Physics · Book 4 · Bachelor Year 2

University Physics — Year 2

University Physics — Year 2 · Bachelor Year 2

3Perfect Fluids: Euler and Bernoulli

Hold a sheet of paper by its edge and blow over its top: it lifts. Open the tap in the shower and the curtain leans in. A wing holds up three hundred tonnes because the air flows faster over its upper surface than under it. All three are the same statement: where a fluid moves faster, its pressure is lower. This chapter writes Newton’s second law for a fluid particle in the simplest model — the perfect fluid, which feels pressure but no friction — and draws from it Bernoulli’s theorem, the energy balance of a streamline, whose applications run from the flow meter in a pipe to the speed indicator of an aircraft.

3.1 The Euler equation

Proposition 3.1 (Pressure force on a fluid particle)

The resultant of the pressure forces exerted by the surrounding fluid on a particle of volume  ⁣dτ\dd\tau is

 ⁣dFP=gradP ⁣dτ:\dd\vect F_P = -\operatorname{\vect{grad}}P\,\dd\tau :

pressure acts as a volume force of density gradP-\operatorname{\vect{grad}}P, pushing from high toward low pressure.

Proof. On the box of Theorem 2.8, the faces at xx and x+ ⁣dxx + \dd x receive +P(x) ⁣dy ⁣dz+P(x)\dd y\dd z and P(x+ ⁣dx) ⁣dy ⁣dz-P(x + \dd x)\dd y\dd z along xx: net xP ⁣dx ⁣dy ⁣dz-\partial_xP\,\dd x\dd y\dd z; likewise for yy and zz.

Definition 3.2 (Perfect fluid)

A perfect fluid is one in which the only contact force between neighbouring particles is the pressure — normal to every surface, no tangential (viscous) stress. It is an idealization valid, as the next chapter explains, far from walls and at high Reynolds number: water in a pipe away from the wall, air around a wing outside the thin boundary layer, a wave on the sea.

Theorem 3.3 (Euler’s equation)

In a Galilean frame, a perfect fluid of density ρ\rho subject to gravity obeys, at every point,

ρ(vt+(vgrad)v)=gradP+ρg,\rho\Bigl(\frac{\partial\vect v}{\partial t} + (\vect v\cdot\operatorname{\vect{grad}}) \vect v\Bigr) = -\operatorname{\vect{grad}}P + \rho\vect g ,

to which any other volume force density fv\vect f_v (electric, inertial in a non-Galilean frame) is added on the right. At rest it reduces to the hydrostatic law gradP=ρg\operatorname{\vect{grad}}P = \rho\vect g of the Year 1 volume.

Proof. Newton’s second law for the particle of mass ρ ⁣dτ\rho\,\dd\tau: its acceleration is the material derivative (Theorem 2.4), the forces are the pressure resultant and the weight ρg ⁣dτ\rho\vect g\,\dd\tau; divide by  ⁣dτ\dd\tau.

Example 3.4 (A tank that accelerates)

Water in a tank carried by a truck accelerating at a\vect a is at rest in the truck’s frame; there, Euler with the inertial force ρa-\rho\vect a gives gradP=ρ(ga)\operatorname{\vect{grad}}P = \rho(\vect g - \vect a): the pressure grows along the "effective gravity" ga\vect g - \vect a, the free surface (an isobar) is perpendicular to it and tilts backward by the angle arctan(a/g)\arctan(a/g)1111{}^{\circ} for a=2m/s2a = 2\,\mathrm{m}/\mathrm{s}^{2}. In a bucket spinning at Ω\Omega, the centrifugal force ρΩ2rer\rho\Omega^2r\,\vect e_r gives P=P0+12ρΩ2r2ρgzP = P_0 + \tfrac12\rho\Omega^2r^2 - \rho gz and the free surface is the paraboloid z=Ω2r2/2gz = \Omega^2r^2/2g.

Left: the pressure forces on the faces of a fluid box do not cancel when P varies — their resultant is - gradP per unit volume. Middle and right: two fluids at rest in an accelerated frame; the free surface is everywhere perpendicular to the effective gravity.
Left: the pressure forces on the faces of a fluid box do not cancel when PP varies — their resultant is gradP-\operatorname{\vect{grad}}P per unit volume. Middle and right: two fluids at rest in an accelerated frame; the free surface is everywhere perpendicular to the effective gravity.

3.2 Bernoulli’s theorem

Theorem 3.5 (Bernoulli)

For a perfect, incompressible fluid of uniform density in steady flow, in a Galilean frame with uniform gravity, the quantity

P+12ρv2+ρgzP + \tfrac12\rho v^2 + \rho gz

is constant along each streamline. If the flow is moreover irrotational, it is the same constant throughout the fluid. The term 12ρv2\tfrac12\rho v^2 is the dynamic pressure; P+12ρv2P + \tfrac12\rho v^2 is the stagnation pressure, the pressure the fluid would reach if brought to rest along its streamline.

Proof. Steady Euler with (vgrad)v=grad(v2/2)+ωv(\vect v\cdot\operatorname{\vect{grad}})\vect v = \operatorname{\vect{grad}}(v^2/2) + \vect\omega\wedge\vect v and ρg=grad(ρgz)\rho\vect g = -\operatorname{\vect{grad}}(\rho gz), ρ\rho uniform:

grad(P+12ρv2+ρgz)=ρωv.\operatorname{\vect{grad}}\bigl(P + \tfrac12\rho v^2 + \rho gz\bigr) = -\rho\, \vect\omega\wedge\vect v .

The right side is perpendicular to v\vect v, so the gradient of the Bernoulli quantity has no component along the streamline: the quantity is constant along it. If ω=0\vect\omega = \vect 0 the gradient vanishes everywhere.

Remark 3.6 (What Bernoulli says and does not say)

Divided by ρ\rho, the theorem reads: the mechanical energy per unit mass, v2/2+gzv^2/2 + gz, plus P/ρP/\rho is conserved along a particle’s path. The pressure term is the work done on the particle by the pressure of the fluid behind it, minus the work it does on the fluid ahead: the energy theorem for a particle pushed through a pressure field without friction. Four conditions: perfect fluid (no viscous loss), steady, incompressible, and along a streamline. Comparing two points on different streamlines is allowed only in irrotational flow. It does not say "fast air sucks": it says that a particle that has been accelerated (by a pressure drop) is now at lower pressure — the cause is the pressure field, the speed is the effect.

