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Consider a large vertical plate with a uniform surface temperature of \(130^{\circ} \mathrm{C}\) suspended in quiescent air at \(25^{\circ} \mathrm{C}\) and atmospheric pressure. (a) Estimate the boundary layer thickness at a location \(0.25 \mathrm{~m}\) measured from the lower edge. (b) What is the maximum velocity in the boundary layer at this location and at what position in the boundary layer does the maximum occur? (c) Using the similarity solution result, Equation \(9.19\), determine the heat transfer coefficient \(0.25 \mathrm{~m}\) from the lower edge. (d) At what location on the plate measured from the lower edge will the boundary layer become turbulent?

Short Answer

Expert verified
The boundary layer thickness at a location \(0.25\,m\) from the lower edge is given by \(\delta = 5x \left(\frac{\nu}{v_s}\right)^{1/2}\), where \(x = 0.25\,m\), \(\nu\) is the air's kinematic viscosity, and \(v_s\) is the free stream velocity. The maximum velocity in the boundary layer occurs at the position \(y_{max} = \sqrt{2} \delta\) and has the value \(u_{max} = v_s\). The heat transfer coefficient at that location is given by \(h = \frac{Nu_x k}{x}\), where \(Nu_x\) is the Nusselt number and \(k\) is the air's thermal conductivity. Finally, the location on the plate where the boundary layer becomes turbulent is given by \(x_{crit} = \frac{Re_{crit} \nu}{v_s}\), where \(Re_{crit}\) is the critical Reynolds number, approximately \(5 \times 10^5\).

Step by step solution

01

(a) Finding the boundary layer thickness)

To estimate the boundary layer thickness at a location \(0.25\,m\) from the lower edge, we can use the similarity solution provided by Equation \(7.41\) for the laminar boundary layer: \[ \delta = 5x \left(\frac{\nu}{v_s}\right)^{1/2} \] where - \(\delta\) is the boundary layer thickness - \(x = 0.25\,m\) is the distance from the lower edge - \(\nu\) is the kinematic viscosity of air - \(v_s\) is the free stream velocity Now, we need the free stream velocity. Since the flow is natural convection, we can use the Rayleigh number to find it: \[ Ra_x = \frac{g \beta (T_s - T_\infty) x^3}{\nu \alpha} \] where - \(g = 9.81\,m/s^2\) is the acceleration due to gravity - \(\beta = 1/T_\infty\) is the volumetric thermal expansion coefficient - \(T_s = 130^\circ C\) is the surface temperature - \(T_\infty = 25^\circ C\) is the ambient temperature - \(\alpha\) is the thermal diffusivity of air From the Rayleigh number, we can find the Grashof number: \[ Gr_x = \frac{Ra_x}{Pr} \] where - \(Pr = \frac{\nu}{\alpha}\) is the Prandtl number For natural convection, the laminar flow holds when \(Gr_x < Gr_{crit} = 10^9\). Since we are given that the flow is laminar, we can assume this condition holds. Now, we can find the free stream velocity (\(v_s\)) using the relation between Grashof number and the Reynolds number: \[ Re_x = \frac{Gr_x^{1/2}}{Pr^{1/2}} = \frac{v_s x}{\nu} \] With \(v_s\), we can find \(\delta\) using the above equation for the boundary layer thickness.
02

(b) Finding the maximum velocity)

To find the maximum velocity in the boundary layer at the given location and its position, we can use the similarity solution given by Equation \(9.7\): \[ u(x,y) = v_s \frac{\eta^2}{2} \frac{d^2F(\eta)}{d\eta^2} \] where - \(u(x,y)\) is the local velocity in the horizontal direction - \(\eta = \frac{y}{\delta}\) is the similarity variable - \(F(\eta)\) is the stream function The maximum velocity occurs when \(\frac{d^2F(\eta)}{d\eta^2} = 0\), which means: \[ \frac{d^2F(\eta)}{d\eta^2} = 0 \Rightarrow \eta_{max} = \sqrt{2} \] Plugging this into the equation for the maximum velocity and the position in the boundary layer, we have: \[ u_{max} = v_s \frac{2}{2} \frac{d^2F(\eta_{max})}{d\eta^2} = v_s\] \[ y_{max} = \eta_{max} \delta = \sqrt{2} \delta \]
03

(c) Finding the heat transfer coefficient)

