Elementary Flow: Source/Sink Flow

In my previous post on uniform flow, we saw how we can use the velocity potential to find the velocity component of the flow at discrete grid points. We will use this methodology again here to find the velocity induced at discrete grid points from a source/sink in the flow. The velocity of source/sink flow is given below (with no derivation here).

(1)   \begin{equation*} \varphi_s = \frac{\Lambda}{2\pi}\text{ln}\left(r\right) \end{equation*}

We can see that the velocity potential is a function of the radial distance from the origin of the source (r), and so most textbooks will solve for the radial and angular components of the velocity (V_r and V_\theta). We will stick with the Cartesian coordinates here though, because it will show another method and it will also be helpful in later derivations of the source panel method (SPM) and vortex panel method (VPM). The source strength (uppercase lambda), \Lambda, is constant here, so we can take it out of the derivative term.

(2)   \begin{equation*} \begin{aligned} V_x &= \frac{\partial \varphi_s}{\partial x} = \frac{\Lambda}{2\pi}\frac{\partial \text{ln}\left(r\right)}{\partial x} = \frac{\Lambda}{2\pi r} \frac{\partial r}{\partial x} \\[5pt] V_y &= \frac{\partial \varphi_s}{\partial y} = \frac{\Lambda}{2\pi}\frac{\partial \text{ln}\left(r\right)}{\partial y} = \frac{\Lambda}{2\pi r} \frac{\partial r}{\partial y} \end{aligned} \end{equation*}

The velocity induced at point \text{P} (X_\text{P}, Y_\text{P}) depends on the distance from the sourse/sink origin (X_0, Y_0), r_\text{P}, which is defined below.

(3)   \begin{equation*} r_\text{P} = \sqrt{\left(X_\text{P}-X_0\right)^2 + \left(Y_\text{P}-Y_0\right)^2} \end{equation*}

Performing the derivative using the chain rule, we get the following expression for the partial derivatives.

(4)   \begin{equation*} \begin{aligned} \frac{\partial r_\text{P}}{\partial x} &= \frac{1}{2}\left[\left(X_\text{P}-X_0\right)^2 + \left(Y_\text{P}-Y_0\right)^2\right]^{-1/2}\left(2\right)\left(X_\text{P}-X_0\right) \\[2pt] &= \frac{\left(X_\text{P}-X_0\right)}{r_\text{P}} \\[2pt] \frac{\partial r_\text{P}}{\partial y} &= \frac{1}{2}\left[\left(X_\text{P}-X_0\right)^2 + \left(Y_\text{P}-Y_0\right)^2\right]^{-1/2}\left(2\right)\left(Y_\text{P}-Y_0\right)\\[2pt] &= \frac{\left(Y_\text{P}-Y_0\right)}{r_\text{P}} \end{aligned} \end{equation*}

Plugging these expressions into the V_x and V_y equations from Eq. 2, we obtain the following.

(5)   \begin{equation*} \begin{aligned} V_x &= \frac{\Lambda \left(X_\text{P}-X_0\right)}{2\pi r_\text{P}^2} \\[2pt] V_y &= \frac{\Lambda \left(Y_\text{P}-Y_0\right)}{2\pi r_\text{P}^2} \end{aligned} \end{equation*}

We can code the source/sink flow in the same way we coded the uniform flow. Note that in Python, lambda is a reserved keyword that is used to create an anonymous function, so I have used lmbda instead in my Python code. To create a source flow, the value of \Lambda must be positive, while for sink flow \Lambda is negative.

% Source/sink knowns
lambda = 1;									 % Source/sink magnitude
X0     = 0;									 % Source/sink X origin
Y0     = 0;									 % Source/sink Y origin

% Create the grid
numX = 20;                        % Number of X points
numY = 20;	                      % Number of Y points
X    = linspace(-10,10,numX)';		% Create X points array
Y    = linspace(-10,10,numY)';		% Create Y points array
[XX,YY] = meshgrid(X,Y);					% Create the meshgrid