Remark 3.7 (Compressible fluids)

For a gas the density varies, but if the flow is steady, perfect and isentropic the same proof gives the conservation of h+v2/2+gzh + v^2/2 + gz along a streamline, where hh is the enthalpy per unit mass (h=cPTh = c_PT for a perfect gas): the form used for nozzles and turbines in Chapter 27. At speeds well below the speed of sound (v100m/sv \lesssim 100\,\mathrm{m}/\mathrm{s} in air) the density changes by less than 5%5\% and the incompressible theorem is accurate.

3.3 Applications

Proposition 3.8 (The Venturi meter)

In a horizontal pipe narrowing from section S1S_1 to S2<S1S_2 < S_1, the speed rises (v2=v1S1/S2v_2 = v_1S_1/S_2, mass conservation) and the pressure drops:

P1P2=12ρ(v22v12)=12ρv12(S12S221),DV=S1v1=S1S22(P1P2)ρ(S12S22).P_1 - P_2 = \tfrac12\rho(v_2^2 - v_1^2) = \tfrac12\rho v_1^2\Bigl(\frac{S_1^2}{S_2^2} - 1\Bigr) , \qquad D_V = S_1v_1 = S_1S_2\sqrt{\frac{2(P_1 - P_2)}{\rho(S_1^2 - S_2^2)}} .

Measuring the pressure difference with a manometer gives the flow rate: a Venturi meter. The same effect drives a carburettor, a paint spray, a Bunsen burner’s air intake and the "suction" of a passing train.

Proof. Bernoulli along a central streamline at constant height, with v2=v1S1/S2v_2 = v_1S_1/S_2; solve for v1v_1.

Proposition 3.9 (The Pitot tube)

A tube facing the flow, closed at the far end, brings the fluid to rest at its mouth (a stagnation point); a second opening on the side, parallel to the flow, reads the static pressure PP. The difference is the dynamic pressure:

PstagP=12ρv2,v=2(PstagP)/ρ.P_{\text{stag}} - P = \tfrac12\rho v^2 , \qquad v = \sqrt{2(P_{\text{stag}} - P)/\rho} .

Every aircraft measures its airspeed this way.

Proof. Bernoulli along the streamline that ends at the stagnation point, where v=0v = 0; the side holes do not disturb the flow, which passes at the undisturbed vv and PP.

Proposition 3.10 (Torricelli’s formula)

A large open tank drains through a small hole at depth hh below the free surface; the jet leaves at

v=2gh,v = \sqrt{2gh} ,

the speed of free fall from the surface. The flow rate is DVαs2ghD_V \approx \alpha s\sqrt{2gh} with ss the hole’s area and α0.6\alpha \approx 0.6 the contraction coefficient of a sharp-edged orifice (the streamlines keep converging past the hole).

Proof. Bernoulli from the free surface (at rest, since the tank is large: vsurf=vs/Svv_{\text{surf}} = v\,s/S \ll v; pressure P0P_0) to the jet (pressure P0P_0 just outside the hole): P0+ρgh=P0+12ρv2P_0 + \rho gh = P_0 + \tfrac12\rho v^2. The flow is quasi-steady: hh varies slowly.

Three applications of Bernoulli’s theorem. Left: the Venturi meter — the manometer reads the pressure drop at the throat, hence the flow rate. Middle: the Pitot tube — the stagnation pressure at the mouth exceeds the static pressure at the side holes by the dynamic pressure. Right: Torricelli’s efflux at the free-fall speed.
Three applications of Bernoulli’s theorem. Left: the Venturi meter — the manometer reads the pressure drop at the throat, hence the flow rate. Middle: the Pitot tube — the stagnation pressure at the mouth exceeds the static pressure at the side holes by the dynamic pressure. Right: Torricelli’s efflux at the free-fall speed.

Example 3.11 (Numbers)

A Venturi of 5cm5\,\mathrm{cm} narrowing to 2.5cm2.5\,\mathrm{cm} on a water pipe, with Δh=20cm\Delta h = 20\,\mathrm{cm} of water (2.0kPa2.0\,\mathrm{kPa}): v1=2×2000/(1000×15)=0.52m/sv_1 = \sqrt{2 \times 2000/ (1000 \times 15)} = 0.52\,\mathrm{m}/\mathrm{s}, DV=1.0L/sD_V = 1.0\,\mathrm{L}/\mathrm{s}. An airliner at 11km11\,\mathrm{km} (ρ=0.36kg/m3\rho = 0.36\,\mathrm{kg}/\mathrm{m}^{3}) at 250m/s250\,\mathrm{m}/\mathrm{s}: dynamic pressure 11kPa11\,\mathrm{kPa}, 11%11\% of the ambient pressure — the Pitot tube still works, with a compressibility correction. A water tower 40m40\,\mathrm{m} above the taps: 4bar4\,\mathrm{bar} when closed, a jet at 28m/s28\,\mathrm{m}/\mathrm{s} if opened wide (in practice far less: the pipes are not perfect).

Proposition 3.12 (Lift on a wing)

In the flow around a wing the air passes faster over the upper surface than under the lower one; the pressure is therefore lower above than below, and the resultant is the lift FL=12ρv2SCLF_L = \tfrac12\rho v^2SC_L (SS the wing area, CL0.3C_L \approx 0.31.51.5 the lift coefficient, depending on the profile and the angle of attack). The speed difference is equivalent to a circulation Γ\Gamma of the velocity around the profile, and the lift per unit span is FL=ρvΓF_L' = \rho v\Gamma (Kutta–Joukowski, admitted). A spinning ball drags air round with it and is lifted sideways the same way: the Magnus effect of a sliced tennis ball or a curving free kick.

Proof. Bernoulli on the streamlines just above and below, which start from the same upstream conditions: PlowPup=12ρ(vup2vlow2)P_{\text{low}} - P_{\text{up}} = \tfrac12\rho (v_{\text{up}}^2 - v_{\text{low}}^2); integrate over the chord. Why the upper flow is faster — the sharp trailing edge forces the rear stagnation point there and fixes the circulation (the Kutta condition) — is beyond the perfect-fluid model alone; it needs the boundary layer of the next chapter.

