Drawing constant pressure lines in flow field

Click For Summary
To draw lines of constant pressure in an inviscid flow field, such as flow around a cylinder, Bernoulli's equation is essential for determining pressure variations. The pressure distribution can be expressed using specific equations derived from Bernoulli's principle, which relate pressure to velocity and the stream function. The discussion highlights the importance of coordinate systems when analyzing the relationship between the stream function and velocity, with suggestions to use Cartesian or cylindrical coordinates for clarity. Additionally, it is noted that lines of constant pressure are perpendicular to streamlines, emphasizing the need to understand the pressure gradient in relation to the flow direction. Overall, the conversation revolves around the mathematical foundations necessary to accurately depict pressure lines in fluid dynamics.
member 428835
Hi PF!

Can someone help me understand how to draw lines of constant pressure in an inviscid flow field, say flow around a cylinder. I am having trouble understanding how to draw these. Any help is greatly appreciated!

I ask this question because I am preparing for the Q exam for PhD and one of my classmates asked me about a Hele-Shaw flow: imagine two circular plates very close to each other (infinitely close). Now compare the streamlines of this Hele-Shaw flow and inviscid flow around a cylinder. Also draw lines of constant pressure for both cases. Evidently the streamlines looks identical but the pressure lines are different.
 
Last edited by a moderator:
Engineering news on Phys.org
What is your equation for the variations of pressure in inviscid flow?
 
Chestermiller said:
What is your equation for the variations of pressure in inviscid flow?
Bernoulli's equation, will give a pressure distribution for inviscid flow regimes, so this could give us the pressure variations too, right? For flow around a cylinder this is expressed as $$p = \frac{1}{2} \rho U^2 (2 R^2 \cos(2\theta)/r^2-R^4/r^4)+p_\infty$$
 
joshmccraney said:
Bernoulli's equation, will give a pressure distribution for inviscid flow regimes, so this could give us the pressure variations too, right? For flow around a cylinder this is expressed as $$p = \frac{1}{2} \rho U^2 (2 R^2 \cos(2\theta)/r^2-R^4/r^4)+p_\infty$$
Yes. That's fine. How about in general, in terms of the stream function.
 
Chestermiller said:
Yes. That's fine. How about in general, in terms of the stream function.
My thoughts are to take Bernoullis equation ##p + \rho v^2/2 =p_\infty + \rho u_\infty^2/2## (ignoring unsteady and gravity terms) and then write ##v## in terms of the streamfunction. but this will depend on the coordinate system we choose. Since you're asking for a "general" description I'm confused what coordinate system to represent ##\psi## in. Or am I missing the point?
 
joshmccraney said:
My thoughts are to take Bernoullis equation ##p + \rho v^2/2 =p_\infty + \rho u_\infty^2/2## (ignoring unsteady and gravity terms) and then write ##v## in terms of the streamfunction. but this will depend on the coordinate system we choose. Since you're asking for a "general" description I'm confused what coordinate system to represent ##\psi## in. Or am I missing the point?
You should be able to do it irrespective of the coordinate system.
 
In 2D, what is the gradient of the stream function dotted with itself?
 
Chestermiller said:
In 2D, what is the gradient of the stream function dotted with itself?
You're asking for ##\nabla \psi \cdot \nabla \psi##? I am not sure. I know ##\nabla \psi## is normal to the velocity, but this is all I can say about it, and without selecting a coordinate system I am not sure how to proceed. Any help?
 
joshmccraney said:
You're asking for ##\nabla \psi \cdot \nabla \psi##? I am not sure. I know ##\nabla \psi## is normal to the velocity, but this is all I can say about it, and without selecting a coordinate system I am not sure how to proceed. Any help?
Isn't it ##V^2##?
 
  • #10
Chestermiller said:
Isn't it ##V^2##?
Is it? I've always seen the relationship with ##\psi## and the velocity as either ##\vec{V} = \nabla \times \psi \vec{e}## where ##\vec{e}## is the basis vector we do not need in order to describe the flow. How could I prove ##\nabla \psi \cdot \nabla \psi = V^2##?
 
  • #11
joshmccraney said:
Is it? I've always seen the relationship with ##\psi## and the velocity as either ##\vec{V} = \nabla \times \psi \vec{e}## where ##\vec{e}## is the basis vector we do not need in order to describe the flow. How could I prove ##\nabla \psi \cdot \nabla \psi = V^2##?
Just do it in cartesian coordinates.
 
