Fluid Mechanics and Heat Transfer: Flow Over a Flat Plate
Drag Coefficient and Shear Stress Calculations for Flat Plates
Flow Over a Flat Plate Parameters: * The ambient temperature is defined as T∞=10∘C. * The wall temperature is initially defined as Tw=10∘C. * The local drag coefficient (Cf,x) for laminar flow over a flat plate is given by the correlation: * Cf,x=0.664×Rex−1/2
The average drag coefficient (Cf,L) for the entire length of the plate is given by: * Cf,L=1.328×ReL−1/2
Shear Stress and Force Formulation: * The shear stress (τw) exerted on the fluid by the wall is calculated using the average drag coefficient: * τw=21×ρ×u2×Cf,L * Where u represents the free stream velocity. * Substituting the average drag coefficient formula into the shear stress equation yields: * τw=21×ρ×u2×1.328×ReL−1/2 * The total force (F) is the product of wall shear stress and the surface area: * Force=Stress×Area * Assuming a unit length for the width of the plate (W=1), the area is L×1. * The total force is derived as: * F=21×ρ×u2×1.328×ReL−1/2×L×1
Power Consumption and Velocity Relationships
Power Derivation: * Power is defined as the product of force and velocity: * Power=Force×Velocity * Substituting the force expression: * Power=21×ρ×u2×1.328×ReL−1/2×L×1×u * Recalling the definition of the Reynolds number (ReL=νu×L), the power expression becomes: * P=0.664×ρ×u3×(νu×L)−1/2×L * Simplifying the powers of velocity (u) and length (L): * P=0.664×ρ×u3×u−1/2×L−1/2×ν1/2×L * P=0.664×ρ×u5/2×ν1/2×L1/2
Proportionality: * From the derived formula, Power (P) is proportional to the kinematic viscosity (ν) raised to the power of one-half: * P∝ν1/2
Comparative Analysis of Temperature Conditions on Fluid Properties
Condition Changes (Question 1a): * Scenario: The wall temperature is increased to Tw=90∘C. * The film temperature (Tf) is calculated as the average of the wall temperature and the free stream temperature: * Tf=290+10=50∘C * The properties of water vary between the cold condition (10∘C) and the film condition (50∘C).
Viscosity Data: * Dynamic viscosity at 10∘C (μ10∘C): 0.013g/am.s * Dynamic viscosity at 50∘C (μ50∘C): 0.00548g/amis * Comparing the power requirements between the two states using the proportionality P∝μ1/2 (assuming constant density): * P10∘CP50∘C=(μ10∘Cμ50∘C)1/2 * P10∘CP50∘C=(0.0130.00548)1/2≈0.65
Heat Transfer Nuance and Power Savings Analysis
Power Savings (Question 1b): * The relative power at the higher temperature is 65% of the power at the lower temperature (Pf=0.65×Pc). * The power saving is calculated as: * Psaving=Pc−Pf=Pc−0.65×Pc=0.35×Pc * The literal expression for power saving is: * Psaving=0.35×0.664×ρ×νc1/2×u5/2×L1/2
Heating Power via Convection: * The convection correlation for the Nusselt number (Nu) is: * Nu=khˉ×L=0.664×ReL1/2×Pr1/3 * The average heat transfer coefficient (hˉ) is: * hˉ=0.664×Lk×(νu×L)1/2×Pr1/3 * The power required for heating is given by: * Power (heating)=hˉ×A×ΔT * Power (heating)=(0.664×Lk×ReL1/2×Pr1/3)×(L×1)×ΔT * Power (heating)=0.664×k×ReL1/2×Pr1/3×ΔT