Left: streamlines around a wing — crowded and fast above, slow below; the pressure difference is the lift. Right: a liquid column of total length L oscillating in a U-tube, the simplest unsteady application of Euler’s equation.
Left: streamlines around a wing — crowded and fast above, slow below; the pressure difference is the lift. Right: a liquid column of total length LL oscillating in a U-tube, the simplest unsteady application of Euler’s equation.

Proposition 3.13 (An unsteady flow: the U-tube)

A liquid column of total length LL fills a U-tube of uniform section; displaced by zz from equilibrium, it oscillates with

z¨+2gLz=0,T=2πL2g,\ddot z + \frac{2g}{L}\,z = 0 , \qquad T = 2\pi\sqrt{\frac{L}{2g}} ,

like a pendulum of length L/2L/2. More generally, for an unsteady but irrotational flow with potential φ\varphi, Euler integrates to ρtφ+P+12ρv2+ρgz=C(t)\rho\,\partial_t\varphi + P + \tfrac12\rho v^2 + \rho gz = C(t), the same constant throughout the fluid (unsteady Bernoulli).

Proof. The speed v=z˙v = \dot z is uniform along the tube (incompressible, uniform section). Project Euler on the tube’s axis and integrate along the column from one free surface to the other: the pressure terms cancel (P0P_0 at both ends), ρtv ⁣ds=ρLz¨\int\rho\,\partial_tv\,\dd s = \rho L\ddot z, the convective term ρΔ(v2/2)\rho\,\Delta(v^2/2) vanishes (same speed at both ends), and the gravity term gives ρg2z\rho g\cdot2z. Hence ρLz¨=2ρgz\rho L\ddot z = -2\rho gz. The general statement follows from tv=gradtφ\partial_t\vect v = \operatorname{\vect{grad}} \partial_t\varphi for v=gradφ\vect v = \operatorname{\vect{grad}}\varphi.

Example 3.14 (Starting a pipe)

A horizontal pipe of length \ell leads from a reservoir of constant head hh to an open end; the valve is opened at t=0t = 0. With vv uniform along the pipe, Euler integrated from the reservoir surface to the outlet gives  ⁣dv/ ⁣dt=gh12v2\ell\,\dd v/\dd t = gh - \tfrac12v^2, whose solution is v=Vtanh(Vt/2)v = V\tanh(Vt/2\ell) with V=2ghV = \sqrt{2gh}: the flow reaches Torricelli’s speed with the time constant 2/V2\ell/V13s13\,\mathrm{s} for a 400m400\,\mathrm{m} penstock under 200m200\,\mathrm{m} of head.

Method 3.15 (Using Bernoulli)

(1) Check the four conditions; decide whether the flow is irrotational (uniform upstream flow around an obstacle: yes; flow in a pipe with a velocity profile: no — stay on one streamline). (2) Choose two points on a streamline where as many quantities as possible are known: a free surface (P=P0P = P_0, v0v \approx 0 if the section is large), a jet in the open air (P=P0P = P_0), a stagnation point (v=0v = 0). (3) Add mass conservation vS=vS = const to relate the speeds. (4) For unsteady flows, integrate Euler along the line instead.

3.4 Exercises

Exercise 3.1

Water flows in a horizontal pipe of diameter 8cm8\,\mathrm{cm} at 1.5m/s1.5\,\mathrm{m}/\mathrm{s} and pressure 3.0bar3.0\,\mathrm{bar}. It passes into a 4cm4\,\mathrm{cm} section: speed and pressure there; into a 2cm2\,\mathrm{cm} section: pressure — what happens if it would come out negative?

Solution

Solution of Exercise 3.1.

v2=1.5×4=6.0m/sv_2 = 1.5 \times 4 = 6.0\,\mathrm{m}/\mathrm{s}, P2=3.0×105500(362.25)=2.83barP_2 = 3.0 \times 10^5 - 500(36 - 2.25) = 2.83\,\mathrm{bar}. At 2cm2\,\mathrm{cm}: v=24m/sv = 24\,\mathrm{m}/\mathrm{s}, P=3.0×105500(5762.25)=0.13barP = 3.0 \times 10^5 - 500 (576 - 2.25) = 0.13\,\mathrm{bar} — close to the vapour pressure. A negative result means the assumed flow rate is impossible: the water cavitates and the flow is throttled.

Exercise 3.2

The Pitot tube of an aircraft at 5km5\,\mathrm{km} (ρ=0.74kg/m3\rho = 0.74\,\mathrm{kg}/\mathrm{m}^{3}) reads a dynamic pressure of 15kPa15\,\mathrm{kPa}. True airspeed. The airspeed indicator is calibrated for sea-level density (1.22kg/m31.22\,\mathrm{kg}/\mathrm{m}^{3}): what "indicated airspeed" does it show, and why do pilots find the difference useful rather than annoying?

Solution

Solution of Exercise 3.2.

v=2×15000/0.74=201m/sv = \sqrt{2 \times 15000/0.74} = 201\,\mathrm{m}/\mathrm{s}; indicated 2×15000/1.22=157m/s\sqrt{2 \times 15000/ 1.22} = 157\,\mathrm{m}/\mathrm{s}. The indicated airspeed measures the dynamic pressure, which is what the wing feels: the stall speed is a fixed indicated speed at any altitude.

Exercise 3.3

A tank holds water 3.0m3.0\,\mathrm{m} deep; a 1.0cm21.0\,\mathrm{cm}^{2} hole is pierced 1.0m1.0\,\mathrm{m} above the floor. Exit speed; flow rate (contraction 0.60.6); where does the jet hit the floor? At what depth should a second hole be pierced to reach the same point?

Solution

Solution of Exercise 3.3.

