View source for One-dimensional flow with heat addition

[[Category:Compressible flow]]
[[Category:One-dimensional flow]]
[[Category:Inviscid flow]]
[[Category:Continuous solution]]

__TOC__

==== Flow-station relations ====

The aim is to derive relations for pressure ratio and temperature ratio as a function of Mach numbers. We will do that starting from the momentum equation.

<math display="block">
p_2-p_1=\rho_1 u_1^2 - \rho_2 u_2^2 
</math>

Assuming calorically perfect gas

<math display="block">
\rho u^2=\rho a^2 M^2=\rho \frac{\gamma p}{\rho} M^2=\gamma p M^2
</math>

which inserted in Eqn. \ref{eq:governing:mom} gives

<math display="block">
p_2-p_1=\gamma p_1 M_1^2 - \gamma p_2 M_2^2
</math>

<math display="block">
p_2(1+\gamma M_2^2)=p_1(1+\gamma M_1^2)
</math>

and thus

<math display="block">
\frac{p_2}{p_1}=\frac{1+\gamma M_1^2}{1+\gamma M_2^2}
</math>

From the equation of state <math>p=\rho RT</math>, we get

<math display="block">
\frac{T_2}{T_1}=\frac{p_2}{\rho_2 R}\frac{\rho_1 R}{p_1}=\frac{p_2}{p_1}\frac{\rho_1}{\rho_2}
</math>

Using the continuity equation, we can get <math>\rho_1/\rho_2</math>

<math display="block">
\rho_1 u_1=\rho_2 u_2 \Rightarrow \frac{\rho_1}{\rho_2}=\frac{u_2}{u_1}
</math>

Inserted in Eqn. \ref{eq:tr:a} gives

<math display="block">
\frac{T_2}{T_1}=\frac{p_2}{p_1}\frac{u_2}{u_1}
</math>

<math display="block">
\frac{u_2}{u_1}=\frac{M_2a_2}{M_1a_1}=\frac{M_2}{M_1}\frac{\sqrt{\gamma RT_2}}{\sqrt{\gamma RT_1}}=\frac{M_2}{M_1}\sqrt{\frac{T_2}{T_1}}
</math>

Eqn. \ref{eq:tr:c} in Eqn. \ref{eq:tr:b} gives

<math display="block">
\sqrt{\frac{T_2}{T_1}}=\frac{p_2}{p_1}\frac{M_2}{M_1}
</math>

With <math>p_2/p_1</math> from Eqn. \ref{eq:governing:mom:b}, Eqn \ref{eq:tr:d} becomes

<math display="block">
\frac{T_2}{T_1}=\left(\frac{1+\gamma M_1^2}{1+\gamma M_2^2}\right)^2\left(\frac{M_2}{M_1}\right)^2
</math>

==== Differential Relations ====

The equations presented in the previous section gives us the flow state after heat addition but since the heat addition, unlike the normal shock, is a continuous process, it is of interest to study the the heat addition from start to end. In order to do so we will now derive differential relations starting from the governing equations on differential form. We will start with converting the integral equation for conservation of mass for one-dimensional flows to differential form.

<math display="block">
\rho_1 u_1 = \rho_2 u_2 = const \Rightarrow d(\rho u)=0
</math>

<math display="block">
d(\rho u)=\rho du+ud\rho=0
</math>

Divide by <math>\rho u</math> gives

<math display="block">
\dfrac{d\rho}{\rho}=\dfrac{du}{u}
</math>

The integral form of the conservation of momentum equation for one-dimensional flows is converted to differential form as follows.

<math display="block">
p_1+\rho_1u_1^2=p_2+\rho_2u_2^2=const \Rightarrow d(p+\rho u^2)=0
</math>

<math display="block">
dp+\rho udu+u\underbrace{d(\rho u)}_{=0}=0\Rightarrow dp=-\rho udu
</math>

with <math>\rho=\dfrac{p}{RT}</math> and <math>u^2=M^2a^2=M^2\gamma RT</math> in Eqn.~\ref{eq:governing:mom:diff:b}, we get\\

<math display="block">
dp=-\dfrac{p}{RT}u^2\dfrac{du}{u}=-\dfrac{p}{RT}M^2\gamma RT\dfrac{du}{u}\Rightarrow
</math>

<math display="block">
\dfrac{dp}{p}=-\gamma M^2\dfrac{du}{u}
</math>

which gives the relative change in pressure, <math>dp/p</math>, as a function of the relative change in flow velocity, <math>du/u</math>. The next equation to derive is an equation that describes the relative change in temperature, <math>dT/T</math>, as a function of the relative change in flow velocity, <math>du/u</math>. The starting point is the equation of state (the gas law).

