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=10CT_{\infty} = 10^{\circ}C.     * The wall temperature is initially defined as Tw=10CT_w = 10^{\circ}C.     * The local drag coefficient (Cf,xC_{f,x}) for laminar flow over a flat plate is given by the correlation:         * Cf,x=0.664×Rex1/2C_{f,x} = 0.664 \times Re_x^{-1/2}     

  • The average drag coefficient (Cf,LC_{f,L}) for the entire length of the plate is given by:         * Cf,L=1.328×ReL1/2C_{f,L} = 1.328 \times Re_L^{-1/2}

  • Shear Stress and Force Formulation:     * The shear stress (τw\tau_w) exerted on the fluid by the wall is calculated using the average drag coefficient:         * τw=12×ρ×u2×Cf,L\tau_w = \frac{1}{2} \times \rho \times u^2 \times C_{f,L}     * Where uu represents the free stream velocity.     * Substituting the average drag coefficient formula into the shear stress equation yields:         * τw=12×ρ×u2×1.328×ReL1/2\tau_w = \frac{1}{2} \times \rho \times u^2 \times 1.328 \times Re_L^{-1/2}     * The total force (FF) is the product of wall shear stress and the surface area:         * Force=Stress×Area\text{Force} = \text{Stress} \times \text{Area}     * Assuming a unit length for the width of the plate (W=1W = 1), the area is L×1L \times 1.     * The total force is derived as:         * F=12×ρ×u2×1.328×ReL1/2×L×1F = \frac{1}{2} \times \rho \times u^2 \times 1.328 \times Re_L^{-1/2} \times L \times 1

Power Consumption and Velocity Relationships

  • Power Derivation:     * Power is defined as the product of force and velocity:         * Power=Force×Velocity\text{Power} = \text{Force} \times \text{Velocity}     * Substituting the force expression:         * Power=12×ρ×u2×1.328×ReL1/2×L×1×u\text{Power} = \frac{1}{2} \times \rho \times u^2 \times 1.328 \times Re_L^{-1/2} \times L \times 1 \times u     * Recalling the definition of the Reynolds number (ReL=u×LνRe_L = \frac{u \times L}{\nu}), the power expression becomes:         * P=0.664×ρ×u3×(u×Lν)1/2×LP = 0.664 \times \rho \times u^3 \times \left(\frac{u \times L}{\nu}\right)^{-1/2} \times L     * Simplifying the powers of velocity (uu) and length (LL):         * P=0.664×ρ×u3×u1/2×L1/2×ν1/2×LP = 0.664 \times \rho \times u^3 \times u^{-1/2} \times L^{-1/2} \times \nu^{1/2} \times L         * P=0.664×ρ×u5/2×ν1/2×L1/2P = 0.664 \times \rho \times u^{5/2} \times \nu^{1/2} \times L^{1/2}

  • Proportionality:     * From the derived formula, Power (PP) is proportional to the kinematic viscosity (ν\nu) raised to the power of one-half:         * Pν1/2P \propto \nu^{1/2}

Comparative Analysis of Temperature Conditions on Fluid Properties

  • Condition Changes (Question 1a):     * Scenario: The wall temperature is increased to Tw=90CT_w = 90^{\circ}C.     * The film temperature (TfT_f) is calculated as the average of the wall temperature and the free stream temperature:         * Tf=90+102=50CT_f = \frac{90 + 10}{2} = 50^{\circ}C     * The properties of water vary between the cold condition (10C10^{\circ}C) and the film condition (50C50^{\circ}C).

  • Viscosity Data:     * Dynamic viscosity at 10C10^{\circ}C (μ10C\mu_{10^{\circ}C}): 0.013g/am.s0.013\,g/am.s     * Dynamic viscosity at 50C50^{\circ}C (μ50C\mu_{50^{\circ}C}): 0.00548g/amis0.00548\,g/amis     * Comparing the power requirements between the two states using the proportionality Pμ1/2P \propto \mu^{1/2} (assuming constant density):         * P50CP10C=(μ50Cμ10C)1/2\frac{P_{50^{\circ}C}}{P_{10^{\circ}C}} = \left(\frac{\mu_{50^{\circ}C}}{\mu_{10^{\circ}C}}\right)^{1/2}         * P50CP10C=(0.005480.013)1/20.65\frac{P_{50^{\circ}C}}{P_{10^{\circ}C}} = \left(\frac{0.00548}{0.013}\right)^{1/2} \approx 0.65

