What is the governing equation for incompressible, inviscid, irrotational flow?
The flow reduces to solving Laplace’s equation: ∇²φ = 0
Solutions of this equation are called harmonic functions.
What boundary conditions are required to solve Laplace’s equation in aerodynamic problems?
At infinity: velocity → free-stream condition.
On a stationary surface: (u · n) = 0.
On a moving surface: (u - u_body) · n = 0.
Tangential velocity is unconstrained in inviscid flow.
What is the significance of solving Laplace’s equation in aerodynamics?
Once φ is known, velocity is u = ∇φ. Pressure is found using Bernoulli’s equation, and aerodynamic forces are obtained from pressure integration over surfaces.
Why can solutions to Laplace’s equation be linearly combined?
Because ∇² is linear: if ∇²φ = 0 and ∇²ψ = 0, then C1φ + C2ψ is also a solution. [SUPERPOSITION PRINCIPLE]
Give an example of using superposition to construct a new flow solution.
Combining uniform horizontal flow Ux and uniform vertical flow Vy gives the solution Ux + Vy, representing a uniform flow inclined to the x-axis.
What flow is obtained by superposing Ux and a 2D source (Q / 2π) ln r?
The Rankine ogive flow, representing a uniform stream disturbed by a source (or sink), forming a streamlined body shape.
Why is the derivative of a harmonic function also harmonic?
Because derivatives commute with the Laplacian:
∇²(∂φ/∂A) = ∂(∇²φ)/∂A = 0
if φ is harmonic.
A derivative is the limit of the distance between two functions. If these functions are harmonic, so will the derivative be.
What physical structure results from taking the derivative of a source potential with respect to its position?
A dipole (doublet) representing a source and a nearby sink.
2D: φ ≈ (A cosθ) / r
3D: φ ≈ (A cosθ) / r²
How can the flow around a cylinder or sphere be constructed?
By superposing a uniform flow potential with a dipole potential aligned with the free-stream direction.
How do complex functions help generate harmonic solutions in 2D?
If F(z) is analytic, where z = x + i y, then both Re[F(z)] and Im[F(z)] satisfy Laplace’s equation.
Example: F(z) = z² = x² − y² + 2i xy → x² − y² and 2xy are harmonic
What is the advantage of using conformal mapping?
If z = z(w) is a mapping and F(z) is analytic, then G(w) = F[z(w)] is analytic too. This generates new harmonic solutions in transformed geometries.
hat boundary conditions apply for flow around a stationary sphere?
At infinity: φ → Ux
At the surface (r = R): radial velocity ur = 0
What is the general form of the potential for uniform flow plus a dipole?
φ = U ( r cosθ + (a cosθ) / r² )
How is the dipole strength a determined?
Apply ∂φ/∂r = 0 at r = R:
cosθ (1 - 2a / R³) = 0 → a = R³ / 2
What is the final potential for flow around a stationary sphere?
φ = U cosθ ( r + R³ / (2 r²) )
What is the physical meaning of the dipole term?
It represents the induced velocity from the sphere’s presence, required to satisfy the no-penetration condition on the surface.
How does the boundary condition change for a breathing sphere?
Instead of ∂φ/∂r = 0, the boundary condition is:
(∂φ/∂r) at r = R = dR/dt
What additional potential term is needed for a breathing sphere?
Because the radius of the sphere changes with time, d(phi)/d(r) doesn’t = 0 but it = dR/dt. This can’t be implemented by changing the strength of the dipole but it can be by introducing A source term:
φ = -C(t) / r
with C / R² = dR/dt
What is ∂φ/∂t for a breathing sphere?
∂φ/∂t = (3 U C(t) cosθ) / (2 r²) - (1 / r) dC/dt
What is the general velocity vector u from ∇φ?
u = U î + A e_r + B e_θ
A = C / r² - U cosθ (R³ / r³)
B = U sinθ (R³ / (2 r³))
What is the key property of the stream function in 2D incompressible flow?
A stream function satisfies automatically the incompressibility condition.
Because of that (doing some math) ew can see It automatically satisfies continuity. If:
u = ∂ψ / ∂y
v = -∂ψ / ∂x
then ∂u/∂x + ∂v/∂y = 0.
What are the stream function relations in 2D polar coordinates?
r u_r = ∂ψ / ∂θ
u_θ = -∂ψ / ∂r
What are the relations in axisymmetric coordinates (r, z)?
r u_z = ∂ψ / ∂r
r u_r = -∂ψ / ∂z
What are the relations in spherical coordinates (r, θ) with no azimuthal dependence?
r² sinθ u_r = ∂ψ / ∂θ
r sinθ u_θ = -∂ψ / ∂r