<math display="block">
p=\rho RT\Rightarrow dp = R(\rho dT+ Td\rho)\Rightarrow dT=\dfrac{1}{R\rho}dp-\dfrac{T}{\rho}d\rho
</math>

Divide by <math>T</math>

<math display="block">
\dfrac{dT}{T}=\dfrac{1}{\rho RT}dp-\dfrac{1}{\rho}d\rho
</math>

substitute <math>dp</math> from Eqn.~\ref{eq:governing:mom:diff:c} and <math>d\rho</math> from Eqn.~\ref{eq:governing:cont:diff:b} gives

<math display="block">
\dfrac{dT}{T}=(1-\gamma M^2)\dfrac{du}{u}
</math>

The entropy equation reads

<math display="block">
ds=C_v\dfrac{dp}{p}-C_p\dfrac{d\rho}{\rho}
</math>

which after substituting <math>dp</math> from Eqn.~\ref{eq:governing:mom:diff:c} and <math>d\rho</math> from Eqn.~\ref{eq:governing:cont:diff:b} becomes

<math display="block">
ds=C_v\gamma(1-M^2)\dfrac{du}{u}
</math>

From the definition of total temperature <math>T_o</math> we get


<math display="block">
T_o=T+\dfrac{u^2}{2C_p}\Rightarrow dT_o=dT+\dfrac{1}{C_p}udu=dT+\dfrac{\gamma-1}{\gamma RT}T u^2\dfrac{du}{u}\Rightarrow
</math>

<math display="block">
dT_o=dT+(\gamma-1)M^2 T\dfrac{du}{u}
</math>

Inserting <math>dT</math> from Eqn~\ref{eq:governing:temp:diff:c} in Eqn~\ref{eq:governing:To:diff:a} we get

<math display="block">
dT_o=(1-\gamma M^2)T\dfrac{du}{u}+(\gamma-1)M^2 T\dfrac{du}{u}
</math>

or

<math display="block">
dT_o=(1-M^2)T\dfrac{du}{u}
</math>

Dividing Eqn.~\ref{eq:governing:To:diff:b} by <math>T_o</math> and using

<math display="block">
T_o=T\left(1+\dfrac{\gamma-1}{2}M^2\right)
</math>

we get

<math display="block">
\dfrac{dT_o}{T_o}=\dfrac{1-M^2}{1+\dfrac{\gamma-1}{2}M^2}\dfrac{du}{u}
</math>

Finally, we will derive a differential relation that describes the change in Mach number.

<math display="block">
M=\dfrac{u}{\sqrt{\gamma RT}}\Rightarrow dM=\dfrac{1}{\sqrt{\gamma R}}(T^{1/2}du+ud(T^{-1/2}))=\dfrac{du}{\sqrt{\gamma RT}}-\dfrac{u}{2\sqrt{\gamma R}}T^{-3/2}dT\Rightarrow
</math>

<math display="block">
dM=\dfrac{1}{\sqrt{\gamma RT}}\dfrac{du}{u}-\dfrac{1}{2}\dfrac{u}{\sqrt{\gamma RT}}\dfrac{dT}{T}=M\dfrac{du}{u}-\dfrac{M}{2}\dfrac{dT}{T}
</math>

Inserting <math>dT/T</math> from Eqn.~\ref{eq:governing:temp:diff:c}, we get

<math display="block">
\dfrac{dM}{M}=\dfrac{1+\gamma M^2}{2}\dfrac{du}{u}
</math>

All the derived differential relations are expressed as functions of <math<du/u</math> but it would be more convenient to relate the changes in flow properties to the added heat or the change in total temperature, which can be related to the added heat through the energy equation.

