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To a good approximation, the dynamic viscosity \(\mu\), the thermal conductivity \(k\), and the specific heat \(c_{p}\) are independent of pressure. In what manner do the kinematic viscosity \(v\) and thermal diffusivity \(\alpha\) vary with pressure for an incompressible liquid and an ideal gas? Determine \(\alpha\) of air at \(350 \mathrm{~K}\) for pressures of 1,5 , and \(10 \mathrm{~atm}\). Assuming a transition Reynolds number of \(5 \times 10^{5}\), determine the distance from the leading edge of a flat plate at which transition will occur for air at \(350 \mathrm{~K}\) at pressures of 1,5 , and 10 atm with \(u_{s}=2 \mathrm{~m} / \mathrm{s}\).

Short Answer

Expert verified
For an incompressible liquid, both kinematic viscosity \(v\) and thermal diffusivity \(\alpha\) are constant and independent of pressure. For an ideal gas, \(v\) is inversely proportional to pressure (\(v \propto \frac{1}{P}\)) while \(\alpha\) is directly proportional to pressure (\(\alpha \propto P\)). The thermal diffusivities for air at 350 K are \(\alpha_{1\,\mathrm{atm}}=2.54\times10^{-5}\,\mathrm{m^2/s}\), \(\alpha_{5\,\mathrm{atm}}=1.27\times10^{-4}\,\mathrm{m^2/s}\), and \(\alpha_{10\,\mathrm{atm}}=2.54\times10^{-4}\,\mathrm{m^2/s}\). The distances of transition for each pressure are \(x_{1\,\mathrm{atm}}=3.78\,\mathrm{m}\), \(x_{5\,\mathrm{atm}}=0.756\,\mathrm{m}\), and \(x_{10\,\mathrm{atm}}=0.378\,\mathrm{m}\).

Step by step solution

01

Determine how kinematic viscosity and thermal diffusivity vary with pressure for incompressible liquids and ideal gases.

For an incompressible liquid, the density \(\rho\) is constant and independent of pressure. Since \(\mu\), \(c_p\), and \(k\) are also independent of pressure, both the kinematic viscosity \(v = \frac{\mu}{\rho}\) and thermal diffusivity \(\alpha = \frac{k}{\rho c_p}\) will be constant and independent of pressure for an incompressible liquid. For an ideal gas, the density \(\rho\) depends on the pressure and temperature according to the ideal gas equation: \(\rho = \frac{P}{RT}\), where \(P\) is the pressure, \(R\) is the specific gas constant, and \(T\) is the temperature. As the pressure increases, the density will increase proportionally. Therefore, for an ideal gas: 1. The kinematic viscosity v will be inversely proportional to the pressure: \(v \propto \frac{1}{P}\). 2. The thermal diffusivity \(\alpha\) will be proportional to the pressure: \(\alpha \propto P\).
02

Calculate the thermal diffusivity of air at 350 K for pressures of 1, 5, and 10 atm.

Using the relationship for thermal diffusivity \(\alpha = \frac{k}{\rho c_p}\), we can calculate the values of \(\alpha\) for given pressure values. Assume that air behaves like an ideal gas at the given temperature and pressure conditions. At 350 K and 1 atm (101325 Pa), the properties of air are as follows: - Specific gas constant, \(R = 287 \, \mathrm{J/(kg \cdot K)}\) - Density, \(\rho = \frac{P}{RT} = \frac{101325}{287 \cdot 350} = 1.177 \, \mathrm{kg / m^3}\) - Thermal conductivity, \(k = 0.03 \, \mathrm{W/(m \cdot K)}\) - Specific heat, \(c_p = 1005 \, \mathrm{J/(kg \cdot K)}\) Now, we can find the thermal diffusivity of air at 1 atm: \[ \alpha_{1 \, \mathrm{atm}} = \frac{k}{\rho c_p} = \frac{0.03}{1.177 \cdot 1005} = 2.54\times10^{-5} \, \mathrm{m^2/s} \] Now, we can find the thermal diffusivity of air at 5 and 10 atm using the proportionality relationship between \(\alpha\) and \(P\) for ideal gases: \[ \alpha_{5 \, \mathrm{atm}} = 5\alpha_{1 \, \mathrm{atm}} = 1.27\times10^{-4} \, \mathrm{m^2/s} \] \[ \alpha_{10 \, \mathrm{atm}} = 10\alpha_{1 \, \mathrm{atm}} = 2.54\times10^{-4} \, \mathrm{m^2/s} \]
03

Calculate the distance of transition for air at 350 K at pressures of 1, 5, and 10 atm with \(u_{s}=2 \mathrm{~m} / \mathrm{s}\) assuming a transition Reynolds number of \(5 \times 10^{5}\).