% Solve for velocities
Vx = zeros(numX,numY);			    % Initialize X velocity
Vy = zeros(numX,numY);			    % Initialize Y velocity
for i = 1:1:numX							  % Loop over X-points
	for j = 1:1:numY						  % Loop over Y-points
		x  = XX(i,j);						   % X-value of current point
		y  = YY(i,j);						   % Y-value of current point
		dx = x - X0;						    % X distance
		dy = y - Y0;						    % Y distance
		r  = sqrt(dx^2 + dy^2);				     % Distance (Eq. 3)
		Vx(i,j) = (lambda*dx)/(2*pi*r^2);	 % X velocity (Eq. 4)
		Vy(i,j) = (lambda*dy)/(2*pi*r^2);	 % Y velocity (Eq. 4)
		
		V(i,j)  = sqrt(Vx(i,j)^2+Vy(i,j)^2); % Total velocity
		Vr(i,j) = lambda/(2*pi*r);			     % Radial velocity
	end
end

% Plot the velocity on the grid
figure(1);									   % Create figure
cla; hold on; grid off;		    % Get ready for plotting
set(gcf,'Color','White');	    % Set background to white
set(gca,'FontSize',12);		    % Change font size
quiver(X,Y,Vx,Vy,'r');			   % Velocity vector arrows
xlim([min(X) max(X)]);			   % Set X-axis limits
ylim([min(Y) max(Y)]);			   % Set Y-axis limits
xlabel('X Axis');							% Set X-axis label
ylabel('Y Axis');							% Set Y-axis label
title('Source/Sink Flow');		 % Set title

Since the source and sink flow is usually described by the radial and angular components, let’s compute their velocities below (V_r computed on line 27 in the code).

(6)   \begin{equation*} \begin{aligned} V_r &= \frac{\partial \varphi}{\partial r} = \frac{\Lambda}{2\pi r} \\ V_\theta &= \frac{1}{r} \frac{\partial \varphi}{\partial \theta} = 0 \end{aligned} \end{equation*}

Since the angular component of the velocity is zero, we can compare the magnitude of the radial component to the magnitude of the velocity from the Cartesian V_x and V_y components. In the code (line 26), the Cartesian velocity magnitude is V. Comparing these two matrices, it is clear that they are the same, which is a good check that our Cartesian velocity derivation is correct.

The results for source and sink flow can be seen in Fig. 1 and Fig. 2, respectively. The velocity vector arrows either point directly out from the origin (source) or directly into the origin (sink).

Figure 1: Source flow with a strength of \Lambda = 1. Blue line is curve along which the circulation is calculated
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Figure 2: Sink flow with a strength of \Lambda = -1.

We can also now compute the circulation around the solid blue curve as shown in Fig. 1. Again, the expected circulation is zero since there is no vortex in the flow, and this agrees with the computed circulation of \Lambda = -2.11419 \times 10^{-18}. The same circulation can be computed for the sink in Fig. 2, and the same results are obtained.

Source_Sink_Flow.m
Source_Sink_Flow.m

You will need the COMPUTE_CIRCULATION.m function file in the same folder in order to run this code.

COMPUTE_CIRCULATION.m
COMPUTE_CIRCULATION.m
Source_Sink_Flow.py
Source_Sink_Flow.py

You will need the COMPUTE_CIRCULATION.py function file in the same folder in order to run this code.

Note: I can’t upload “.py” files, so this is a “.txt” file. Just download it and change the extension to “.py”, and it should work fine.

COMPUTE_CIRCULATION.py
COMPUTE_CIRCULATION.py

Note: I can’t upload “.py” files, so this is a “.txt” file. Just download it and change the extension to “.py”, and it should work fine.

Elementary Flow: Uniform Flow

For this first (and simplest) flow, our discussion will appear a little circular. That is, first we will specify the x and y velocity components of a uniform flow (at an angle of attack, \alpha), then we will determine the velocity potential (\varphi_\text{u}), and then we will find the velocity components from that velocity potential. The reason is just to show that we can go forward or backwards. In the remaining elementary potential flow cases, we will start with the velocity potential (we won’t derive it) and find the x and y velocity components.