<math display="block">
dT_o=\dfrac{\delta q}{C_p}
</math>

From Eqn.~\ref{eq:governing:To:diff:c}, we get

<math display="block">
\dfrac{du}{u}=\left(\dfrac{1+\dfrac{\gamma-1}{2}M^2}{1-M^2}\right)\dfrac{dT_o}{T_o}
</math>

Now, we can substitute $du/u$ in all the above relations using Eqn.~\ref{eq:governing:du:diff:final}, we get the following relations

<math display="block">
\dfrac{d\rho}{\rho}=-\left(\dfrac{1+\dfrac{\gamma-1}{2}M^2}{1-M^2}\right)\dfrac{dT_o}{T_o}
</math>

<math display="block">
\dfrac{dp}{p}=\gamma M^2\left(\dfrac{1+\dfrac{\gamma-1}{2}M^2}{1-M^2}\right)\dfrac{dT_o}{T_o}
</math>

<math display="block">
\dfrac{dT}{T}=(1-\gamma M^2)\left(\dfrac{1+\dfrac{\gamma-1}{2}M^2}{1-M^2}\right)\dfrac{dT_o}{T_o}
</math>

<math display="block">
\dfrac{dT}{T}=\left(\dfrac{1+\gamma M^2}{2}\right)\left(\dfrac{1+\dfrac{\gamma-1}{2}M^2}{1-M^2}\right)\dfrac{dT_o}{T_o}
</math>

<math display="block">
\dfrac{dT}{T}=C_v\gamma \left(1+\dfrac{\gamma-1}{2}M^2\right)\dfrac{dT_o}{T_o}
</math>

==== Heat Addition Process ====

\noindent With the differential relations in place, we can now study the continuous change in flow quantities from the initial flow state to the flow state after the heat addition process by dividing the total amount of heat added to the flow, $q$, into small portions, $\delta q$, and calculate the change in flow properties for each of these heat additions, see Figure~\ref{fig:dq}.\\

\begin{figure}[ht!]
\begin{center}
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/incremental-heat-addition.pdf}
\end{center}
\caption{Change in flow quantities due to the addition of an infinitesimal amount of heat $\delta q$}
\label{fig:dq}
\end{figure}

\noindent Let's first examine the temperature change by rewriting Eqn.~\ref{eq:governing:dT:diff:final} as\\

\begin{equation}
dT=\dfrac{1-\gamma M^2}{1-M^2}dT_o\Leftrightarrow \dfrac{dT}{dT_o}=\dfrac{1-\gamma M^2}{1-M^2}
\label{eq:governing:dT:diff:mod:a}
\end{equation}\\

\noindent which is equivalent to\\

\begin{equation}
\dfrac{dh}{\delta q}=\dfrac{1-\gamma M^2}{1-M^2}
\label{eq:governing:dT:diff:mod:b}
\end{equation}\\

\noindent Form Eqn.~\ref{eq:governing:dT:diff:mod:a} we can make the following observation\\

\[\dfrac{dT}{dT_o}=0\Rightarrow \gamma M^2=1\Rightarrow M=\sqrt{1/\gamma}\]\\

\noindent which means that the maximum temperature will be reached when the Mach number is $\sqrt{1/\gamma}$. Since $\gamma$ is a number grreter than one for all gases, this implies that the maximum temperature can only be reached if the flow is subsonic. For air, this the maximum temperature will be reached at $M=0.845$.\\

\noindent If we evaluate Eqn.~\ref{eq:governing:dT:diff:mod:a} for sonic flow ($M=1$), we see that the derivative becomes infinite.\\

\[|M|\rightarrow 1.0 \Rightarrow \dfrac{dT}{dT_o}\rightarrow \pm \infty\]\\

\noindent Now, by specifying an initial subsonic flow state and dividing the heat addition corresponding to choked flow, $q^\ast$, into small portions $\delta q$, one can perform integration as indicated in Figure~\ref{fig:dq}. The result is presented in the in Figure~\ref{fig:TS:closeup}. The subsonic process corresponds to the upper line. As heat is added the Mach number is increased and at $M=\gamma^{-1/2}$ the maximum temperature is reached. Adding more heat will reduce the temperature and increase the Mach number until sonic conditions are reached ($M=1.0$). As can be seen in Figure~\ref{fig:TS:closeup}, the lean of the subsonic branch of the Rayleigh line is lower than the isobars (gray lines), which means the increasing heat will reduce pressure. The lower part of the blue line in Figure~\ref{fig:TS:closeup} is the supersonic branch of the Rayleigh line, which is obtained in the same way starting from a supersonic flow condition. A flow state resulting in the same sonic conditions as for the subsonic case is calculated and used as a starting state. The corresponding $q^\ast$ is calculated and the same calculation of consecutive flow states in a step-wise manner is performed. As can be seen in Figure~\ref{fig:TS:closeup}, the lean of the supersonic part of the Rayleigh curve is steeper than the isobars (gray lines), which means that pressure increases as heat is added to the flow. As we saw from Eqn.~\ref{eq:governing:dT:diff:mod:b}, $dT/dT_o$ becomes infinite when the flow approaches the sonic the sonic state. After the sonic state is reached, further heat addition is impossible without changing the upstream flow conditions. This will be made clearer in the next section.\\ 