Depth 2.0m2.0\,\mathrm{m}: v=2g×2=6.3m/sv = \sqrt{2g \times 2} = 6.3\,\mathrm{m}/\mathrm{s}; DV=0.6×104×6.3=0.38L/sD_V = 0.6 \times 10^{-4} \times 6.3 = 0.38\,\mathrm{L}/\mathrm{s}; fall time 2/g=0.45s\sqrt{2/g} = 0.45\,\mathrm{s}, range 2.8m2.8\,\mathrm{m}. Range =2h(Hh)= 2\sqrt{h(H - h)} is symmetric in hHhh \leftrightarrow H - h: a hole at depth 1.0m1.0\,\mathrm{m} (2m2\,\mathrm{m} above the floor) hits the same point.

Exercise 3.4

A wind of 30m/s30\,\mathrm{m}/\mathrm{s} blows over a flat roof of 100m2100\,\mathrm{m}^{2}; the air under the roof is still at atmospheric pressure (ρ=1.2kg/m3\rho = 1.2\,\mathrm{kg}/\mathrm{m}^{3}). Pressure difference and net force on the roof; compare with the weight of the roof (50kg/m250\,\mathrm{kg}/\mathrm{m}^{2}). Which way is it pushed?

Solution

Solution of Exercise 3.4.

ΔP=12×1.2×900=540Pa\Delta P = \tfrac12 \times 1.2 \times 900 = 540\,\mathrm{Pa}, outside pressure lower: net force 54kN54\,\mathrm{kN} upward; the roof weighs 49kN49\,\mathrm{kN}: it lifts off. (Real roofs fail at their edges first, where the flow separates.)

Exercise 3.5 ★★

A closed rectangular tank 2.0m2.0\,\mathrm{m} long, half full of water, sits on a truck. (a) Accelerating at 3.0m/s23.0\,\mathrm{m}/\mathrm{s}^{2}: angle of the free surface, and the difference of water height between the rear and the front walls. (b) Pressure difference between the two bottom corners. (c) Braking at 6m/s26\,\mathrm{m}/\mathrm{s}^{2} — does the water reach the lid 0.8m0.8\,\mathrm{m} above the bottom? (d) Same truck going round a bend of radius 40m40\,\mathrm{m} at 15m/s15\,\mathrm{m}/\mathrm{s}: tilt of the surface.

Solution

Solution of Exercise 3.5.

(a) tanθ=3/9.81\tan\theta = 3/9.81, θ=17\theta = 17{}^{\circ}; 2×0.306=0.61m2 \times 0.306 = 0.61\,\mathrm{m} (higher at the rear). (b) ΔP=ρaL=6.0kPa\Delta P = \rho aL = 6.0\,\mathrm{kPa}. (c) tanθ=0.61\tan\theta = 0.61, difference 1.22m1.22\,\mathrm{m}: the front rises 0.61m0.61\,\mathrm{m} above the mean 0.40m0.40\,\mathrm{m}: 1.01m1.01\,\mathrm{m} >> 0.8m0.8\,\mathrm{m}, it hits the lid. (d) a=v2/R=5.6m/s2a = v^2/R = 5.6\,\mathrm{m}/\mathrm{s}^{2}: θ=30\theta = 30{}^{\circ}, outward side higher.

Exercise 3.6 ★★

A bucket of radius 15cm15\,\mathrm{cm} containing water 20cm20\,\mathrm{cm} deep is spun about its axis at 2.0turns/s2.0\,\mathrm{turns}/\mathrm{s}. (a) Shape and equation of the free surface. (b) Height difference between rim and centre. (c) Volume being conserved, height of the water at the centre and at the rim. (d) At what rotation rate does the bottom centre dry out? (e) Why does the same paraboloid make a perfect telescope mirror (a spinning pool of mercury)?

Solution

Solution of Exercise 3.6.

(a) Paraboloid z=z0+Ω2r2/2gz = z_0 + \Omega^2r^2/2g, Ω=4π=12.6rad/s\Omega = 4\pi = 12.6\,\mathrm{rad}/\mathrm{s}. (b) Ω2R2/2g=158×0.0225/19.6=0.18m\Omega^2R^2/2g = 158 \times 0.0225/19.6 = 0.18\,\mathrm{m}. (c) The mean height of a paraboloid over the disk is halfway: centre 0.200.09=0.11m0.20 - 0.09 = 0.11\,\mathrm{m}, rim 0.29m0.29\,\mathrm{m}. (d) Centre dry when Ω2R2/4g=h0\Omega^2R^2/4g = h_0: Ω=4gh0/R=18.7rad/s=3.0\Omega = \sqrt{4gh_0}/R = 18.7\,\mathrm{rad}/\mathrm{s} = 3.0 turns per second. (e) A paraboloid focuses parallel rays to one point, at f=g/2Ω2f = g/2\Omega^2; liquid-mirror telescopes spin mercury.

Exercise 3.7 ★★

Siphon. A tube carries water from a tank over a crest 2.0m2.0\,\mathrm{m} above the free surface to an outlet 3.0m3.0\,\mathrm{m} below it. (a) Exit speed and, for a 2cm2\,\mathrm{cm} tube, flow rate. (b) Pressure at the crest. (c) Maximum height of the crest for the siphon to work (the water’s vapour pressure, 2.3kPa2.3\,\mathrm{kPa}, must not be reached). (d) Why does the siphon not work with the tube full of air?

Solution

Solution of Exercise 3.7.

(a) v=2g×3=7.7m/sv = \sqrt{2g \times 3} = 7.7\,\mathrm{m}/\mathrm{s}; DV=π×104×7.7=2.4L/sD_V = \pi \times 10^{-4} \times 7.7 = 2.4\,\mathrm{L}/\mathrm{s}. (b) P=P0ρg(2)12ρv2=10019.629.4=51kPaP = P_0 - \rho g(2) - \tfrac12\rho v^2 = 100 - 19.6 - 29.4 = 51\,\mathrm{kPa}. (c) P0ρghc12ρv22.3kPaP_0 - \rho gh_c - \tfrac12\rho v^2 \ge 2.3\,\mathrm{kPa}: hc7.0mh_c \le 7.0\,\mathrm{m}. (d) Air is compressible and light: no continuous liquid column to transmit the pressure, the water on both sides just stays.