Determining Velocity Threshold: * For the power saved by heating the oil to exceed the power required to do the heating (P_{saving} > P_{heating}): * 0.35 \times 0.664 \times \rho \times \nu_c^{1/2} \times u^{5/2} \times L^{1/2} > 0.664 \times u^{1/2} \times L^{1/2} \times \nu_f^{-1/2} \times Pr^{1/3} \times k \times \Delta T * Simplifying common terms: * 0.35 \times \rho \times \nu_c^{1/2} \times u^2 > \nu_f^{-1/2} \times Pr^{1/3} \times k \times \Delta T * Given values for the fluid at film temperature: * k=0.64W/mK, Prf=3.57, ΔT=80, ρ=1000. * νf=3.16×10−7m2/s, νc=1.2×10−5m2/s. * The inequality becomes: * u^2 > \frac{(3.16 \times 10^{-7})^{-1/2} \times 3.57^{1/3} \times 0.64 \times 80}{0.35 \times 1000 \times (1.2 \times 10^{-5})^{1/2}} * u^2 > 3630 * u≈60.3m/s
Case Study: Convective Heat Transfer over a Surface
Input Parameters (Question 2): * Twall=50∘C * T∞=20∘C * Film Temperature: Tfilm=250+20=35∘C * Distance along plate: x=100cm=1.0m * Velocity: V∞=0.05m/s * Dynamic/Kinematic viscosity at 35∘C (interpolated/given): ν=0.00725
Reynolds Number Calculation: * Rex=νu×x=0.007250.5×100=68965.5172 * Since Re_x < 5 \times 10^5, the flow is confirmed as laminar.
Local and Average Heat Transfer Coefficient Determination
Nusselt Number Calculations: * Local Nusselt Number (Nux): * Nux=0.332×Pr1/3×Rex1/2 * Using Pr=4.87: * Nux=0.332×(4.87)1/3×(68965.5)1/2=147.78 * Local Convection Coefficient (hx): * hx=xNux×k=1147.78×0.62=91.623W/m2K
Average Coefficients and Heat Flux: * Average Heat Transfer Coefficient (hˉ): * hˉ=2×hx=2×91.623=183.246W/m2K * Average Heat Flux (q′′): * q′′=hˉ×ΔT=183.246×(50−20)=5497.4W/m2 * Total Heat (q): * q=q′′×Area=5497.4×(0.2×1)=4398W
Boundary Layer Characteristics
Thickness Calculation: * The boundary layer thickness (δ) for laminar flow is given by: * δ=4.92×Rexx * δ=4.92×(68965)−1/2≈0.01873m=1.873cm * Since δ≪L, the thin boundary layer assumption and theoretical results are justified.
Shear Stress and Heat Flux at Specified Conditions
Computation of Average Shear Stress (\tau): * τ=21×ρ×u2×Cf,L * Cf,L=1.328×ReL−1/2 * ReL=0.010.5×1×100=5000 * τ=0.5×997×0.52×1.328×(5000)−1/2 * τ=124.625×1.328×0.01414=2.34N/m2
Computation of Average Heat Flux: * Using properties at 20∘C: k=0.59W/mK, Pr=7.07. * q′′=hˉ×ΔT=(LNuL×k)×ΔT * q′′=0.010.59×0.664×(7.07)1/3×(5000)1/2 * q′′=5316.7W/m2
Derivation of the Similarity Solution for Boundary Layer Flow
Similarity Variable and Stream Function: * Definitions for Blasius derivation: * η=y×νxu∞ * u=u∞f′(η) * ψ=(u∞νx)1/2f(η)
Goal: Show that the Blasius equation can be generalized as: * 2f′′′+(n+1)ff′′+2m[1−(f′)2]=0 * This incorporates the case where free stream velocity follows a power law u∞=Cxm.
Derivation Steps: * Substitution for stream function gradients: * u=∂y∂ψ * v=−∂x∂ψ * The momentum equation is transformed into similarity coordinates by calculating the derivatives of f with respect to x and y: * ψyψyx−ψxψyy=mudxdu+νψyyy * Applying the power law u∝xm leads to the coefficients involving m and n in the final ODE.
Energy Equation Analogy: * The governing energy equation is: * u∂x∂T+v∂y∂T=α∂y2∂2T * Defining non-dimensional temperature θ(η)=T∞−TwT−Tw, the energy equation transforms into an ODE similar to the momentum equation, depending on the Prandtl number (Pr).