\noindent Using the differential relations above, we can get a good picture of the development of flow variables as heat is continuously added to the flow (see Figure~\ref{fig:rayleigh:trends}).

\begin{figure}[ht!]
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-subsonic-trends.pdf}
\caption{trends (subsonic flow)}
\end{subfigure}
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-supersonic-trends.pdf}
\caption{trends (supersonic flow)}
\end{subfigure}
\caption{Change in flow variables as heat is continuously added to a subsonic flow (left) and supersonic flow (right).}
\label{fig:rayleigh:trends}
\end{figure}

\begin{figure}[ht!]
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-close-up.pdf}
\caption{The Rayleigh line (the blue line) in a Ts-diagram. Gray lines are constant-pressure lines (isobars).}
\label{fig:TS:closeup}
\end{figure}

==== Rayleigh Line ====

\noindent The continuity equation for steady-state, one-dimensional flow reads

\begin{equation}
\rho_1 u_1 = \rho_2 u_2 = C
\label{eq:governing:cont}
\end{equation}\\

\noindent where $C$ is the massflow per square meter (massflow divided by area). Inserted in the momentum equation we get\\

\begin{equation}
p_1+\dfrac{C^2}{\rho_1}=p_2+\dfrac{C^2}{\rho_2} \Leftrightarrow p_1+\nu_1 C^2=p_2+\nu_2 C^2\Rightarrow \dfrac{p_2-p_1}{\nu_2-\nu_1}=-C^2
\label{eq:governing:mom:b}
\end{equation}\\

\noindent Eqn.~\ref{eq:governing:mom:b} tells us that any solution to the governing flow equations must lie along a line (a so-called Rayleigh line) in a $p\nu$-diagram. In Figure~\ref{fig:PV}, 1 corresponds to the flow state before heat addition and states 2 and 3 corresponds to the flow state after heat is added. If the flow in state 1 is subsonic, adding heat will change the flow state following the Rayleigh line to the right, i.e. towards flow state 2. If the initial flow state instead is supersonic, heat addition will move the flow state towards state 3.\\

\begin{figure}[ht!]
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-pv.pdf}
\caption{The Rayleigh line in a $p\nu$-diagram. The heat addition process will follow the Rayleigh line, i.e. all solutions to the equations will be on the line. The lean of the line depends on the massflow. }
\label{fig:PV}
\end{figure}

\noindent Now we know in which direction we will move along the Rayleigh curve when heat is added but in order to find the flow state after heat addition we need to add the energy equation to the problem. If we draw a curve corresponding to the energy equation including the heat addition in the same $p\nu$-diagram, the intersection of this curve and the Rayleigh line corresponds to the downstream flow state (the flow state that fulfils the continuity, momentum, and energy equations). To be able to do this we will rewrite the energy equation such that it can be represented by a line in the $p\nu$-diagram.\\

\noindent The energy equation for one-dimensional flow with heat addition reads\\

\begin{equation}
h_1+\dfrac{1}{2}u_1^2+q=h_2+\dfrac{1}{2}u_2^2
\label{eq:governing:energy}
\end{equation}\\

\noindent Inserting the constant $C$ from above (the massflow per $m^2$) and and and $h=C_pT$, we get\\

\begin{equation}
\dfrac{\gamma R}{\gamma - 1}T_1+\dfrac{1}{2}C^2\nu_1^2+q=\dfrac{\gamma R}{\gamma-1}+\dfrac{1}{2}C^2\nu_2^2
\label{eq:governing:energy:b}
\end{equation}\\

