Normal-shock relations: Difference between revisions

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===The Hugoniot equation===
===The Hugoniot equation===


\noindent The Hugoniot equation is an alternative normal shock relation based on thermodynamic quantities only. It is derived from the governing equations and relates the change in energy to the change in pressure and specific volume. The starting point of the derivation of the Hugoniot equation is the governing equations (Eqns~\ref{eq:governing:cont} - \ref{eq:governing:energy}).
The Hugoniot equation is an alternative normal shock relation based on thermodynamic quantities only. It is derived from the governing equations and relates the change in energy to the change in pressure and specific volume. The starting point of the derivation of the Hugoniot equation is the governing equations (Eqns~\ref{eq:governing:cont} - \ref{eq:governing:energy}).


\noindent The continuity equation is rewritten and inserted into the momentum equation\\
The continuity equation is rewritten and inserted into the momentum equation


\begin{equation}
<math display="block">
u_1=\left(\frac{\rho_2}{\rho_1}\right) u_2
u_1=\left(\frac{\rho_2}{\rho_1}\right) u_2
\label{eq:governing:cont:b}
</math>
\end{equation}\\


\noindent Replace $u_1$ in Eqn. \ref{eq:governing:mom} using Eqn. \ref{eq:governing:cont:b}
Replace <math>u_1</math> in Eqn. \ref{eq:governing:mom} using Eqn. \ref{eq:governing:cont:b}


\[\rho_1 \left(\frac{\rho_2}{\rho_1}\right)^2 u^2_2 +p_1=\rho_2 u^2_2 + p_2\]\\
<math display="block">
\rho_1 \left(\frac{\rho_2}{\rho_1}\right)^2 u^2_2 +p_1=\rho_2 u^2_2 + p_2
</math>


\[u^2_2\left(\rho_1\left(\frac{\rho_2}{\rho_1}\right)^2-\rho_2\right)=\left(p_2-p_1\right)\]\\
<math display="block">
u^2_2\left(\rho_1\left(\frac{\rho_2}{\rho_1}\right)^2-\rho_2\right)=\left(p_2-p_1\right)
</math>


\[u^2_2\left(\left(\frac{\rho_2}{\rho_1}\right)\left(\rho_2-\rho_1\right)\right)=\left(p_2-p_1\right)\]\\
<math display="block">
u^2_2\left(\left(\frac{\rho_2}{\rho_1}\right)\left(\rho_2-\rho_1\right)\right)=\left(p_2-p_1\right)
</math>


\begin{equation}
<math display="block">
u^2_2=\left(\frac{\rho_1}{\rho_2}\right)\frac{p_2-p_1}{\rho_2-\rho_1}
u^2_2=\left(\frac{\rho_1}{\rho_2}\right)\frac{p_2-p_1}{\rho_2-\rho_1}
\label{eq:governing:mom:b}
</math>
\end{equation}\\


\noindent Eqn. \ref{eq:governing:cont:b} and \ref{eq:governing:mom:b} gives\\
Eqn. \ref{eq:governing:cont:b} and \ref{eq:governing:mom:b} gives


\begin{equation}
<math display="block">
u^2_1=\left(\frac{\rho_2}{\rho_1}\right)\frac{p_2-p_1}{\rho_2-\rho_1}
u^2_1=\left(\frac{\rho_2}{\rho_1}\right)\frac{p_2-p_1}{\rho_2-\rho_1}
\label{eq:governing:mom:c}
</math>
\end{equation}\\


\noindent Eqn. \ref{eq:governing:mom:b} and Eqn. \ref{eq:governing:mom:c} inserted in the energy equation (Eqn. \ref{eq:governing:energy}) gives\\
Eqn. \ref{eq:governing:mom:b} and Eqn. \ref{eq:governing:mom:c} inserted in the energy equation (Eqn. \ref{eq:governing:energy}) gives


\begin{equation}
<math display="block">
h_1 + \frac{1}{2}\left(\frac{\rho_2}{\rho_1}\right)\left(\frac{p_2-p_1}{\rho_2-\rho_1}\right)=h_2 + \frac{1}{2}\left(\frac{\rho_1}{\rho_2}\right)\left(\frac{p_2-p_1}{\rho_2-\rho_1}\right)
h_1 + \frac{1}{2}\left(\frac{\rho_2}{\rho_1}\right)\left(\frac{p_2-p_1}{\rho_2-\rho_1}\right)=h_2 + \frac{1}{2}\left(\frac{\rho_1}{\rho_2}\right)\left(\frac{p_2-p_1}{\rho_2-\rho_1}\right)
\label{eq:governing:energy:b}
</math>
\end{equation}\\


\[h_2-h_1=\frac{p_2-p_1}{2}\left[\left(\frac{\rho_2}{\rho_1}\right)\left(\frac{1}{\rho_2-\rho_1}\right)-\left(\frac{\rho_1}{\rho_2}\right)\left(\frac{1}{\rho_2-\rho_1}\right)\right]\]\\
<math display="block">
h_2-h_1=\frac{p_2-p_1}{2}\left[\left(\frac{\rho_2}{\rho_1}\right)\left(\frac{1}{\rho_2-\rho_1}\right)-\left(\frac{\rho_1}{\rho_2}\right)\left(\frac{1}{\rho_2-\rho_1}\right)\right]
</math>