Our uniform flow needs to be, well, uniform. That is, the velocity (magnitude and orientation) needs to be the same at every point in the flow. This means that we can specify the magnitude and orientation once, and it will be the same for every (x, y) point in the flow. Let’s define the magnitude as V_\infty, and the orientation as \alpha, which can take any value from 0 to 2\pi radians (0^o to 360^o). This means we can get the x and y components of the velocity vectors (see Fig. 1) using the following equations.

(1)   \begin{equation*} \begin{aligned} V_x &= V_\infty \cos\left(\alpha\right) \\ V_y &= V_\infty \sin\left(\alpha\right) \end{aligned} \end{equation*}

Figure 1: Uniform flow vector definition.
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From the definition of the velocity potential, we know the following.

(2)   \begin{equation*} \begin{aligned} V_x &= \frac{\partial \varphi_u}{\partial x} \\ V_y &= \frac{\partial \varphi_u}{\partial y} \end{aligned} \end{equation*}

This means we can integrate the velocity we defined with respect to the appropriate variables (dx for V_x and dy for V_y).

(3)   \begin{equation*} \begin{aligned} \int V_\infty\cos\left(\alpha\right)dx \rightarrow\, & \varphi_u = V_\infty\cos\left(\alpha\right)x + f\left(y\right) \\ \int V_\infty\sin\left(\alpha\right)dy \rightarrow\, & \varphi_u = V_\infty\sin\left(\alpha\right)y + g\left(x\right) \end{aligned} \end{equation*}

We can find the velocity potential by noting that the first term in the first equation is a function of x (g\left(x\right)), and that the first term in the second equation is a function of y (f\left(y\right)).

(4)   \begin{equation*} \varphi_u = V_\infty\cos\left(\alpha\right)x + V_\infty\sin\left(\alpha\right)y \end{equation*}

Now we will come full circle and find the velocity components from the velocity potential.

(5)   \begin{equation*} \begin{aligned} V_x &= \frac{\partial \varphi_u}{\partial x} = V_\infty\cos\left(\alpha\right) \\ V_y &= \frac{\partial \varphi_u}{\partial y} = V_\infty\sin\left(\alpha\right) \end{aligned} \end{equation*}

Note that these are the same as the velocity components we defined at the beginning of this section, and that makes sense. If they were not the same, then we would have known that we made a mistake in our integration when solving for the velocity potential. We can see that the velocity components are independent of x and y, which means they will always be the same over the entire grid. Let’s put this to practice in the code below. The two knowns that we are specifying are the velocity magnitude and velocity angle.

% Velocity magnitude and angle
Vinf  = 1;							% Velocity magnitude
alpha = 0;							% Velocity vector angle [deg]

% Create the grid
numX = 10;							          % Number of X points
numY = 10;							          % Number of Y points
X    = linspace(-10,10,numX)';		% Create X points array
Y    = linspace(-10,10,numY)';		% Create Y points array

% Solve for velocities
Vx = zeros(numX,numY);				   % Initialize X velocity
Vy = zeros(numX,numY);				   % Initialize Y velocity
for i = 1:1:numX					       % Loop over X-points
	for j = 1:1:numY				       % Loop over Y-points
		Vx(i,j) = Vinf*cosd(alpha);	% X velocity (Eq. 5)
		Vy(i,j) = Vinf*sind(alpha);	% Y velocity (Eq. 5)
	end
end

% Plot the velocity on the grid
figure(1);							       % Create figure
cla; hold on; grid off;				% Get ready for plotting
set(gcf,'Color','White');			% Set background to white
set(gca,'FontSize',12);				% Labels font size
quiver(X,Y,Vx,Vy,'r');				 % Velocity vector arrows
xlim([min(X) max(X)]);				 % Set X-axis limits
ylim([min(Y) max(Y)]);				 % Set Y-axis limits
xlabel('X Axis');					    % Set X-axis label
ylabel('Y Axis');					    % Set Y-axis label
title('Uniform Flow');				 % Set title

The results of the code can be seen in the plots in Figs. 2 and 3. In Fig. 2, the angle of the velocity vector is zero (aligned with the x-axis), while in Fig. 3, the angle of the velocity vector is 30^o. We can see in both plots that the velocity vectors at every grid point are the same (uniform), and do not depend on their x and y locations, which is what we expected.

