partial p}{\partial x}\right)=0
\frac{\partial u}{\partial t}+u\frac{\partial u}{\partial x}+\frac{1}{\rho a}\left(a\frac{\partial p}{\partial x}\right)=0
\label{eq:pde:mom:c}
</math>}}
\end{equation}\\


\noindent If the continuity equation on the form \ref{eq:pde:cont:c} is added to the momentum equation on the form \ref{eq:pde:mom:c}, we get\\
If the continuity equation on the form \ref{eq:pde:cont:c} is added to the momentum equation on the form \ref{eq:pde:mom:c}, we get


\begin{equation}
{{NumEqn|<math>
\left[\frac{\partial u}{\partial t}+(u+a)\frac{\partial u}{\partial x}\right]+\frac{1}{\rho a}\left[\frac{\partial p}{\partial t}+(u+a)\frac{\partial p}{\partial x}\right]=0
\left[\frac{\partial u}{\partial t}+(u+a)\frac{\partial u}{\partial x}\right]+\frac{1}{\rho a}\left[\frac{\partial p}{\partial t}+(u+a)\frac{\partial p}{\partial x}\right]=0
\label{eq:nonlin:a}
</math>}}
\end{equation}\\


\noindent If, instead, the continuity equation on the form \ref{eq:pde:cont:c} is subtracted from the momentum equation on the form \ref{eq:pde:mom:c}, we get\\
If, instead, the continuity equation on the form \ref{eq:pde:cont:c} is subtracted from the momentum equation on the form \ref{eq:pde:mom:c}, we get


\begin{equation}
{{NumEqn|<math>
\left[\frac{\partial u}{\partial t}+(u-a)\frac{\partial u}{\partial x}\right]+\frac{1}{\rho a}\left[\frac{\partial p}{\partial t}+(u-a)\frac{\partial p}{\partial x}\right]=0
\left[\frac{\partial u}{\partial t}+(u-a)\frac{\partial u}{\partial x}\right]+\frac{1}{\rho a}\left[\frac{\partial p}{\partial t}+(u-a)\frac{\partial p}{\partial x}\right]=0
\label{eq:nonlin:b}
</math>}}
\end{equation}\\


\noindent Since $u=u(x,t)$, we have from the definition of a differential\\
Since <math>u=u(x,t)</math>, we have from the definition of a differential


\begin{equation}
{{NumEqn|<math>
du=\frac{\partial u}{\partial t}dt+\frac{\partial u}{\partial x}dx=\frac{\partial u}{\partial t}dt+\frac{\partial u}{\partial x}\frac{dx}{dt}dt
du=\frac{\partial u}{\partial t}dt+\frac{\partial u}{\partial x}dx=\frac{\partial u}{\partial t}dt+\frac{\partial u}{\partial x}\frac{dx}{dt}dt
\label{eq:du}
</math>}}
\end{equation}\\


\noindent Now, let $dx/dt=u+a$\\
Now, let <math>dx/dt=u+a</math>


\begin{equation}
{{NumEqn|<math>
du=\frac{\partial u}{\partial t}dt+(u+a)\frac{\partial u}{\partial x}dt=\left[\frac{\partial u}{\partial t}+(u+a)\frac{\partial u}{\partial x}\right]dt
du=\frac{\partial u}{\partial t}dt+(u+a)\frac{\partial u}{\partial x}dt=\left[\frac{\partial u}{\partial t}+(u+a)\frac{\partial u}{\partial x}\right]dt
\label{eq:du:b}
</math>}}
\end{equation}\\


\noindent which is the change of $u$ in the direction $dx/dt=u+a$\\
which is the change of <math>u</math> in the direction <math>dx/dt=u+a</math>


\noindent In the same way\\
In the same way


\begin{equation}
{{NumEqn|<math>
dp=\frac{\partial p}{\partial t}dt+\frac{\partial p}{\partial x}dx=\frac{\partial p}{\partial t}dt+\frac{\partial p}{\partial x}\frac{dx}{dt}dt
dp=\frac{\partial p}{\partial t}dt+\frac{\partial p}{\partial x}dx=\frac{\partial p}{\partial t}dt+\frac{\partial p}{\partial x}\frac{dx}{dt}dt
\label{eq:dp}
</math>}}
\end{equation}\\