To find the heat transfer coefficient at \(0.25\,m\) from the lower edge, we can use the similarity solution result, Equation \(9.19\) for the Nusselt number: \[ Nu_x = \frac{h x}{k} = 0.664 Re_x^{1/2} Pr^{1/3} \] where - \(h\) is the heat transfer coefficient - \(k\) is the thermal conductivity of air Now, we can find the heat transfer coefficient: \[ h = \frac{Nu_x k}{x} \]
04

(d) Finding the transition location)

To find the location where the boundary layer becomes turbulent, we need to find the critical Reynolds number \(Re_{crit}\). For the flow over a flat plate, the critical Reynolds number is around \(5 \times 10^5\). Using the Reynolds number definition: \[ Re_{crit} = \frac{v_s x_{crit}}{\nu} \] We can solve for the transition location \(x_{crit}\): \[ x_{crit} = \frac{Re_{crit} \nu}{v_s} \]

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Natural Convection
Natural convection occurs when fluid motion is generated by buoyancy forces that result from density variations due to temperature differences in the fluid. This process does not require any external force, such as a fan or pump, to move the fluid. Instead, the fluid flows naturally due to the difference in temperature between the surface and the surrounding medium.
Understanding natural convection is crucial because it significantly affects how heat is transferred from surfaces, especially in applications involving heating and cooling. This phenomenon is commonly observed in situations where a surface, such as a vertical plate, is hotter or cooler than the adjacent fluid. For example, in the exercise above, a vertical plate at 130°C initiates natural convection currents in the quiescent air due to the temperature difference from the ambient air at 25°C.
  • Buoyancy forces cause the warm air near the plate to rise.
  • This movement sets up a fluid flow pattern that aids in the transfer of heat away from the plate.
The fluid dynamics of this process govern how efficiently heat is transferred, and understanding it can lead to better control and optimization of heat exchangers and other thermal systems.
Grashof Number
The Grashof number (Gr) is a dimensionless number that gives a measure of the ratio of the buoyancy force to the viscous force in a fluid. It plays a critical role in analyzing natural convection problems, as it indicates when buoyancy forces overcome viscous forces to initiate fluid flow. The formula for the Grashof number is:\[ Gr_x = \frac{g \beta (T_s - T_\infty) x^3}{u^2} \]where:
  • \(g\) is the acceleration due to gravity.
  • \(\beta\) is the thermal expansion coefficient.
  • \(T_s\) and \(T_\infty\) are the surface and ambient temperatures, respectively.
  • \(x\) is the characteristic length.
  • \(u\) is the kinematic viscosity.
A high Grashof number implies that buoyancy forces are strong compared to viscous forces, leading to more vigorous natural convection currents. In the exercise, Grashof number helps determine the regime of the flow: laminar or turbulent.
For a laminar flow near the vertical plate, maintaining a Grashof number below a critical threshold ensures that the boundary layer does not transition to turbulence, which is crucial for accurate heat transfer calculations.
Reynolds Number
Reynolds number (Re) is another important dimensionless number in fluid dynamics that describes the ratio of inertial forces to viscous forces. It indicates whether a fluid flow is laminar or turbulent.The formula for Reynolds number is:\[ Re_x = \frac{v_s x}{u} \]where:
  • \(v_s\) is the characteristic velocity of the flow.
  • \(x\) is the characteristic length (distance from the leading edge).
  • \(u\) is the kinematic viscosity of the fluid.
In the given exercise, the Reynolds number is used to relate the flow properties in the boundary layer on the plate surface. A low Reynolds number indicates laminar flow, while a high Reynolds number suggests that the flow might transition to turbulent.
This transition is significant because turbulent flow typically results in a different, often higher, heat transfer characteristics compared to laminar flow. Understanding when and where this transition occurs is essential for predicting the flow pattern and calculating the heat transfer accurately.
Heat Transfer Coefficient
The heat transfer coefficient (\(h\)) is a critical parameter in quantifying the efficiency of heat exchange between a surface and a fluid. It measures how well heat is transferred per unit area across the interface. The higher the coefficient, the more efficient the heat transfer.In the context of boundary layer analysis, the heat transfer coefficient is often determined using the Nusselt number (Nu), which is a dimensionless representation of the heat transfer due to convection. The relationship is given by:\[ Nu_x = \frac{h x}{k} \]where:
  • \(h\) is the heat transfer coefficient.
  • \(x\) is the characteristic length.
  • \(k\) is the thermal conductivity of the fluid.
To find the heat transfer coefficient in the exercise, the Nusselt number is calculated using correlations for natural convection, which often involve the Reynolds and Prandtl numbers.
The ability to estimate the heat transfer coefficient accurately is vital for designing efficient thermal systems, and it directly impacts the temperature regulation efficacy of equipment such as radiators, heaters, and cooling devices.