Exercise 3.8 ★★

A light aircraft of 1000kg1000\,\mathrm{kg} cruises at 60m/s60\,\mathrm{m}/\mathrm{s} at sea level on a wing of 15m215\,\mathrm{m}^{2}. (a) Mean pressure difference between the two faces of the wing; lift coefficient. (b) If the speed under the wing is 58m/s58\,\mathrm{m}/\mathrm{s}, what is it over the wing (take the same upstream conditions)? (c) Circulation around the profile from the Kutta–Joukowski formula, for a span of 10m10\,\mathrm{m}. (d) Stalling speed if CLC_L cannot exceed 1.41.4.

Solution

Solution of Exercise 3.8.

(a) ΔP=mg/S=654Pa\Delta P = mg/S = 654\,\mathrm{Pa}; 12ρv2=2.2kPa\tfrac12\rho v^2 = 2.2\,\mathrm{kPa}, CL=0.30C_L = 0.30. (b) vup2=582+2×654/1.22v_{\text{up}}^2 = 58^2 + 2 \times 654/1.22: 66.6m/s66.6\,\mathrm{m}/\mathrm{s}. (c) FL=981N/m=ρvΓF_L' = 981\,\mathrm{N}/\mathrm{m} = \rho v\Gamma: Γ=13.4m2/s\Gamma = 13.4\,\mathrm{m}^{2}/\mathrm{s}. (d) v=2mg/ρSCL=19620/25.6=28m/sv = \sqrt{2mg/ \rho SC_L} = \sqrt{19620/25.6} = 28\,\mathrm{m}/\mathrm{s}.

Exercise 3.9 ★★

Stenosis. Blood (ρ=1060kg/m3\rho = 1060\,\mathrm{kg}/\mathrm{m}^{3}) flows at 0.50m/s0.50\,\mathrm{m}/\mathrm{s} in an artery of section 0.50cm20.50\,\mathrm{cm}^{2} at 13kPa13\,\mathrm{kPa} above atmospheric pressure. A plaque narrows it to 0.10cm20.10\,\mathrm{cm}^{2}. (a) Speed and pressure in the stenosis. (b) The tissue outside the artery is at about 1kPa1\,\mathrm{kPa}: can the artery collapse? (c) If it narrows, the speed rises further: explain the runaway and why such a narrowing can flutter.

Solution

Solution of Exercise 3.9.

(a) v2=2.5m/sv_2 = 2.5\,\mathrm{m}/\mathrm{s}; ΔP=12×1060×(6.250.25)=3.2kPa\Delta P = \tfrac12 \times 1060 \times (6.25 - 0.25) = 3.2\,\mathrm{kPa}, P2=9.8kPaP_2 = 9.8\,\mathrm{kPa}. (b) Still above 1kPa1\,\mathrm{kPa}: no. (c) At 0.05cm20.05\,\mathrm{cm}^{2}, v=5m/sv = 5\,\mathrm{m}/\mathrm{s} and ΔP=13kPa\Delta P = 13\,\mathrm{kPa}: P20P_2 \approx 0, below the tissue pressure — the wall collapses, the flow stops, the pressure recovers, it reopens: a flutter (the murmur a physician hears).

Exercise 3.10 ★★★

Stagnation temperature. For a perfect gas in steady isentropic flow, cPT+v2/2c_PT + v^2/2 is conserved along a streamline. (a) Show that the air brought to rest at the nose of an aircraft reaches T0=T(1+γ12M2)T_0 = T(1 + \tfrac{\gamma - 1}{2}M^2), with M=v/cM = v/c the Mach number and c=γRT/Mmolc = \sqrt{\gamma RT/M_{\text{mol}}} the speed of sound. (b) Nose temperature of an airliner at M=0.85M = 0.85 in air at 220K220\,\mathrm{K}; of a supersonic aircraft at M=2M = 2; of a re-entry capsule at M=25M = 25 (is the formula still meaningful?). (c) Show that the incompressible Pitot formula overestimates the speed at M=0.85M = 0.85, and by roughly how much (expand P0/P=(T0/T)γ/(γ1)P_0/P = (T_0/T)^{\gamma/(\gamma - 1)} to second order in M2M^2).

Solution

Solution of Exercise 3.10.

(a) cPT0=cPT+v2/2c_PT_0 = c_PT + v^2/2 with cP=γR/(γ1)Mmolc_P = \gamma R/(\gamma - 1)M_{\text{mol}} and c2=γRT/Mmolc^2 = \gamma RT/M_{\text{mol}}: v2/2cPT=12(γ1)M2v^2/2c_PT = \tfrac12(\gamma - 1)M^2. (b) M=0.85M = 0.85: T0=220×1.145=252KT_0 = 220 \times 1.145 = 252\,\mathrm{K}; M=2M = 2: 220×1.8=396K220 \times 1.8 = 396\,\mathrm{K}; M=25M = 25: 220×126=28000K220 \times 126 = 28\,000\,\mathrm{K} — meaningless: the air dissociates and ionizes, cPc_P is not constant (real stagnation temperatures are several thousand kelvin). (c) P0/P=(1+γ12M2)γ/(γ1)1+γ2M2+γ8M4P_0/P = (1 + \tfrac{\gamma - 1}2M^2)^{\gamma/(\gamma - 1)} \approx 1 + \tfrac{\gamma}2M^2 + \tfrac{\gamma}8M^4, and γPM2=ρv2\gamma PM^2 = \rho v^2: P0P=12ρv2(1+M2/4)P_0 - P = \tfrac12\rho v^2(1 + M^2/4). Reading vv from 2(P0P)/ρ\sqrt{2(P_0 - P)/\rho} overestimates it by 1+M2/419%\sqrt{1 + M^2/4} - 1 \approx 9\% at M=0.85M = 0.85.

Exercise 3.11 ★★★

Starting transient. A pipe of length =50m\ell = 50\,\mathrm{m} and uniform section leads from a large reservoir (head h=5.0mh = 5.0\,\mathrm{m} above the outlet) to a valve at the open end. The valve is opened at t=0t = 0. (a) Integrate Euler along the pipe to get  ⁣dv/ ⁣dt=ghv2/2\ell\,\dd v/\dd t = gh - v^2/2. (b) Solve it: v=Vtanh(Vt/2)v = V\tanh(Vt/2\ell) with V=2ghV = \sqrt{2gh}. (c) Time to reach 90%90\% of the final speed. (d) The valve is now shut abruptly in 0.5s0.5\,\mathrm{s} from full flow: estimate the mean deceleration and the over-pressure at the valve from ρ ⁣dv/ ⁣dt\rho\ell\,\dd v/\dd t — and why a real closure produces far more (next chapters).