Figure 2: Uniform flow with \alpha = 0^o.
Figure 3: Uniform flow with \alpha = 30^o, and blue line for line integral to compute circulation.

In Fig. 3, the blue line represents the curve that we are computing the circulation along (see my circulation post). The line integral (and code) from my circulation post is used to calculate the circulation, which is equal to \Gamma = 7.702 \times 10^{-16}. This is expected that the circulation is nearly zero, since there is no vortex in the flow

Uniform_Flow.m
Uniform_Flow.m

You will need the COMPUTE_CIRCULATION.m function in the same directory in order to run this script.

COMPUTE_CIRCULATION.m
COMPUTE_CIRCULATION.m
Uniform_Flow.py
Uniform_Flow.py

You will need the COMPUTE_CIRCULATION.py function in the same directory in order to run this script.

Note: I can’t upload “.py” files, so this is a “.txt” file. Just download it and change the extension to “.py”, and it should work fine.

COMPUTE_CIRCULATION.py
COMPUTE_CIRCULATION.py

Note: I can’t upload “.py” files, so this is a “.txt” file. Just download it and change the extension to “.py”, and it should work fine.

Introduction to Incompressible Potential Flow

This post is not meant to be an exhaustive dive into potential flow; it is only meant as an introduction to incompressible potential flow and how we can use potential flow theory to get simplified solutions to some otherwise complicated problems.

When solving complex problems in aerodynamics, we can start with the most general equations we know, for instance, the Navier-Stokes equations (which themselves already have a couple of assumptions built in, but are not very limiting). These equations require detailed numerical solutions, so we would like to simplify them down by making some more valid assumptions. We will be making two assumptions here:

  1. Irrotational flow (angular velocity/vorticity is zero)
  2. Incompressible flow (density is constant)
Continue reading Introduction to Incompressible Potential Flow

Compute Circulation of a Vector Field in MATLAB and Python

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The MATLAB and Python code in this post accompany my YouTube video on how to compute circulation of an arbitrary vector field. Below you will find the MATLAB script and function.

Circulation.m
Circulation.m
COMPUTE_CIRCULATION.m
COMPUTE_CIRCULATION.m

Below you will find the Python script and function. I can’t upload .py files, so I have uploaded .txt files instead. You can download the files and change the extension to .py.

Circulation.py
Circulation.py
COMPUTE_CIRCULATION.py
COMPUTE_CIRCULATION.py

Note: I can’t upload “.py” files, so this is a “.txt” file. Just download it and change the extension to “.py”, and it should work fine.


Load Airfoil Data into MATLAB

In a previous post and video, we saved airfoil data files from the UIUC airfoil database in a folder on our computer. These files below accompany my video about how to load these files into MATLAB. You can download the three files below.

Test_Load_Airfoil_Function.m
Test_Load_Airfoil_Function.m
LOAD_AIRFOIL.m
LOAD_AIRFOIL.m
LOAD_AIRFOIL_SELIG.m
LOAD_AIRFOIL_SELIG.m

You can also view my YouTube video here.

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Running XFoil from Python

In one of my YouTube videos, I show how to run XFoil from a MATLAB script. For those of you that don’t have MATLAB or prefer Python, here is the same script, but now in Python. The functionality should be the exact same. I have uploaded a .txt file with the Python code because I am not able to upload Python files to my website at the moment. Just save it as a .py file when you download it (it will open in a new window).

Python_XFoil.py
Python_XFoil.py

The code can also be seen below.

import os
import numpy as np
import matplotlib.pyplot as plt

# %% CREATE LOADING FILE

# Knowns
NACA       = '0012'
AoA        = '0'
numNodes   = '170'
saveFlnmAF = 'Save_Airfoil.txt'
saveFlnmCp = 'Save_Cp.txt'
xfoilFlnm  = 'xfoil_input.txt'

# Delete files if they exist
if os.path.exists(saveFlnmAF):
    os.remove(saveFlnmAF)

if os.path.exists(saveFlnmCp):
    os.remove(saveFlnmCp)
    