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Most popular questions from this chapter

A vertical, double-pane window, which is \(1 \mathrm{~m}\) on a side and has a \(25-\mathrm{mm}\) gap filled with atmospheric air, separates quiescent room air at \(T_{\infty, i}=20^{\circ} \mathrm{C}\) from quiescent ambient air at \(T_{\infty, o}=-20^{\circ} \mathrm{C}\). Radiation exchange between the window panes, as well as between each pane and its surroundings, may be neglected. (a) Neglecting the thermal resistance associated with conduction heat transfer across each pane, determine the corresponding temperature of each pane and the rate of heat transfer through the window. (b) Comment on the validity of neglecting the conduction resistance of the panes if each is of thickness \(L_{p}=6 \mathrm{~mm}\).

An aluminum alloy (2024) plate, heated to a uniform temperature of \(227^{\circ} \mathrm{C}\), is allowed to cool while vertically suspended in a room where the ambient air and surroundings are at \(27^{\circ} \mathrm{C}\). The plate is \(0.3 \mathrm{~m}\) square with a thickness of \(15 \mathrm{~mm}\) and an emissivity of \(0.25\). (a) Develop an expression for the time rate of change of the plate temperature, assuming the temperature to be uniform at any time. (b) Determine the initial rate of cooling (K/s) when the plate temperature is \(227^{\circ} \mathrm{C}\). (c) Justify the uniform plate temperature assumption. (d) Compute and plot the temperature history of the plate from \(t=0\) to the time required to reach a temperature of \(30^{\circ} \mathrm{C}\). Compute and plot the corresponding variations in the convection and radiation heat transfer rates.

Consider a horizontal pin fin of 6- \(\mathrm{mm}\) diameter and \(60-\mathrm{mm}\) length fabricated from plain carbon steel \((k=57 \mathrm{~W} / \mathrm{m} \cdot \mathrm{K}, \varepsilon=0.5)\). The base of the fin is maintained at \(150^{\circ} \mathrm{C}\), while the quiescent ambient air and the surroundings are at \(25^{\circ} \mathrm{C}\). Assume the fin tip is adiabatic. (a) Estimate the fin heat rate, \(q_{f}\). Use an average fin surface temperature of \(125^{\circ} \mathrm{C}\) in estimating the free convection coefficient and the linearized radiation coefficient. How sensitive is this estimate to your choice of the average fin surface temperature? (b) Use the finite-difference method of solution to obtain \(q_{f}\) when the convection and radiation coefficients are based on local, rather than average, temperatures for the fin. How does your result compare with the analytical solution of part (a)?

A vertical array of circuit boards is immersed in quiescent ambient air at \(T_{\infty}=17^{\circ} \mathrm{C}\). Although the components protrude from their substrates, it is reasonable, as a first approximation, to assume \(A t\) plates with uniform surface heat flux \(q_{s}^{\prime \prime}\). Consider boards of length and width \(L=W=0.4 \mathrm{~m}\) and spacing \(S=25 \mathrm{~mm}\). If the maximum allowable board temperature is \(77^{\circ} \mathrm{C}\), what is the maximum allowable power dissipation per board?

Common practice in chemical processing plants is to clad pipe insulation with a durable, thick aluminum foil. The functions of the foil are to confine the batt insulation and to reduce heat transfer by radiation to the surroundings. Because of the presence of chlorine (at chlorine or seaside plants), the aluminum foil surface, which is initially bright, becomes etched with in- service time. Typically, the emissivity might change from \(0.12\) at installation to \(0.36\) with extended service. For a \(300-\mathrm{mm}\)-diameter foil-covered pipe whose surface temperature is \(90^{\circ} \mathrm{C}\), will this increase in emissivity due to degradation of the foil finish have a significant effect on heat loss from the pipe? Consider two cases with surroundings and ambient air at \(25^{\circ} \mathrm{C}\) : (a) quiescent air and (b) a cross-wind velocity of \(10 \mathrm{~m} / \mathrm{s}\).

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