Solution

Solution of Exercise 3.11.

(a) From the surface (v0v \approx 0, P0P_0, height hh) to the outlet (vv, P0P_0, height 00), with tv ⁣ds= ⁣dv/ ⁣dt\int\partial_tv\,\dd s = \ell\,\dd v/\dd t. (b)  ⁣dv/(V2v2)= ⁣dt/2\dd v/(V^2 - v^2) = \dd t/2\ell, V2=2ghV^2 = 2gh: artanh(v/V)=Vt/2\operatorname{artanh}(v/V) = Vt/2\ell. (c) V=9.9m/sV = 9.9\,\mathrm{m}/\mathrm{s}; tanhx=0.9\tanh x = 0.9 at x=1.47x = 1.47: t=2x/V=15st = 2\ell x/V = 15\,\mathrm{s}. (d)  ⁣dv/ ⁣dt20m/s2\dd v/\dd t \approx -20\,\mathrm{m}/\mathrm{s}^{2}: ΔP=ρ×20=9.9bar\Delta P = \rho\ell \times 20 = 9.9\,\mathrm{bar}. Water is slightly compressible: a fast closure launches a pressure wave, ΔP=ρcΔv140bar\Delta P = \rho c\Delta v \approx 140\,\mathrm{bar}.

Exercise 3.12 ★★★

The free surface of a vortex. Water rotates as the point vortex of Chapter 2, vθ=Γ/2πrv_\theta = \Gamma/2\pi r, irrotational, with a free surface at z=0z = 0 far away. (a) Why may Bernoulli be applied between any two points? (b) Shape of the free surface z(r)z(r). (c) Inside a Rankine core (r<ar < a, vθ=Ωrv_\theta = \Omega r, rotational) use instead Euler in the rotating frame or directly: show z=z(a)+Ω2(r2a2)/2gz = z(a) + \Omega^2(r^2 - a^2)/2g. (d) Total depth of the funnel for a bathtub vortex with Γ=0.03m2/s\Gamma = 0.03\,\mathrm{m}^{2}/\mathrm{s} and a=5mma = 5\,\mathrm{mm}; for a tornado (Γ=3×104m2/s\Gamma = 3 \times 10^{4}\,\mathrm{m}^{2}/\mathrm{s}, a=60ma = 60\,\mathrm{m}, in air: express the result as a pressure drop at the centre instead).

Solution

Solution of Exercise 3.12.

(a) Steady, perfect, incompressible and irrotational: one constant for the whole flow. (b) On the surface P=P0P = P_0: 12ρv2+ρgz=0\tfrac12\rho v^2 + \rho gz = 0, z=Γ2/8π2gr2z = -\Gamma^2/8\pi^2gr^2. (c) Radial Euler: rP=ρΩ2r\partial_rP = \rho\Omega^2r, vertical hydrostatics: the surface satisfies z(r)z(a)=Ω2(r2a2)/2gz(r) - z(a) = \Omega^2(r^2 - a^2)/2g. (d) Bath: Ω=Γ/2πa2=191rad/s\Omega = \Gamma/2\pi a^2 = 191\,\mathrm{rad}/\mathrm{s}; z(a)=Ω2a2/2g=4.7cmz(a) = -\Omega^2a^2/ 2g = -4.7\,\mathrm{cm}, and the core adds another 4.7cm4.7\,\mathrm{cm}: 9.3cm9.3\,\mathrm{cm} deep. Tornado: ΔP=12ρvmax2\Delta P = \tfrac12\rho v_{\max}^2 outside plus the same inside: ρvmax2=1.2×6400=7.7kPa\rho v_{\max}^2 = 1.2 \times 6400 = 7.7\,\mathrm{kPa} below ambient at the centre.

Two penstocks carry the water of a mountain reservoir down to a turbine house: a head of two hundred metres, which Bernoulli’s theorem turns into a jet at sixty metres per second.
Two penstocks carry the water of a mountain reservoir down to a turbine house: a head of two hundred metres, which Bernoulli’s theorem turns into a jet at sixty metres per second.

3.5 Problem: The dam, the penstock and the turbine

Problem 3.1

Weekend problem — a hydroelectric plant from the reservoir to the jet: pressures, speeds, powers, losses and the water hammer

A reservoir holds water 150m150\,\mathrm{m} deep behind a dam; its free surface is H=200mH = 200\,\mathrm{m} above the nozzles of a turbine. A penstock (a steel pipe) of diameter D=3.0mD = 3.0\,\mathrm{m} and length =400m\ell = 400\,\mathrm{m} carries the design flow DV=60m3/sD_V = 60\,\mathrm{m}^{3}/\mathrm{s} down to the turbine house, where a nozzle turns it into a free jet at atmospheric pressure P0=1.0barP_0 = 1.0\,\mathrm{bar} which strikes the buckets of a Pelton wheel. ρ=1000kg/m3\rho = 1000\,\mathrm{kg}/\mathrm{m}^{3}, g=9.81m/s2g = 9.81\,\mathrm{m}/\mathrm{s}^{2}; the fluid is perfect unless stated otherwise.

Part I — At rest and at design flow.

  1. Pressure at the base of the dam, and the force on a 1m1\,\mathrm{m}-wide vertical strip of the dam from top to bottom.
  2. With the turbine valves closed, pressure in the penstock at the turbine house.
  3. Speed in the penstock at design flow; dynamic pressure there; pressure at the turbine house end of the penstock (before the nozzle), by Bernoulli from the reservoir surface.
  4. Speed of the free jet; section and diameter of the nozzle.
  5. Kinetic power carried by the jet; show it equals ρgDVH\rho gD_VH and compute it.
  6. Mass and kinetic energy of the water contained in the penstock at design flow; transit time of a particle down the pipe.
  7. Show that the head HH is shared, at design flow, between the pressure at the bottom of the penstock and the kinetic energy of the water, and that the nozzle converts the first into the second: what is the pressure just after the nozzle?
  8. A perfect fluid has no head loss, a real one does: the loss in a pipe is ΔP=λ(/D)12ρv2\Delta P = \lambda(\ell/D)\,\tfrac12\rho v^2 with λ0.015\lambda \approx 0.015 for smooth steel. Head loss in metres of water, and the fraction of the power lost.
  9. An engineer proposes a 2m2\,\mathrm{m} penstock to save steel. Redo question 7; comment.

