Midterm Prep - Ch3 Flashcards

(23 cards)

1
Q

What is the definition of vorticity?

A

Vorticity is the curl of the velocity field: ω = ∇ × u. (Eq. 3.1)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

What physical quantity does vorticity represent?

A

Local rotation (angular velocity) of fluid elements. For a solid-body rotation with angular velocity Ω, the vorticity equals 2Ω (so vorticity is twice the rotation rate). (Eqs. 3.2–3.3)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Show the vorticity of a solid-body rotation u = Ω × r.

A

Use double cross product: ∇×(Ω × r) = Ω∇·r − Ω·∇r. Since ∇·r = 3 and ∇r = I, this gives ∇×u = 2Ω. (Derivation in text; Eq. 3.3).

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

State Euler’s equations for an incompressible fluid used in the lecture.

A

Momentum: Du/Dt = ∂u/∂t + u·∇u = −∇p/ρ + g.
Continuity (incompressible): ∇·u = 0. (Eqs. 3.4–3.5)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

What identity is used to rewrite u·∇u in the derivation?

A

u × (∇ × u) = ∇(u²/2) − u·∇u. (Eq. 3.6). This identity is used to rearrange Euler’s equation into a form that exposes the vorticity term

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Write the rearranged momentum equation that explicitly shows the vorticity term.

A

∂u/∂t + ∇(u²/2 + p/ρ + gz) = u × ω, where ω = ∇ × u. (Eq. 3.7). This separates a gradient term (potential-like) from the vorticity contribution.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

What is the vorticity-transport equation (final simplified form)?

A

Dω/Dt = ω·∇u. (Eq. 3.9). This is the evolution equation for vorticity in an incompressible inviscid flow.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Physical meaning of the term ω·∇u in Dω/Dt = ω·∇u?

A

It represents vortex stretching/tilting: velocity gradients aligned with vorticity change the magnitude/direction of ω. If ω aligns with a region of extension, its magnitude can increase.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

What does persistence of irrotationality mean (as stated in the lecture)?

A

If the fluid far upstream has ω = 0 and the flow is incompressible and inviscid, then Dω/Dt = 0 → ω remains zero along particle paths; therefore the flow stays irrotational. (Discussion after Eq. 3.9). Caveat: text notes the rigorous proof is subtler (analogy to y’ = y).

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

If ω = 0 everywhere, what simplification applies to the velocity field?

A

The velocity is a gradient of a scalar potential: u = ∇φ. (Eq. 3.10)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

What equation does the velocity potential φ satisfy for incompressible irrotational flow?

A

∇²φ = 0 (Laplace’s equation). (Eq. 3.11). Solving this with boundary conditions gives the velocity field.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

What is the Bernoulli-like relation for a potential (irrotational) flow (unsteady form)?

A

From (3.12)/(3.13): ∂φ/∂t + u²/2 + p/ρ + gz = f(t), where f(t) depends only on time (not on spatial coordinates). (Eq. 3.13)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

How does ∂φ/∂t + u²/2 + p/ρ + gz = f(t) (3.13) differ from the usual Bernoulli equation?

A

Differences: (i) (3.13) requires irrotational flow (ω = 0) but allows unsteady flows (∂φ/∂t may be nonzero). (ii) The constant f(t) is the same across all streamlines (because flow is irrotational), while classical Bernoulli (steady) gives constants that can vary between streamlines in rotational flows.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Typical boundary conditions for solving ∇²φ = 0 in aerodynamics

A

(a) Far away: velocity → constant uniform stream. (b) On solid objects at rest: normal velocity = 0 → n·∇φ = 0 at body surface. Also f(t) fixed by conditions at infinity.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

How do you get forces on a body once φ (and p) are known?

A

Compute pressure p from ∂φ/∂t + u²/2 + p/ρ + gz = f(t) (3.13), then integrate over the body surface: F = −∫ p n dA.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Under what practical conditions is the inviscid, incompressible, irrotational model a reasonable approximation?

A

When: (i) Reynolds number is large (viscous effects negligible except in thin boundary layers), (ii) free stream vorticity is zero, and (iii) flow is not separated (attached flow). Good for many full-size aircraft at moderate angles of attack. Not good for very small flyers (low Re) or strongly separated bluff-body flows.

17
Q

Why is the boundary layer important for the irrotational assumption?

A

Even when the outer flow is nearly irrotational, viscous boundary layers next to solid surfaces are rotational and can generate vorticity; separation creates large vortical regions that violate the irrotational model.

18
Q

Does Bernoulli’s equation apply to unsteady flows, viscous flows, compressible flows?

A

Steady Bernoulli (u²/2 + p/ρ + gz = const along a streamline) applies only for steady, inviscid flow (and incompressible unless modified). For unsteady flows, a time-dependent form like (3.13) applies for irrotational flows. Viscous flows generally violate Bernoulli; compressible flows require using energy & compressible relations (classical Bernoulli must be modified).

19
Q

Exercise 2: List differences between Bernoulli’s equation and equation (3.13).

A

Bernoulli (steady): constant along streamlines only, does not require irrotationality. Equation (3.13): needs irrotational flow (ω = 0), but allows unsteady flows and gives a spatially uniform quantity (equal for all streamlines) up to f(t).

20
Q

Exercise 3: How is vorticity related to local angular velocity?

A

For solid-body rotation with angular velocity Ω, ω = 2Ω. Thus vorticity is twice the local angular velocity vector.

21
Q

Exercise 4: What special properties do inviscid flows with uniform far upstream velocity enjoy?

A

Far-upstream uniform → ω = 0 initially. For incompressible inviscid flow this leads to persistence of irrotationality, allowing potential-flow formulation (u = ∇φ), Laplace’s equation, and a single Bernoulli-like relation valid across the domain (up to f(t)). Simplifies lift/drag computations.

22
Q

Exercise 5: Is the irrotational model applicable at modest Reynolds number? At high Re when flow separates?

A

At modest Re (low-to-moderate), viscous effects are more important — the irrotational model is less applicable. At high Re, the model can be good if flow remains attached; if the flow separates (creating vortices), the irrotational model fails

23
Q

Exercise 6: How is f(t) in (3.13) determined?

A

f(t) is set by boundary conditions (commonly conditions at infinity). The lecture notes state it is “normally determined from boundary conditions given at infinity.” In practice you pick the reference pressure/velocity at far field to fix f(t).