# Create the airfoil
fid = open(xfoilFlnm,"w")
fid.write("NACA " + NACA + "\n")
fid.write("PPAR\n")
fid.write("N " + numNodes + "\n")
fid.write("\n\n")
fid.write("PSAV " + saveFlnmAF + "\n")
fid.write("OPER\n")
fid.write("ALFA " + AoA + "\n")
fid.write("CPWR " + saveFlnmCp + "\n")
fid.close()

# Run the XFoil calling command
os.system("xfoil.exe < xfoil_input.txt")

# Delete file after running
if os.path.exists(xfoilFlnm):
    os.remove(xfoilFlnm)

# %% READ DATA FILE: AIRFOIL

flpth = "C:/Users/Josh/Documents/Python/Panel_Methods/"
flnm  = flpth + saveFlnmAF
    
# Load the data from the text file
dataBuffer = np.loadtxt(flnm, skiprows=0)

# Extract data from the loaded dataBuffer array
XB = dataBuffer[:,0]
YB = dataBuffer[:,1]

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if os.path.exists(saveFlnmAF):
    os.remove(saveFlnmAF)

# %% READ DATA FILE: PRESSURE COEFFICIENT

# Load the data from the text file
dataBuffer = np.loadtxt(saveFlnmCp, skiprows=3)

# Extract data from the loaded dataBuffer array
X_0  = dataBuffer[:,0]
Y_0  = dataBuffer[:,1]
Cp_0 = dataBuffer[:,2]

# Delete file after loading
if os.path.exists(saveFlnmCp):
    os.remove(saveFlnmCp)

# %% EXTRACT UPPER AND LOWER AIRFOIL DATA

# Split airfoil into (U)pper and (L)ower
XB_U = XB[YB >= 0]
XB_L = XB[YB < 0]
YB_U = YB[YB >= 0]
YB_L = YB[YB < 0]

# Split XFoil results into (U)pper and (L)ower
Cp_U = Cp_0[YB >= 0]
Cp_L = Cp_0[YB < 0]
X_U  = X_0[YB >= 0]
X_L  = X_0[YB < 0]

# %% PLOT DATA

# Plot airfoil
fig = plt.figure(1)
plt.cla()
plt.plot(XB_U,YB_U,'b.-',label='Upper')
plt.plot(XB_L,YB_L,'r.-',label='Lower')
plt.xlabel('X-Coordinate')
plt.ylabel('Y-Coordinate')
plt.title('Airfoil')
plt.axis('equal')
plt.legend()
plt.show()

# Plot pressure coefficient
fig = plt.figure(2)
plt.cla()
plt.plot(X_U,Cp_U,'b.-',label='Upper')
plt.plot(X_L,Cp_L,'r.-',label='Lower')
plt.xlim(0,1)
plt.xlabel('X-Axis')
plt.ylabel('Y-Axis')
plt.title('Pressure Coefficient')
plt.show()
plt.legend()
plt.gca().invert_yaxis()


UIUC Airfoil Database File Download

Below are the two Python codes used to download all the airfoils from the UIUC Airfoil Database, found here:

https://m-selig.ae.illinois.edu/ads/coord_database.html

For some reason, I can’t load .py files onto my website, so I’ve saved them as .txt files. You can press the download button, copy the text into a new file, and save it as a .py file.

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Get_Save_Airfoils.py
Get_Save_Airfoils.py
Get_Save_Airfoils_Selig.py
Get_Save_Airfoils_Selig.py

Running XFoil from MATLAB

Below you can download the MATLAB script from my YouTube video about how to run XFoil from MATLAB.  The .m file will open in a separate window.

MATLAB_XFOIL.m
MATLAB_XFOIL.m

The code can also be seen below (without line-by-line comments)

clear;
clc;

NACA       = '2412';
AoA        = '0';
numNodes   = '35';
saveFlnmAF = 'Save_Airfoil.txt';
saveFlnmCp = 'Save_Cp.txt';

% Delete files if they exist
if (exist(saveFlnmAF,'file'))
    delete(saveFlnmAF);
end
if (exist(saveFlnmCp,'file'))
    delete(saveFlnmCp);
end

% Create the airfoil
fid = fopen('xfoil_input.txt','w');
fprintf(fid,['NACA ' NACA '\n']);
fprintf(fid,'PPAR\n');
fprintf(fid,['N ' numNodes '\n']);
fprintf(fid,'\n\n');