\noindent which may be rewritten as\\

\begin{equation}
\dfrac{p_2}{p_1}=\left(\dfrac{\nu_2}{\nu_1}-\dfrac{\gamma+1}{\gamma-1}-\dfrac{2q}{RT_1}\right)\left(1-\dfrac{\gamma+1}{\gamma-1}\dfrac{\nu_2}{\nu_1}\right)^{-1}
\label{eq:governing:energy:c}
\end{equation}\\

\begin{figure}[ht!]
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-pv-subsonic-1.pdf}
\caption{$p\nu$-diagram}
\end{subfigure}
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-subsonic-1.pdf}
\caption{$Ts$-diagram}
\end{subfigure}
\caption{Subsonic heat addition. The filled blue circle denotes the start condition ($M_1=0.2$) and the filled orange circle denotes the flow state after heat addition ($M_2=0.6$). Blue and orange circles denote the corresponding total pressure (left) and total temperature (right), respectively. Dashed lines are isentropes (lines with constant entropy). Gray lines are isotherms (left) and isobars (right), respectively. In the left figure, the solid black line is the Rayleigh line, the solid blue line corresponds to the energy equation before heat addition and the solid orange line represents the energy equation after heat addition.}
\label{fig:TSPV:a}
\end{figure}

\begin{figure}[ht!]
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-pv-subsonic-2.pdf}
\caption{$p\nu$-diagram}
\end{subfigure}
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-subsonic-2.pdf}
\caption{$Ts$-diagram}
\end{subfigure}
\caption{Subsonic heat addition. The filled blue circle denotes the start condition ($M_1=0.2$) and the filled orange circle denotes the flow state after heat addition ($M_2=1.0$). Blue and orange circles denote the corresponding total pressure (left) and total temperature (right), respectively. Dashed lines are isentropes (lines with constant entropy). Gray lines are isotherms (left) and isobars (right), respectively. In the left figure, the solid black line is the Rayleigh line, the solid blue line corresponds to the energy equation before heat addition and the solid orange line represents the energy equation after heat addition.}
\label{fig:TSPV:b}
\end{figure}

\begin{figure}[ht!]
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-pv-supersonic-1.pdf}
\caption{$p\nu$-diagram}
\end{subfigure}
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-supersonic-1.pdf}
\caption{$Ts$-diagram}
\end{subfigure}
\caption{Supersonic heat addition. The filled blue circle denotes the start condition ($M_1=1.8$) and the filled orange circle denotes the flow state after heat addition ($M_2=1.4$). Blue and orange circles denote the corresponding total pressure (left) and total temperature (right), respectively. Dashed lines are isentropes (lines with constant entropy). Gray lines are isotherms (left) and isobars (right), respectively. In the left figure, the solid black line is the Rayleigh line, the solid blue line corresponds to the energy equation before heat addition and the solid orange line represents the energy equation after heat addition.}
\label{fig:TSPV:c}
\end{figure}

\begin{figure}[ht!]
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-pv-supersonic-2.pdf}
\caption{$p\nu$-diagram}
\end{subfigure}
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-supersonic-2.pdf}
\caption{$Ts$-diagram}
\end{subfigure}
\caption{Supersonic heat addition. The filled blue circle denotes the start condition ($M_1=1.8$) and the filled orange circle denotes the flow state after heat addition ($M_2=1.0$). Blue and orange circles denote the corresponding total pressure (left) and total temperature (right), respectively. Dashed lines are isentropes (lines with constant entropy). Gray lines are isotherms (left) and isobars (right), respectively. In the left figure, the solid black line is the Rayleigh line, the solid blue line corresponds to the energy equation before heat addition and the solid orange line represents the energy equation after heat addition.}
\label{fig:TSPV:d}
\end{figure}

\noindent As you can see in the examples above (Figures~\ref{fig:TSPV:b} and \ref{fig:TSPV:d}), sonic conditions are reached when the Rayleigh line is tangent to the curve representing the energy equation in the $p\nu$-diagram. Adding more heat would move the energy equation line upwards and thus there can not be any solution after reaching this state unless the upstream conditions are changed such that the energy line intersects the Rayleigh line after further heat addition. Let's have a second look at the equations and see if it is possible to verify that the case where the Rayleigh line is a tangent to the energy-equation curve is in fact the sonic state.\\

\noindent Starting from Eqn.~\ref{eq:governing:energy:b}, it is easy to see that for any point along the energy equation curve the flow state may be expressed as a function of the initial flow state and the added heat $q$ as\\

\begin{equation}
\dfrac{\gamma}{\gamma-1}p\nu+\dfrac{1}{2}C^2\nu^2=\dfrac{\gamma}{\gamma-1}p_1\nu_1+\dfrac{1}{2}C^2\nu_1^2+q=D
\label{eq:governing:energy:d}
\end{equation}\\