Heat Transfer Nuance and Power Savings Analysis

  • Power Savings (Question 1b):     * The relative power at the higher temperature is 65%65\% of the power at the lower temperature (Pf=0.65×PcP_f = 0.65 \times P_c).     * The power saving is calculated as:         * Psaving=PcPf=Pc0.65×Pc=0.35×PcP_{saving} = P_c - P_f = P_c - 0.65 \times P_c = 0.35 \times P_c     * The literal expression for power saving is:         * Psaving=0.35×0.664×ρ×νc1/2×u5/2×L1/2P_{saving} = 0.35 \times 0.664 \times \rho \times \nu_c^{1/2} \times u^{5/2} \times L^{1/2}

  • Heating Power via Convection:     * The convection correlation for the Nusselt number (NuNu) is:         * Nu=hˉ×Lk=0.664×ReL1/2×Pr1/3Nu = \frac{\bar{h} \times L}{k} = 0.664 \times Re_L^{1/2} \times Pr^{1/3}     * The average heat transfer coefficient (hˉ\bar{h}) is:         * hˉ=0.664×kL×(u×Lν)1/2×Pr1/3\bar{h} = 0.664 \times \frac{k}{L} \times \left(\frac{u \times L}{\nu}\right)^{1/2} \times Pr^{1/3}     * The power required for heating is given by:         * Power (heating)=hˉ×A×ΔT\text{Power (heating)} = \bar{h} \times A \times \Delta T         * Power (heating)=(0.664×kL×ReL1/2×Pr1/3)×(L×1)×ΔT\text{Power (heating)} = \left(0.664 \times \frac{k}{L} \times Re_L^{1/2} \times Pr^{1/3}\right) \times (L \times 1) \times \Delta T         * Power (heating)=0.664×k×ReL1/2×Pr1/3×ΔT\text{Power (heating)} = 0.664 \times k \times Re_L^{1/2} \times Pr^{1/3} \times \Delta T

  • 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/mKk = 0.64\,W/mK, Prf=3.57Pr_f = 3.57, ΔT=80\Delta T = 80, ρ=1000\rho = 1000.         * νf=3.16×107m2/s\nu_f = 3.16 \times 10^{-7}\,m^2/s, νc=1.2×105m2/s\nu_c = 1.2 \times 10^{-5}\,m^2/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         * u60.3m/su \approx 60.3\,m/s

  • Laminar Flow Stability Check:     * To ensure flow remains laminar (Re_L < 5 \times 10^5):         * \frac{u \times L}{\nu} < 5 \times 10^5         * L < \frac{5 \times 10^5 \times 3.16 \times 10^{-7}}{60.3}         * L < 2.62 \times 10^{-3}\,m

Case Study: Convective Heat Transfer over a Surface

  • Input Parameters (Question 2):     * Twall=50CT_{wall} = 50^{\circ}C     * T=20CT_{\infty} = 20^{\circ}C     * Film Temperature: Tfilm=50+202=35CT_{film} = \frac{50 + 20}{2} = 35^{\circ}C     * Distance along plate: x=100cm=1.0mx = 100\,cm = 1.0\,m     * Velocity: V=0.05m/sV_{\infty} = 0.05\,m/s     * Dynamic/Kinematic viscosity at 35C35^{\circ}C (interpolated/given): ν=0.00725\nu = 0.00725

  • Reynolds Number Calculation:     * Rex=u×xν=0.5×1000.00725=68965.5172Re_x = \frac{u \times x}{\nu} = \frac{0.5 \times 100}{0.00725} = 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 (NuxNu_x):         * Nux=0.332×Pr1/3×Rex1/2Nu_x = 0.332 \times Pr^{1/3} \times Re_x^{1/2}         * Using Pr=4.87Pr = 4.87:         * Nux=0.332×(4.87)1/3×(68965.5)1/2=147.78Nu_x = 0.332 \times (4.87)^{1/3} \times (68965.5)^{1/2} = 147.78     * Local Convection Coefficient (hxh_x):         * hx=Nux×kx=147.78×0.621=91.623W/m2Kh_x = \frac{Nu_x \times k}{x} = \frac{147.78 \times 0.62}{1} = 91.623\,W/m^2K

  • Average Coefficients and Heat Flux:     * Average Heat Transfer Coefficient (hˉ\bar{h}):         * hˉ=2×hx=2×91.623=183.246W/m2K\bar{h} = 2 \times h_x = 2 \times 91.623 = 183.246\,W/m^2K     * Average Heat Flux (qq''):         * q=hˉ×ΔT=183.246×(5020)=5497.4W/m2q'' = \bar{h} \times \Delta T = 183.246 \times (50 - 20) = 5497.4\,W/m^2     * Total Heat (qq):         * q=q×Area=5497.4×(0.2×1)=4398Wq = q'' \times \text{Area} = 5497.4 \times (0.2 \times 1) = 4398\,W

Boundary Layer Characteristics

  • Thickness Calculation:     * The boundary layer thickness (δ\delta) for laminar flow is given by:         * δ=4.92×xRex\delta = 4.92 \times \frac{x}{\sqrt{Re_x}}         * δ=4.92×(68965)1/20.01873m=1.873cm\delta = 4.92 \times (68965)^{-1/2} \approx 0.01873\,m = 1.873\,cm     * Since δL\delta \ll L, the thin boundary layer assumption and theoretical results are justified.