\noindent and thus, in the direction $dx/dt=u+a$\\
and thus, in the direction <math>dx/dt=u+a</math>


\begin{equation}
{{NumEqn|<math>
dp=\frac{\partial p}{\partial t}dt+(u+a)\frac{\partial p}{\partial x}dt=\left[\frac{\partial p}{\partial t}+(u+a)\frac{\partial p}{\partial x}\right]dt
dp=\frac{\partial p}{\partial t}dt+(u+a)\frac{\partial p}{\partial x}dt=\left[\frac{\partial p}{\partial t}+(u+a)\frac{\partial p}{\partial x}\right]dt
\label{eq:dp:b}
</math>}}
\end{equation}\\


\noindent If we go back and examine Eqn. \ref{eq:nonlin:a}, we see that Eqns. \ref{eq:du:b} and \ref{eq:dp:b} appear in the equation and thus it can now be rewritten as follows\\
If we go back and examine Eqn. \ref{eq:nonlin:a}, we see that Eqns. \ref{eq:du:b} and \ref{eq:dp:b} appear in the equation and thus it can now be rewritten as follows


\begin{equation}
{{NumEqn|<math>
\frac{du}{dt}+\frac{1}{\rho a}\frac{dp}{dt}=0\Rightarrow du+\frac{dp}{\rho a}=0
\frac{du}{dt}+\frac{1}{\rho a}\frac{dp}{dt}=0\Rightarrow du+\frac{dp}{\rho a}=0
\label{eq:nonlin:a:ode}
</math>}}
\end{equation}\\


\noindent Eqn. \ref{eq:nonlin:a:ode} applies along a $C^+$ characteristic, i.e., a line in the direction $dx/dt=u+a$ in $xt$-space and is called the compatibility equation along the $C^+$ characteristic. If we instead chose a $C^-$ characteristic, i.e., a line in the direction $dx/dt=u-a$ in $xt$-space, we get\\
Eqn. \ref{eq:nonlin:a:ode} applies along a <math>C^+</math> characteristic, i.e., a line in the direction <math>dx/dt=u+a</math> in <math>xt</math>-space and is called the compatibility equation along the <math>C^+</math> characteristic. If we instead chose a <math>C^-</math> characteristic, i.e., a line in the direction <math>dx/dt=u-a</math> in <math>xt</math>-space, we get


\begin{equation}
{{NumEqn|<math>
du=\left[\frac{\partial u}{\partial t}+(u-a)\frac{\partial u}{\partial x}\right]dt
du=\left[\frac{\partial u}{\partial t}+(u-a)\frac{\partial u}{\partial x}\right]dt
\label{eq:du:c}
</math>}}
\end{equation}\\


\begin{equation}
{{NumEqn|<math>
dp=\left[\frac{\partial p}{\partial t}+(u-a)\frac{\partial p}{\partial x}\right]dt
dp=\left[\frac{\partial p}{\partial t}+(u-a)\frac{\partial p}{\partial x}\right]dt
\label{eq:dp:c}
</math>}}
\end{equation}\\


\noindent which can be identified as subsets of Eqn. \ref{eq:nonlin:b} and thus\\
which can be identified as subsets of Eqn. \ref{eq:nonlin:b} and thus


\begin{equation*}
{{NumEqn|<math>
\frac{du}{dt}-\frac{1}{\rho a}\frac{dp}{dt}=0
\frac{du}{dt}-\frac{1}{\rho a}\frac{dp}{dt}=0
\end{equation*}\\
</math>}}


\noindent In order to fulfill the relation above, either $du=dp=0$ or\\
In order to fulfil the relation above, either <math>du=dp=0</math> or


\begin{equation}
{{NumEqn|<math>
du-\frac{dp}{\rho a}=0
du-\frac{dp}{\rho a}=0
\label{eq:nonlin:b:ode}
</math>}}
\end{equation}\\


\noindent Eqn. \ref{eq:nonlin:b:ode} applies along a $C^-$ characteristic, i.e., a line in the direction $dx/dt=u-a$ in $xt$-space and is called the compatibility equation along the $C^-$ characteristic.\\
Eqn. \ref{eq:nonlin:b:ode} applies along a <math>C^-</math> characteristic, i.e., a line in the direction <math>dx/dt=u-a</math> in <math>xt</math>-space and is called the compatibility equation along the <math>C^-</math> characteristic.