% Save the airfoil data points
fprintf(fid,['PSAV ' saveFlnmAF '\n']);

% Find the Cp vs. X plot
fprintf(fid,'OPER\n');
fprintf(fid,['Alfa ' AoA '\n']);
fprintf(fid,['CPWR ' saveFlnmCp]);

% Close file
fclose(fid);

% Run XFoil using input file
cmd = 'xfoil.exe < xfoil_input.txt';
[status,result] = system(cmd);

%% READ DATA FILE: AIRFOIL

saveFlnmAF = 'Save_Airfoil.txt';
fidAirfoil = fopen(saveFlnmAF);  

dataBuffer = textscan(fidAirfoil,'%f %f','CollectOutput',1,...
                                 'Delimiter','','HeaderLines',0);
fclose(fidAirfoil);
delete(saveFlnmAF);

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XB = dataBuffer{1}(:,1);
YB = dataBuffer{1}(:,2);   

%% READ DATA FILE: PRESSURE COEFFICIENT
saveFlnmCp = 'Save_Cp.txt';
fidCP = fopen(saveFlnmCp);
dataBuffer = textscan(fidCP,'%f %f %f','HeaderLines',3,...
                            'CollectOutput',1,...
                            'Delimiter','');
fclose(fidCP);
delete(saveFlnmCp);

% Separate Cp data
X_0  = dataBuffer{1,1}(:,1);
Y_0  = dataBuffer{1,1}(:,2);
Cp_0 = dataBuffer{1,1}(:,3);

%% PLOT DATA

% Split airfoil into (U)pper and (L)ower
XB_U = XB(YB >= 0);
XB_L = XB(YB < 0);
YB_U = YB(YB >= 0);
YB_L = YB(YB < 0);

% Split Xfoil results into (U)pper and (L)ower
Cp_U = Cp_0(YB >= 0);
Cp_L = Cp_0(YB < 0);
X_U  = X_0(YB >= 0);
X_L  = X_0(YB < 0);

% Plot: Airfoil
figure(1);
cla; hold on; grid off;
set(gcf,'Color','White');
set(gca,'FontSize',12);
plot(XB_U,YB_U,'b.-');
plot(XB_L,YB_L,'r.-');
xlabel('X Coordinate');
ylabel('Y Coordinate');
axis equal;

% Plot: Pressure coefficient
figure(2);
cla; hold on; grid on;
set(gcf,'Color','White');
set(gca,'FontSize',12);
plot(X_U,Cp_U,'bo-','LineWidth',2);
plot(X_L,Cp_L,'ro-','LineWidth',2);
xlabel('X Coordinate');
ylabel('Cp');
ylim('auto');
set(gca,'Ydir','reverse')

CFD with SU2: Normal Shock in CD Nozzle

Below are links to the mesh (SU2) and configuration (CFG) files that are used in my video on how to simulate the normal shock in a converging-diverging nozzle.  I also included the mesh geometry file (GEO) as well in case you want to change the parameters of the mesh (e.g. mesh density).  I know it says Mesh_Sup, but it’s the same mesh as the Mesh_NSN.su2 file below it.

Mesh_Sup.geo
Mesh_Sup.geo

Mesh_NSN.su2
Mesh_NSN.su2

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Nozzle_NS_0p38.cfg
Nozzle_NS_0p38.cfg

Nozzle_NS_0p5.cfg
Nozzle_NS_0p5.cfg

CFD with SU2: Isentropic Supersonic Nozzle Flow

Below are the links to download the GEO, SU2, and CFG files that I use in my video for the supersonic isentropic flow in a rocket nozzle (this mesh will be used in all my rocket nozzle simulations).  You don’t need the GEO file unless you want to load it into GMSH and change the output options of the SU2 mesh file.  Right now, the mesh file uses a characteristic length of 0.05.  If you want a finer mesh, you can decrease this value.  If you want a coarser mesh, you can increase this value.

Mesh_Sup.geo
Mesh_Sup.geo

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Mesh_Sup.su2
Mesh_Sup.su2

Nozzle_Sup.cfg
Nozzle_Sup.cfg