Boundary condition for a flow past a spherical obstacle

In summary, the study of boundary conditions for fluid flow past a spherical obstacle involves analyzing how the fluid behaves at the surface of the sphere and in the surrounding domain. Key factors include the no-slip condition at the sphere's surface, where fluid velocity matches that of the sphere, and the far-field conditions, which dictate the flow characteristics far from the obstacle. The interaction between the fluid and the sphere influences flow patterns, pressure distribution, and potential vortex formation, making accurate boundary conditions essential for predicting fluid behavior and optimizing designs in various engineering applications.
  • #1
happyparticle
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Homework Statement
Consider the steady flow pattern produced when an impenetrable rigid spherical obstacle is placed in a uniformly flowing, incompressible, inviscid fluid.
Relevant Equations
##r(r,\theta, \phi) = V \hat{z} , r \to\infty##
##\vec{v} = - \nabla \Phi##
I'm trying to find how the author finds the boundary condition at ##r\to\infty## is ## \Phi(r,\theta, \phi) = - V r cos \theta##.

Using the spherical coordinates.

##- V \hat{z} = \nabla \Phi##

##- V ( cos \theta \hat{r} - sin \theta \hat{\theta}) = \frac{d \Phi}{dr}\hat{r} + 1/r \frac{d \Phi}{d \theta} \hat{\theta} + \frac{1}{r sin \theta} \frac{d \Phi}{ d \phi} \hat{\phi} ##

I'm not sure to understand why most of the terms vanishes.
 
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  • #2
happyparticle said:
I'm trying to find how the author finds the boundary condition at ##r\to\infty## is ## \Phi(r,\theta, \phi) = - V r cos \theta##.
What is the pattern of a uniformly flowing, incompressible, inviscid fluid before the obstacle is inserted into the flow? That's the same pattern the flow must approach at long distances (##r\rightarrow\infty##) after insertion of the object.
 
  • #3
renormalize said:
What is the pattern of a uniformly flowing, incompressible, inviscid fluid before the obstacle is inserted into the flow? That's the same pattern the flow must approach at long distances (##r\rightarrow\infty##) after insertion of the object.
I understand that part. However is more the mathematical part that I don't really understand. Where ##\Phi(r,\theta, \phi) = - V r cos \theta## come from.
 
  • #4
What are the velocity components far from the sphere?
 
  • #5
happyparticle said:
I understand that part. However is more the mathematical part that I don't really understand. Where ##\Phi(r,\theta, \phi) = - V r cos \theta## come from.

The background velocity is [itex]V\mathbf{e}_z[/itex].

The calculation is [tex]
\Phi = -\int \mathbf{v} \cdot d\mathbf{x}.[/tex] You can either do in cartesians, which is straightforward, or you can do in spherical polars; this however is much trickier, since the polar basis vectors are not constant, but vary with position, so that you cannot integrate component by component as you can with cartesians.
 
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  • #6
I think I'm even more confuse.

Using cartesians coordinates I have:

##-\vec{v} = \frac{d \Phi}{dx}\hat{x} + \frac{d \Phi}{dy}\hat{y} + \frac{d \Phi}{dz}\hat{z}##

##-V \hat{z} = \frac{d \Phi}{dx}\hat{x} + \frac{d \Phi}{dy}\hat{y} + \frac{d \Phi}{dz}\hat{z}##

It seems like you kept only the ##\hat{x}## component. Why?
Also, to have ##z = r cos \theta##, I must use polar coordinates.
 
  • #7
What are the components of the far-field velocity in spherical coordinates?
 
  • #8
Chestermiller said:
What are the components of the far-field velocity in spherical coordinates?
##V (cos \theta \hat{r} - sin \theta \hat{\theta})##
 
  • #9
happyparticle said:
##V (cos \theta \hat{r} - sin \theta \hat{\theta})##
So, at large r, $$\frac{\partial\Phi}{\partial r}=V\cos{\theta}$$ and $$\frac{\partial \Phi}{\partial \theta}=-Vr\sin{\theta}$$
 
  • #10
It seems like there is a issue with the sign. Is there an error on the page linked above?
 
  • #11
happyparticle said:
It seems like there is a issue with the sign. Is there an error on the page linked above?
Oops. I assumed that v was equal to the gradient of phi rather than minus the gradient of phi. So just flip the signs in my previous post.
 
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  • #12
happyparticle said:
It seems like you kept only the ##\hat{x}## component. Why?

The spherical object has no preferred axes, but the background flow does have one: the direction of the flow. In spherical polar coodinates, that direction is usually aligned with the [itex]\theta = 0[/itex] ray, which is the positive [itex]z[/itex] axis.

We are only interested in the gradient of the potential, so we can take the constant of integration to be zero.
 
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  • #13
Thank you!
 

FAQ: Boundary condition for a flow past a spherical obstacle

What are boundary conditions in fluid dynamics?

Boundary conditions in fluid dynamics are constraints that are applied to the flow field at the boundaries of the fluid domain. They define how the fluid interacts with solid surfaces or other fluids, and are essential for solving the governing equations of fluid flow, such as the Navier-Stokes equations.

What boundary conditions are typically used for flow past a spherical obstacle?

For flow past a spherical obstacle, the common boundary conditions include no-slip conditions at the surface of the sphere, where the fluid velocity equals the velocity of the sphere's surface, and far-field conditions at a distance from the sphere, where the flow is typically uniform and characterized by a specified velocity or pressure.

How does the no-slip boundary condition affect the flow around a sphere?

The no-slip boundary condition implies that the fluid in immediate contact with the surface of the sphere has zero relative velocity with respect to the sphere. This condition leads to the development of a boundary layer around the sphere, where the velocity gradient is significant, influencing the overall drag and flow patterns around the obstacle.

What is the significance of the far-field boundary condition?

The far-field boundary condition is significant because it defines the behavior of the fluid at a distance from the spherical obstacle, where the effects of the sphere are negligible. It is essential for ensuring that the flow returns to a uniform state and helps in accurately modeling the flow characteristics and predicting the forces acting on the sphere.

How do boundary conditions affect the numerical simulation of flow past a sphere?

Boundary conditions play a crucial role in numerical simulations, as they directly influence the accuracy and stability of the solution. Properly defined boundary conditions ensure that the numerical model captures the physical behavior of the flow, including the effects of viscosity, turbulence, and the interaction between the fluid and the sphere, ultimately impacting the results of the simulation.

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