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\noindent So, what we have done now is that we have have found paths through a point ($x_1$,$t_1$) along which the governing partial differential equations Eqns. \ref{eq:nonlin:a} and \ref{eq:nonlin:b} reduces to the ordinary differential equations \ref{eq:nonlin:a:ode} and \ref{eq:nonlin:b:ode}. The $C^+$ and $C^-$ characteristic lines are physically the paths of right- and left-running sound waves in the $xt$-plane.\\
So, what we have done now is that we have have found paths through a point (<math>x_1</math>, <math>t_1</math>) along which the governing partial differential equations Eqns. \ref{eq:nonlin:a} and \ref{eq:nonlin:b} reduces to the ordinary differential equations \ref{eq:nonlin:a:ode} and \ref{eq:nonlin:b:ode}. The <math>C^+</math> and <math>C^-</math> characteristic lines are physically the paths of right- and left-running sound waves in the <math>xt</math>-plane.


\subsection{Riemann Invariants}
==== Riemann Invariants ====


\noindent If the compatibility equations are integrated along respective characteristic line, i.e., integrate \ref{eq:nonlin:a:ode} along the $C^+$ characteristic and  \ref{eq:nonlin:b:ode} along the $C^-$ characteristic, we get the Riemann invariants $J^+$ and $J^-$.\\
If the compatibility equations are integrated along respective characteristic line, i.e., integrate \ref{eq:nonlin:a:ode} along the <math>C^+</math> characteristic and  \ref{eq:nonlin:b:ode} along the <math>C^-</math> characteristic, we get the Riemann invariants <math>J^+</math> and <math>J^-</math>.


\begin{equation}
{{NumEqn|<math>
J^+=u+\int\frac{dp}{\rho a}=const
J^+=u+\int\frac{dp}{\rho a}=const
\label{eq:riemann:a}
</math>}}
\end{equation}\\


\begin{equation}
{{NumEqn|<math>
J^-=u-\int\frac{dp}{\rho a}=const
J^-=u-\int\frac{dp}{\rho a}=const
\label{eq:riemann:b}
</math>}}
\end{equation}\\


\noindent The Riemann invariants are constants along the associated characteristic line.\\
The Riemann invariants are constants along the associated characteristic line.


\noindent We have assumed isentropic flow and thus we may use the isentropic relations\\
We have assumed isentropic flow and thus we may use the isentropic relations


\begin{equation}
{{NumEqn|<math>
p=C_1T^{\gamma/(\gamma-1)}=C_2a^{2\gamma/(\gamma-1)}
p=C_1T^{\gamma/(\gamma-1)}=C_2a^{2\gamma/(\gamma-1)}
\label{eq:isentropic:a}
</math>}}
\end{equation}\\


\noindent where $C_1$ and $C_2$ are constants. Differentiating Eqn. \ref{eq:isentropic:a} gives\\
where <math>C_1</math> and <math>C_2</math> are constants. Differentiating Eqn. \ref{eq:isentropic:a} gives


\begin{equation}
{{NumEqn|<math>
dp=C_2\left(\frac{2\gamma}{\gamma-1}\right)a^{[2\gamma/(\gamma-1)-1]}da
dp=C_2\left(\frac{2\gamma}{\gamma-1}\right)a^{[2\gamma/(\gamma-1)-1]}da
\label{eq:isentropic:b}
</math>}}
\end{equation}\\


\noindent Now, if we further assume the gas to be calorically perfect\\
Now, if we further assume the gas to be calorically perfect


\begin{equation}
{{NumEqn|<math>
a^2=\gamma RT=\frac{\gamma p}{\rho}\Rightarrow \rho=\frac{\gamma p}{a^2}
a^2=\gamma RT=\frac{\gamma p}{\rho}\Rightarrow \rho=\frac{\gamma p}{a^2}
\label{eq:isentropic:c}
</math>}}
\end{equation}\\


\noindent Eqn. \ref{eq:isentropic:a} in \ref{eq:isentropic:c} gives\\
Eqn. \ref{eq:isentropic:a} in \ref{eq:isentropic:c} gives


\begin{equation}
{{NumEqn|<math>
\rho=C_2\gamma a^{[2\gamma/(\gamma-1)-2]}
\rho=C_2\gamma a^{[2\gamma/(\gamma-1)-2]}
\label{eq:isentropic:d}
</math>}}
\end{equation}\\