\[h_2-h_1=\frac{p_2-p_1}{2}\left[\frac{\rho^2_2-\rho^2_1}{\rho_1\rho_2(\rho_2-\rho_1)}\right]=\frac{p_2-p_1}{2}\left[\frac{\rho_2+\rho_1}{\rho_1\rho_2}\right]\]\\
<math display="block">
h_2-h_1=\frac{p_2-p_1}{2}\left[\frac{\rho^2_2-\rho^2_1}{\rho_1\rho_2(\rho_2-\rho_1)}\right]=\frac{p_2-p_1}{2}\left[\frac{\rho_2+\rho_1}{\rho_1\rho_2}\right]
</math>


\begin{equation}
<math display="block">
h_2-h_1=\frac{p_2-p_1}{2}\left(\frac{1}{\rho_1}+\frac{1}{\rho_2}\right)
h_2-h_1=\frac{p_2-p_1}{2}\left(\frac{1}{\rho_1}+\frac{1}{\rho_2}\right)
\label{eq:governing:energy:c}
</math>
\end{equation}\\


\noindent Now, replacing the enthalpies with internal energies using $h=e+p/\rho$ gives\\
Now, replacing the enthalpies with internal energies using <math>h=e+p/\rho</math> gives


\[e_2-e_1=\frac{p_1}{\rho_1}-\frac{p_2}{\rho_2}+\frac{p_2-p_1}{2}\left(\frac{1}{\rho_1}+\frac{1}{\rho_2}\right)\]\\
<math display="block">
e_2-e_1=\frac{p_1}{\rho_1}-\frac{p_2}{\rho_2}+\frac{p_2-p_1}{2}\left(\frac{1}{\rho_1}+\frac{1}{\rho_2}\right)
</math>


\noindent which after some rewriting becomes the Hugoniot equation\\
which after some rewriting becomes the Hugoniot equation


\begin{equation}
<math display="block">
e_2-e_1=\frac{p_2+p_1}{2}\left(\frac{1}{\rho_1}-\frac{1}{\rho_2}\right)=\dfrac{p_2+p_1}{2}(\nu_1-\nu_2)
e_2-e_1=\frac{p_2+p_1}{2}\left(\frac{1}{\rho_1}-\frac{1}{\rho_2}\right)=\dfrac{p_2+p_1}{2}(\nu_1-\nu_2)
\label{eq:governing:hogoniot}
</math>
\end{equation}\\


%\noindent The Hugoniot equation relates thermodynamic properties over the normal shock
To give an idea about how the normal shock relates to an isentropic compression (a flow compression process without losses) the change in flow density as a function of pressure ratio is compared in Figure~\ref{fig:normal:shock:compression:vs:isentropic}. One can see that the normal-shock compression is more effective but less efficient than the corresponding isentropic process.
 
\noindent To give an idea about how the normal shock relates to an isentropic compression (a flow compression process without losses) the change in flow density as a function of pressure ratio is compared in Figure~\ref{fig:normal:shock:compression:vs:isentropic}. One can see that the normal-shock compression is more effective but less efficient than the corresponding isentropic process.


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\noindent Introducing C as the massflow per unit area (which is a constant)
Introducing <math>C</math> as the massflow per unit area (which is a constant)


\[\rho_1 u_1 = \rho_2 u_2 = C\]
<math display="block">
\rho_1 u_1 = \rho_2 u_2 = C
</math>


\noindent Inserted into the momentum equation this gives
Inserted into the momentum equation this gives


\[p_1+\dfrac{C^2}{\rho_1}=p_2+\dfrac{C^2}{\rho_2}\]
<math display="block">
p_1+\dfrac{C^2}{\rho_1}=p_2+\dfrac{C^2}{\rho_2}
</math>


or
or


\[\dfrac{p_2-p_1}{\nu_2-\nu_1}=-C^2\]
<math display="block">
\dfrac{p_2-p_1}{\nu_2-\nu_1}=-C^2
</math>


\noindent which implies that all possible solutions to the governing equations must be located on a line in $p\nu$-space (the so-called Rayleigh line). If we add the Hugoniot relation to this we will find that there are two possible solutions, the upstream condition and the condition downstream of the normal shock and the flow cannot be in any of the intermediate stages. The normal-process is a so-called wave solution to the governing equations where the flow state must jump directly from one flow state to another without passing the intermediate conditions. If we add heat or friction to the problem we will instead get continuous solutions as we will see in the following sections. Figures \ref{fig:shock:pv} and \ref{fig:shock:Ts} shows a normal shock process in a $p\nu$- and $Ts$-diagram, respectively. Note that the flow passes the characteristic conditions as it is going through the shock, which means that the flow goes from supersonic to subsonic.
which implies that all possible solutions to the governing equations must be located on a line in <math>p\nu</math>-space (the so-called Rayleigh line). If we add the Hugoniot relation to this we will find that there are two possible solutions, the upstream condition and the condition downstream of the normal shock and the flow cannot be in any of the intermediate stages. The normal-process is a so-called wave solution to the governing equations where the flow state must jump directly from one flow state to another without passing the intermediate conditions. If we add heat or friction to the problem we will instead get continuous solutions as we will see in the following sections. Figures \ref{fig:shock:pv} and \ref{fig:shock:Ts} shows a normal shock process in a <math>p\nu</math>- and <math>Ts</math>-diagram, respectively. Note that the flow passes the characteristic conditions as it is going through the shock, which means that the flow goes from supersonic to subsonic.


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