Part II — Measuring the flow. A Venturi is built into the penstock, with a throat of 2.0m2.0\,\mathrm{m}.

  1. Speed at the throat and pressure drop between the pipe and the throat at design flow.
  2. The drop is read on a mercury manometer (ρHg=13600kg/m3\rho_{\text{Hg}} = 13\,600\,\mathrm{kg}/\mathrm{m}^{3}): height difference.
  3. Show that the flow rate is proportional to the square root of the manometer reading, and give the reading at half the design flow.
  4. Why must the pressure taps be flush with the wall and not protrude into the flow?
  5. A section of the pipe runs, for topographic reasons, over a crest 6m6\,\mathrm{m} above the reservoir surface. Pressure there at design flow; what happens, and what must the designer do?

Part III — Unsteady regimes. The reservoir has a surface area A=2.0km2A = 2.0\,\mathrm{km}^{2}.

  1. Rate at which the reservoir level falls at design flow, in centimetres per hour.
  2. The turbine is stopped and the nozzle (section from question 4) is left open to the air: the reservoir drains by gravity. Write the mass balance and find the level h(t)h(t) (quasi-steady Torricelli flow).
  3. Time for the level to fall by 10m10\,\mathrm{m}; compare with the time at constant design flow.
  4. Starting the plant: the penstock is full, the nozzle is opened at t=0t = 0. Taking the speed uniform along the penstock and neglecting the nozzle’s geometry, integrate Euler along the pipe to obtain  ⁣dv/ ⁣dt=gHv2/2\ell\,\dd v/\dd t = gH - v^2/2, solve it, and give the time constant.
  5. During this start-up, at the instant when vv is half its final value, what is the pressure at the bottom of the penstock? Explain the sign of the difference with the steady value.

Part IV — Closing the valve.

  1. The valve at the turbine is shut in τ=10s\tau = 10\,\mathrm{s}; assume the water in the penstock decelerates uniformly. Using Euler along the pipe, estimate the over-pressure at the valve, in bars.
  2. For a fast closure the water is not incompressible: a pressure wave travels up the pipe at c=1400m/sc = 1400\,\mathrm{m}/\mathrm{s} (the speed of sound in water in a steel pipe — Chapter 7), and the over-pressure is ΔP=ρcΔv\Delta P = \rho c\,\Delta v (Joukowsky). Value for a sudden stop from design flow; compare with the static pressure. How long does the wave take to reach the reservoir and back, and what does that say about the meaning of "fast"?
  3. To protect the penstock a surge tank — a vertical open shaft of section As=100m2A_s = 100\,\mathrm{m}^{2} — is connected where a horizontal tunnel of length L=2000mL = 2000\,\mathrm{m} and section A=7.0m2A = 7.0\,\mathrm{m}^{2} from the reservoir joins the penstock. After a sudden closure, the water in the tunnel keeps moving and the level zz in the shaft rises. Write mass conservation between the tunnel and the shaft.
  4. Integrate Euler along the tunnel (perfect fluid) to show that zz obeys z¨+gALAsz=0\ddot z + \dfrac{gA}{LA_s}z = 0; period of the oscillation.
  5. Maximum rise of the level in the shaft after a closure from design flow (energy argument: the kinetic energy of the tunnel water becomes potential energy in the shaft).
  6. Sum up: the five pressures met in this plant (static at the dam, static at the turbine, dynamic in the pipe, water hammer, surge) and the law that gives each.
Solution

Solution of Problem 3.1.

1. ρg×150=14.7bar\rho g \times 150 = 14.7\,\mathrm{bar} above atmospheric; 12ρgHd2×1m=1.1×108N\tfrac12\rho gH_d^2 \times 1\,\mathrm{m} = 1.1 \times 10^{8}\,\mathrm{N}.

2. ρgH=19.6bar\rho gH = 19.6\,\mathrm{bar} gauge, 20.6bar20.6\,\mathrm{bar} absolute.

3. v=60/7.07=8.5m/sv = 60/7.07 = 8.5\,\mathrm{m}/\mathrm{s}; 12ρv2=0.36bar\tfrac12\rho v^2 = 0.36\,\mathrm{bar}; P=P0+ρgH12ρv2=20.3barP = P_0 + \rho gH - \tfrac12\rho v^2 = 20.3\,\mathrm{bar} absolute.

4. vj=2gH=62.6m/sv_j = \sqrt{2gH} = 62.6\,\mathrm{m}/\mathrm{s}; s=60/62.6=0.96m2s = 60/62.6 = 0.96\,\mathrm{m}^{2}, d=1.1md = 1.1\,\mathrm{m}.

5. 12ρDVvj2=12ρDV(2gH)=ρgDVH=118MW\tfrac12\rho D_Vv_j^2 = \tfrac12\rho D_V(2gH) = \rho gD_VH = 118\,\mathrm{MW}.

6. m=ρS=2.8×106kgm = \rho S\ell = 2.8 \times 10^{6}\,\mathrm{kg}, Ek=12mv2=1.0×108JE_k = \tfrac12mv^2 = 1.0 \times 10^{8}\,\mathrm{J}; transit /v=47s\ell/v = 47\,\mathrm{s}.

7. ρgH=(PP0)+12ρv2\rho gH = (P - P_0) + \tfrac12\rho v^2: 19.3bar19.3\,\mathrm{bar} of pressure and 0.36bar0.36\,\mathrm{bar} of kinetic energy; in the nozzle the pressure falls to P0P_0 while 12ρv2\tfrac12\rho v^2 rises to ρgH\rho gH: just after it, P=P0P = P_0.

8. Δh=λ(/D)v2/2g=0.015×133×3.67=7.3m\Delta h = \lambda(\ell/D)v^2/2g = 0.015 \times 133 \times 3.67 = 7.3\,\mathrm{m}, 3.7%3.7\% of the power.