\noindent and thus\\
and thus


\begin{equation*}
{{NumEqn|<math>
J^+=u+\int\frac{C_2\left(\frac{2\gamma}{\gamma-1}\right)a^{[2\gamma/(\gamma-1)-1]}}{C_2\gamma a^{[2\gamma/(\gamma-1)-2]}a}da=u+\left(\frac{2}{\gamma-1}\right)\int da
J^+=u+\int\frac{C_2\left(\frac{2\gamma}{\gamma-1}\right)a^{[2\gamma/(\gamma-1)-1]}}{C_2\gamma a^{[2\gamma/(\gamma-1)-2]}a}da=u+\left(\frac{2}{\gamma-1}\right)\int da
\end{equation*}\\
</math>}}


\begin{equation}
{{NumEqn|<math>
J^+=u+\frac{2a}{\gamma-1}
J^+=u+\frac{2a}{\gamma-1}
\label{eq:riemann:a:b}
</math>}}
\end{equation}\\


\begin{equation}
{{NumEqn|<math>
J^-=u-\frac{2a}{\gamma-1}
J^-=u-\frac{2a}{\gamma-1}
\label{eq:riemann:b:b}
</math>}}
\end{equation}\\


\noindent Eqns. \ref{eq:riemann:a:b} and \ref{eq:riemann:b:b} are the Riemann invariants for a calorically perfect gas. The Riemann invariants are constants along $C^+$ and $C^-$ characteristics and if the situation shown in Fig. \ref{fig:characteristics} appears, that fact can be used to calculate the flow velocity and speed of sound in the location ($x_1$,$t_1$).\\
Eqns. \ref{eq:riemann:a:b} and \ref{eq:riemann:b:b} are the Riemann invariants for a calorically perfect gas. The Riemann invariants are constants along <math>C^+</math> and <math>C^-</math> characteristics and if the situation shown in Fig. \ref{fig:characteristics} appears, that fact can be used to calculate the flow velocity and speed of sound in the location (<math>x_1</math>, <math>t_1</math>).


\begin{equation}
{{NumEqn|<math>
J^++J^-=u+\frac{2a}{\gamma-1}+u-\frac{2a}{\gamma-1}=2u\Rightarrow u=\frac{1}{2}(J^++J^-)
J^++J^-=u+\frac{2a}{\gamma-1}+u-\frac{2a}{\gamma-1}=2u\Rightarrow u=\frac{1}{2}(J^++J^-)
\label{eq:riemann:evaluation:a}
</math>}}
\end{equation}\\


\begin{equation}
{{NumEqn|<math>
J^+=u+\frac{2a}{\gamma-1}=\frac{1}{2}(J^++J^-)+\frac{2a}{\gamma-1}\Rightarrow a=\frac{\gamma-1}{4}(J^+-J^-)
J^+=u+\frac{2a}{\gamma-1}=\frac{1}{2}(J^++J^-)+\frac{2a}{\gamma-1}\Rightarrow a=\frac{\gamma-1}{4}(J^+-J^-)
\label{eq:riemann:evaluation:b}
</math>}}
\end{equation}\\

Latest revision as of 13:36, 1 April 2026

Starting point: the governing flow equations on partial differential form

Continuity equation:

ρt+uρx+ρux=0(Eq. 6.105)

Momentum equation:

ut+uux+1ρpx=0(Eq. 6.106)

Any thermodynamic property can be expressed as a function of two other thermodynamic properties. This means that we can get density as a function of pressure and entropy: ρ=ρ(p,s) and therefore

dρ=(ρp)sdp+(ρs)pds(Eq. 6.107)

Assuming isentropic flow ds=0 gives

dρ=(ρp)sdp(Eq. 6.108)
ρt=(ρp)spt=1a2ptρx=(ρp)spx=1a2px(Eq. 6.109)

Now, insert \ref{eq:rhotop} in \ref{eq:pde:cont} gives

pt+upx+ρa2ux=0(Eq. 6.110)

Dividing \ref{eq:pde:cont:b} by ρa gives

1ρa(pt+upx)+aux=0(Eq. 6.111)

A slightly modified form of the momentum equation is obtained by multiplying and dividing the last term by a

ut+uux+1ρa(apx)=0(Eq. 6.112)

If the continuity equation on the form \ref{eq:pde:cont:c} is added to the momentum equation on the form \ref{eq:pde:mom:c}, we get