Shear Stress and Heat Flux at Specified Conditions

  • Scenario (Question 3):     * u=0.5m/su_{\infty} = 0.5\,m/s     * L=1cm=0.01mL = 1\,cm = 0.01\,m     * ΔT=1C\Delta T = 1^{\circ}C     * T=20CT_{\infty} = 20^{\circ}C     * Properties at 50C50^{\circ}C (specified for computation):         * ρ=0.997g/cm3\rho = 0.997\,g/cm^3         * μ=0.01cm2/s\mu = 0.01\,cm^2/s

  • Computation of Average Shear Stress (\tau):     * τ=12×ρ×u2×Cf,L\tau = \frac{1}{2} \times \rho \times u^2 \times C_{f,L}     * Cf,L=1.328×ReL1/2C_{f,L} = 1.328 \times Re_L^{-1/2}     * ReL=0.5×10.01×100=5000Re_L = \frac{0.5 \times 1}{0.01} \times 100 = 5000     * τ=0.5×997×0.52×1.328×(5000)1/2\tau = 0.5 \times 997 \times 0.5^2 \times 1.328 \times (5000)^{-1/2}     * τ=124.625×1.328×0.01414=2.34N/m2\tau = 124.625 \times 1.328 \times 0.01414 = 2.34\,N/m^2

  • Computation of Average Heat Flux:     * Using properties at 20C20^{\circ}C: k=0.59W/mKk = 0.59\,W/mK, Pr=7.07Pr = 7.07.     * q=hˉ×ΔT=(NuL×kL)×ΔTq'' = \bar{h} \times \Delta T = \left(\frac{Nu_L \times k}{L}\right) \times \Delta T     * q=0.590.01×0.664×(7.07)1/3×(5000)1/2q'' = \frac{0.59}{0.01} \times 0.664 \times (7.07)^{1/3} \times (5000)^{1/2}     * q=5316.7W/m2q'' = 5316.7\,W/m^2

Derivation of the Similarity Solution for Boundary Layer Flow

  • Governing Equations:     * Continuity Equation: ux+vy=0\frac{\partial u}{\partial x} + \frac{\partial v}{\partial y} = 0     * Momentum Equation: uux+vuy=ν2uy2u \frac{\partial u}{\partial x} + v \frac{\partial u}{\partial y} = \nu \frac{\partial^2 u}{\partial y^2}

  • Similarity Variable and Stream Function:     * Definitions for Blasius derivation:         * η=y×uνx\eta = y \times \sqrt{\frac{u_{\infty}}{\nu x}}         * u=uf(η)u = u_{\infty} f'(\eta)         * ψ=(uνx)1/2f(η)\psi = (u_{\infty} \nu x)^{1/2} f(\eta)

  • Goal: Show that the Blasius equation can be generalized as:     * 2f+(n+1)ff+2m[1(f)2]=02f''' + (n+1)ff'' + 2m[1 - (f')^2] = 0     * This incorporates the case where free stream velocity follows a power law u=Cxmu_{\infty} = C x^m.

  • Derivation Steps:     * Substitution for stream function gradients:         * u=ψyu = \frac{\partial \psi}{\partial y}         * v=ψxv = -\frac{\partial \psi}{\partial x}     * The momentum equation is transformed into similarity coordinates by calculating the derivatives of ff with respect to xx and yy:         * ψyψyxψxψyy=mududx+νψyyy\psi_y \psi_{yx} - \psi_x \psi_{yy} = m u \frac{du}{dx} + \nu \psi_{yyy}     * Applying the power law uxmu \propto x^m leads to the coefficients involving mm and nn in the final ODE.

  • Energy Equation Analogy:     * The governing energy equation is:         * uTx+vTy=α2Ty2u \frac{\partial T}{\partial x} + v \frac{\partial T}{\partial y} = \alpha \frac{\partial^2 T}{\partial y^2}     * Defining non-dimensional temperature θ(η)=TTwTTw\theta(\eta) = \frac{T - T_w}{T_{\infty} - T_w}, the energy equation transforms into an ODE similar to the momentum equation, depending on the Prandtl number (PrPr).