\noindent where $D$ is a constant.\\

\noindent Now, let's different the Eqn.\ref{eq:governing:energy:d} with respect to $\nu$\\

\begin{equation}
\dfrac{\gamma}{\gamma-1}\left(\nu\dfrac{dp}{d\nu}+p\right)+C^2\nu=0\Rightarrow \dfrac{dp}{d\nu}=-\dfrac{\gamma}{\gamma-1}C^2-\dfrac{p}{\nu}
\label{eq:governing:energy:e}
\end{equation}\\

\noindent The Rayleigh line is a tangent to the energy equation curve when $dp/d\nu=-C^2$ and thus\\

\begin{equation}
\dfrac{C^2}{\gamma}=\dfrac{p}{\nu}
\label{eq:governing:energy:f}
\end{equation}\\

\noindent By definition $C=\rho u$ and $\nu=1/\rho$, which inserted in Eqn.~\ref{eq:governing:energy:f} gives\\

\begin{equation}
u=\sqrt{\dfrac{\gamma p}{\rho}}=a
\label{eq:governing:energy:g}
\end{equation}\\

==== Thermal Choking ====

\noindent When the heat addition reaches $q^\ast$ the flow becomes sonic and the flow is said to thermally choked. Thermal choking is illustrated in Figure~\ref{fig:TSPV:d}, where the curve representing the energy equation (the blue line in the $p\nu$-diagram) is tangent to the Rayleigh line and if more heat is added the blue line will move to the right of the Rayleigh line and thus there are no solutions for $q>q^\ast$. So what happens if more heat is added to the flow after thermal choking is reached. The answer is different if the flow is subsonic or supersonic. For a subsonic flow, the upstream flow will be adjusted such that the slope of the Rayleigh line changes and the energy equation curve becomes tangent to the Rayleigh line. This means that the massflow per unit area ($C$) is reduced and $q^\ast$ is increased such that $q^\ast$ equals the heat added to the flow. Note that the upstream total conditions will not be changed in this process (see Figure~\ref{fig:thermal:choking:sub}).

\[
\begin{aligned}
M_{1'} & = f(q^\ast)\\
T_{1'} & = f(T_o, M_{1'})\\
p_{1'} & = f(p_o, M_{1'})\\
\rho_{1'} & = f(p_{1'}, T_{1'})\\
a_{1'} & = f(T_{1'})\\
u_{1'} & = M_{1'}a_{1'}\\
\end{aligned}
\] 

\begin{figure}[ht!]
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-subsonic-choked-mod.pdf}
\caption{$Ts$-diagram}
\end{subfigure}
\begin{subfigure}[b]{0.5\textwidth}
\centering
\includegraphics[]{figures/standalone-figures/Chapter04/pdf/rayleigh-Ts-subsonic-choked-mod-close-up.pdf}
\caption{$Ts$-diagram (close up)}
\end{subfigure}
\caption{For thermally choked subsonic flow, further heat addition will lead to an updated of the inlet static conditions such that the massflow per unit area is changed and the heat corresponding to thermal choking $q^\ast$ is increased.}
\label{fig:thermal:choking:sub}
\end{figure}

\noindent In a choked supersonic flow, there is no possibility for pressure waves to travel upstream in the flow and thus the upstream flow conditions can not be changed as in the subsonic case. Moreover, since a normal shock is an adiabatic process (a jump between two points on the same Rayleigh line), the total temperature is not changed over a chock. From before we have

\[\dfrac{T_o}{T_o^\ast}=\dfrac{(\gamma+1)M_1^2}{(1+\gamma M_1^2)^2}(2+(\gamma-1)M_1^2)\] 

\noindent Inserting the normal shock relation

\[M_2^2=\dfrac{2+(\gamma-1)M_1^2}{2\gamma M_1^2-(\gamma-1)}\]

\noindent one can show that 

\[\dfrac{T_o}{T_o^\ast}=\dfrac{(\gamma+1)M_2^2}{(1+\gamma M_2^2)^2}(2+(\gamma-1)M_2^2)\] 

\noindent and thus $T_o^\ast$ is not changed by the normal shock and consequently $q^\ast$ is unchanged if there is a normal shock between station 1 and 2. So, it is not possible to change the upstream static flow conditions and a normal shock will not make it possible to add more heat. The only possible solution is a normal shock upstream of station 1 and thus subsonic flow through the heat addition process.