9. v=19.1m/sv = 19.1\,\mathrm{m}/\mathrm{s}, v2/2g=18.6mv^2/2g = 18.6\,\mathrm{m}, Δh=0.015×200×18.6=56m\Delta h = 0.015 \times 200 \times 18.6 = 56\,\mathrm{m}: 28%28\% lost — the saving in steel is paid every second in energy.

10. vt=60/π=19.1m/sv_t = 60/\pi = 19.1\,\mathrm{m}/\mathrm{s}; ΔP=500(19.128.492)=146kPa\Delta P = 500(19.1^2 - 8.49^2) = 146\,\mathrm{kPa}.

11. ΔP=(ρHgρ)gΔh\Delta P = (\rho_{\text{Hg}} - \rho)g\,\Delta h: Δh=146000/(12600×9.81)=1.18m\Delta h = 146000/(12600 \times 9.81) = 1.18\,\mathrm{m}.

12. ΔPv2DV2\Delta P \propto v^2 \propto D_V^2: DVΔhD_V \propto \sqrt{\Delta h}; half the flow gives a quarter, 0.30m0.30\,\mathrm{m}.

13. A protruding tap faces or disturbs the flow and reads part of the dynamic pressure (a Pitot), not the static pressure.

14. P=P0ρg×612ρv2=1005936=5kPaP = P_0 - \rho g \times 6 - \tfrac12\rho v^2 = 100 - 59 - 36 = 5\,\mathrm{kPa}: near the vapour pressure, dissolved air comes out and the water may boil (cavitation), breaking the column. Lower the crest, or fit an air valve and a vacuum pump, or reduce the flow.

15. DV/A=60/2×106=3×105m/s=11cm/hD_V/A = 60/2 \times 10^6 = 3 \times 10^{-5}\,\mathrm{m}/\mathrm{s} = 11\,\mathrm{cm}/\mathrm{h}.

16. A ⁣dh/ ⁣dt=s2ghA\,\dd h/\dd t = -s\sqrt{2gh}: h=h0(s/A)g/2t\sqrt h = \sqrt{h_0} - (s/A)\sqrt{g/2}\,t.

17. Δt=(A/s)2/g(200190)=2.09×106×0.45×0.36=3.4×105s=3.9days\Delta t = (A/s)\sqrt{2/g}(\sqrt{200} - \sqrt{190}) = 2.09 \times 10^6 \times 0.45 \times 0.36 = 3.4 \times 10^{5}\,\mathrm{s} = 3.9\,\mathrm{days}; at constant design flow 10A/DV=3.3×105s10A/D_V = 3.3 \times 10^{5}\,\mathrm{s}: nearly the same, the nozzle having been sized for Torricelli’s flow at hHh \approx H.

18.  ⁣dv/ ⁣dt=gHv2/2\ell\,\dd v/\dd t = gH - v^2/2: v=Vtanh(Vt/2)v = V\tanh(Vt/2\ell), V=62.6m/sV = 62.6\,\mathrm{m}/\mathrm{s}, time constant 2/V=13s2\ell/V = 13\,\mathrm{s}.

19. At v=V/2v = V/2:  ⁣dv/ ⁣dt=(gHV2/8)/=3.7m/s2\dd v/\dd t = (gH - V^2/8)/\ell = 3.7\,\mathrm{m}/\mathrm{s}^{2}; P=P0+ρgH12ρv2ρ ⁣dv/ ⁣dt=1.0+19.64.914.7=1.0barP = P_0 + \rho gH - \tfrac12\rho v^2 - \rho\ell\,\dd v/\dd t = 1.0 + 19.6 - 4.9 - 14.7 = 1.0\,\mathrm{bar}: most of the head is busy accelerating the column, so the pressure at the bottom is far below its steady value.

20.  ⁣dv/ ⁣dt=8.49/10=0.85m/s2|\dd v/\dd t| = 8.49/10 = 0.85\,\mathrm{m}/\mathrm{s}^{2}: ΔP=ρ×0.85=3.4bar\Delta P = \rho\ell \times 0.85 = 3.4\,\mathrm{bar}.

21. ΔP=1000×1400×8.49=119bar\Delta P = 1000 \times 1400 \times 8.49 = 119\,\mathrm{bar}, six times the static pressure. The wave’s round trip is 2/c=0.57s2\ell/c = 0.57\,\mathrm{s}: a closure faster than that is "sudden" and gets the full Joukowsky over-pressure; slower closures get less.

22. Av=As ⁣dz/ ⁣dtAv = A_s\,\dd z/\dd t.

23. Euler along the tunnel, from the reservoir (pressure P0+ρg×P_0 + \rho g\timesdepth) to the foot of the shaft (pressure P0+ρg(depth+z)P_0 + \rho g (\text{depth} + z)): ρL ⁣dv/ ⁣dt=ρgz\rho L\,\dd v/\dd t = -\rho gz; with v=(As/A)z˙v = (A_s/A)\dot z: z¨+(gA/LAs)z=0\ddot z + (gA/LA_s)z = 0; T=2πLAs/gA=2π2000×100/68.7=340s5.7minT = 2\pi\sqrt{LA_s/gA} = 2\pi\sqrt{2000 \times 100/ 68.7} = 340\,\mathrm{s} \approx 5.7\,\mathrm{min}.

24. 12ρALv2=12ρgAszmax2\tfrac12\rho ALv^2 = \tfrac12\rho gA_sz_{\max}^2 with v=60/7=8.6m/sv = 60/7 = 8.6\,\mathrm{m}/\mathrm{s}: zmax=vAL/gAs=32mz_{\max} = v\sqrt{AL/gA_s} = 32\,\mathrm{m}.

25. Dam: hydrostatics, ρgh\rho gh. Turbine, valves closed: the same, ρgH\rho gH. Penstock in operation: Bernoulli, 12ρv2\tfrac12\rho v^2 taken from the static head. Water hammer: compressibility, ρcΔv\rho c\Delta v. Surge: unsteady Euler along the tunnel, an oscillation of period 2πLAs/gA2\pi\sqrt{LA_s/gA}.

Terms defined in this chapter

See all 393 terms in the glossary