  • #12
Chestermiller said:
Just do it in cartesian coordinates.
Yea, I see it's true in cartesian, but writing this in cartesian coordinates goes against your comment in post 6. Could you direct me where to go to find the general proof that ##\nabla\psi\cdot\nabla\psi=V^2##? I've searched around but have been unable to find anything.
 
  • #13
joshmccraney said:
Yea, I see it's true in cartesian, but writing this in cartesian coordinates goes against your comment in post 6. Could you direct me where to go to find the general proof that ##\nabla\psi\cdot\nabla\psi=V^2##? I've searched around but have been unable to find anything.
I don't have a reference. Try cylindrical and see if it works for that.
 
  • #14
Chestermiller said:
I don't have a reference. Try cylindrical and see if it works for that.
Ok, so in cylindrical I'll assume we have flow only in ##r## and ##\theta##, so there is no ##z## component (I could do a different flow if you prefer?). Define the streamfunction ##\psi## as $$\vec{V} = \nabla \times \psi \hat{z} =-\frac{\psi_\theta}{r}\hat{r}+\psi_r\hat{\theta} \implies\\ |\vec{V}|^2 = v_r^2+v_\theta^2 = \frac{\psi_\theta^2}{r^2}+\psi_r^2$$ and notice
$$\nabla \psi \cdot\nabla\psi = \frac{\psi_\theta^2}{r^2}+\psi_r^2$$ so this works. Bernoullis is then
$$p + \rho v^2/2 =p_\infty + \rho u_\infty^2/2 \implies\\ p =p_\infty + \rho u_\infty^2/2 - \rho \nabla\psi\cdot\nabla\psi/2.$$
But then how to draw ##p##; I don't see how writing it in terms of the streamfunction helps. Any ideas?
 
  • #15
joshmccraney said:
Ok, so in cylindrical I'll assume we have flow only in ##r## and ##\theta##, so there is no ##z## component (I could do a different flow if you prefer?). Define the streamfunction ##\psi## as $$\vec{V} = \nabla \times \psi \hat{z} =-\frac{\psi_\theta}{r}\hat{r}+\psi_r\hat{\theta} \implies\\ |\vec{V}|^2 = v_r^2+v_\theta^2 = \frac{\psi_\theta^2}{r^2}+\psi_r^2$$ and notice
$$\nabla \psi \cdot\nabla\psi = \frac{\psi_\theta^2}{r^2}+\psi_r^2$$ so this works. Bernoullis is then
$$p + \rho v^2/2 =p_\infty + \rho u_\infty^2/2 \implies\\ p =p_\infty + \rho u_\infty^2/2 - \rho \nabla\psi\cdot\nabla\psi/2.$$
But then how to draw ##p##; I don't see how writing it in terms of the streamfunction helps. Any ideas?
You calculate p on a grid, and then use a graphics package with 2D contour plotting capability to draw the diagram showing the lines of constant p.
 
  • #16
Chestermiller said:
You calculate p on a grid, and then use a graphics package with 2D contour plotting capability to draw the diagram showing the lines of constant p.
So there's no real way to intuitively do this sort of thing "on the fly"?
 
  • #17
There are complete analytic solutions for stream function and velocity potential for a few idealised situations .

These can sometimes be used to generate analytic solutions for more practical problems .

They are also useful when devising efficient numerical solution methods and when just sketching flow patterns .

http://www.freestudy.co.uk/fluid mechanics/t5203.pdf

Ch.4-7 are most relevant .
 
  • #18
joshmccraney said:
So there's no real way to intuitively do this sort of thing "on the fly"?
I don't know what you mean. In some cases, you can solve for ##\psi## as a function of the spatial coordinates, and then solve for the lines of constant ##\psi##.
 
  • #19
Chestermiller said:
I don't know what you mean. In some cases, you can solve for ##\psi## as a function of the spatial coordinates, and then solve for the lines of constant ##\psi##.
Sorry for the ambiguity: by "intuitive" I mean, can you look at a velocity field with a known geometry and infer the pressure lines? For example, the streamlines of a flow around a cylinder are not normal to lines of constant pressure. However, if we have to cylindrical plates that are very very close, evidently the streamlines won't change, yet now the pressure is always normal to the streamlines. Can you help me understand why this is and how I would know they are normal to the streamlines?
 
  • #20
If the lines of constant pressure are perpendicular to the streamlines, then the gradient of pressure is in the same direction as the velocity vector. Using the Navier Stokes equations, what can you do to test this?
 

Similar threads

Replies
0
Views
2K
  • · Replies 16 ·
Replies
16
Views
5K
Replies
4
Views
2K
  • · Replies 45 ·
2
Replies
45
Views
6K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 8 ·
Replies
8
Views
4K