[ut+(u+a)ux]+1ρa[pt+(u+a)px]=0(Eq. 6.113)

If, instead, the continuity equation on the form \ref{eq:pde:cont:c} is subtracted from the momentum equation on the form \ref{eq:pde:mom:c}, we get

[ut+(ua)ux]+1ρa[pt+(ua)px]=0(Eq. 6.114)

Since u=u(x,t), we have from the definition of a differential

du=utdt+uxdx=utdt+uxdxdtdt(Eq. 6.115)

Now, let dx/dt=u+a

du=utdt+(u+a)uxdt=[ut+(u+a)ux]dt(Eq. 6.116)

which is the change of u in the direction dx/dt=u+a

In the same way

dp=ptdt+pxdx=ptdt+pxdxdtdt(Eq. 6.117)

and thus, in the direction dx/dt=u+a

dp=ptdt+(u+a)pxdt=[pt+(u+a)px]dt(Eq. 6.118)

If we go back and examine Eqn. \ref{eq:nonlin:a}, we see that Eqns. \ref{eq:du:b} and \ref{eq:dp:b} appear in the equation and thus it can now be rewritten as follows

dudt+1ρadpdt=0du+dpρa=0(Eq. 6.119)

Eqn. \ref{eq:nonlin:a:ode} applies along a C+ characteristic, i.e., a line in the direction dx/dt=u+a in xt-space and is called the compatibility equation along the C+ characteristic. If we instead chose a C characteristic, i.e., a line in the direction dx/dt=ua in xt-space, we get

du=[ut+(ua)ux]dt(Eq. 6.120)
dp=[pt+(ua)px]dt(Eq. 6.121)

which can be identified as subsets of Eqn. \ref{eq:nonlin:b} and thus

dudt1ρadpdt=0(Eq. 6.122)

In order to fulfil the relation above, either du=dp=0 or

dudpρa=0(Eq. 6.123)

Eqn. \ref{eq:nonlin:b:ode} applies along a C characteristic, i.e., a line in the direction dx/dt=ua in xt-space and is called the compatibility equation along the C characteristic.


So, what we have done now is that we have have found paths through a point (x1, t1) along which the governing partial differential equations Eqns. \ref{eq:nonlin:a} and \ref{eq:nonlin:b} reduces to the ordinary differential equations \ref{eq:nonlin:a:ode} and \ref{eq:nonlin:b:ode}. The C+ and C characteristic lines are physically the paths of right- and left-running sound waves in the xt-plane.

Riemann Invariants

If the compatibility equations are integrated along respective characteristic line, i.e., integrate \ref{eq:nonlin:a:ode} along the C+ characteristic and \ref{eq:nonlin:b:ode} along the C characteristic, we get the Riemann invariants J+ and J.

J+=u+dpρa=const(Eq. 6.124)
J=udpρa=const(Eq. 6.125)

The Riemann invariants are constants along the associated characteristic line.

We have assumed isentropic flow and thus we may use the isentropic relations

p=C1Tγ/(γ1)=C2a2γ/(γ1)(Eq. 6.126)

where C1 and C2 are constants. Differentiating Eqn. \ref{eq:isentropic:a} gives

dp=C2(2γγ1)a[2γ/(γ1)1]da(Eq. 6.127)

Now, if we further assume the gas to be calorically perfect

a2=γRT=γpρρ=γpa2(Eq. 6.128)

Eqn. \ref{eq:isentropic:a} in \ref{eq:isentropic:c} gives

ρ=C2γa[2γ/(γ1)2](Eq. 6.129)

and thus

J+=u+C2(2γγ1)a[2γ/(γ1)1]C2γa[2γ/(γ1)2]ada=u+(2γ1)da(Eq. 6.130)
J+=u+2aγ1(Eq. 6.131)
J=u2aγ1(Eq. 6.132)

Eqns. \ref{eq:riemann:a:b} and \ref{eq:riemann:b:b} are the Riemann invariants for a calorically perfect gas. The Riemann invariants are constants along C+ and C characteristics and if the situation shown in Fig. \ref{fig:characteristics} appears, that fact can be used to calculate the flow velocity and speed of sound in the location (x1, t1).

J++J=u+2aγ1+u2aγ1=2uu=12(J++J)(Eq. 6.133)
J+=u+2aγ1=12(J++J)+2aγ1a=γ14(J+J)(Eq. 6.134)