To find the distance of transition, \(x\), we will use the transition Reynolds number equation \(Re_x = \frac{\rho u_s x}{\mu}\). Using the given transition Reynolds number \(Re_x = 5\times10^5\), we can solve for the distance \(x\) at each pressure: As \(\rho\) and \(\mu\) are dependent on pressure, we can first find \(\mu\) for each condition using the relationship \(v = \frac{\mu}{\rho}\), then calculate the distance of transition: At 1 atm: - Dynamic viscosity, \(\mu = \rho v = 1.177 \cdot 1.516\times10^{-5} = 1.785\times10^{-5} \, \mathrm{Pa \cdot s}\) - \(x_{1 \, \mathrm{atm}} = \frac{\mu \, Re_x}{\rho u_s} = \frac{1.785\times10^{-5} \cdot 5\times10^5}{1.177 \cdot 2} = 3.78 \, \mathrm{m}\) At 5 atm: - Density is 5 times higher, \(\rho = 5 \cdot 1.177 = 5.885 \, \mathrm{kg / m^3}\) - Dynamic viscosity, \(\mu = \rho v = 5.885 \cdot 0.303\times10^{-5} = 1.785\times10^{-5} \, \mathrm{Pa \cdot s}\) (remains unchanged) - \(x_{5 \, \mathrm{atm}} = \frac{\mu \, Re_x}{\rho u_s} = \frac{1.785\times10^{-5} \cdot 5\times10^5}{5.885 \cdot 2} = 0.756 \, \mathrm{m}\) At 10 atm: - Density is 10 times higher, \(\rho = 10 \cdot 1.177 = 11.77 \, \mathrm{kg / m^3}\) - Dynamic viscosity, \(\mu = \rho v = 11.77 \cdot 0.1518\times10^{-5} = 1.785\times10^{-5} \, \mathrm{Pa \cdot s}\) (remains unchanged) - \(x_{10 \, \mathrm{atm}} = \frac{\mu \, Re_x}{\rho u_s} = \frac{1.785\times10^{-5} \cdot 5\times10^5}{11.77 \cdot 2} = 0.378 \, \mathrm{m}\)

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Key Concepts

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

Kinematic Viscosity
Kinematic viscosity, represented as u (nu), is a measure of a fluid's resistance to flow when gravity is the force causing flow, relative to its density. It's defined as the dynamic viscosity \( \(\mu\) \) divided by the fluid's density \( \(\rho\) \) and is expressed in \(\text{m}^2/\text{s}\). For liquids, particularly incompressible ones, kinematic viscosity is typically unaffected by changes in pressure since both \(\mu\) and \(\rho\) are constant.

For ideal gases, however, the situation is different. Because density \(\rho\) changes with pressure according to the ideal gas law \( \rho = \frac{P}{RT} \) where \(P\) is the pressure and \(T\) is the temperature, kinematic viscosity varies inversely with pressure \( v \propto \frac{1}{P} \) for an ideal gas. This means as pressure increases, \(\rho\) increases, and since \(\mu\) remains constant, \(v\) decreases.
Dynamic Viscosity
Dynamic viscosity \(\mu\) is a fundamental property of A fluid indicating its resistance to shear or viscous force at a given temperature and pressure. It represents the internal friction within the fluid, quantifying how a fluid resists motion between its layers. Unlike kinematic viscosity, dynamic viscosity doesn't factor in the fluid's density; it's a direct measurement of the force required to move one layer over another and is expressed in \(\text{Pa·s}\) (Pascal-seconds) or \(\text{Poise}\).

In the exercise, the dynamic viscosity for air at different pressures remains constant as it is independent of pressure to a good approximation, and therefore the calculation of transition distances for flow over a flat plate can be simplified by considering the pressures' effect on density alone.
Reynolds Number
Reynolds number \(\text{Re}\) is a dimensionless quantity used in fluid mechanics to predict flow patterns in different fluid flow situations. It's the ratio of inertial forces to viscous forces and provides a criterion for determining whether a flow will be laminar or turbulent. The transition Reynolds number mentioned in the problem, \(5 \times 10^{5}\), signifies the point at which flow over a surface becomes unstable and transitions from a smooth, predictable laminar flow to a chaotic turbulent flow.

Calculating the Reynolds number requires knowledge of kinematic viscosity \(v\), and the characteristic velocity and length scales in the flow. For flow over a flat plate, the distance from the leading edge \(x\) where transition occurs can be calculated by equating the product of flow velocity \(u_s\), density \(\rho\), and the distance \(x\) to the product of dynamic viscosity \(\mu\) and the critical Reynolds number.
Specific Heat
Specific heat (often denoted as \(c_p\) when referring to constant pressure) is the amount of heat needed to raise the temperature of a unit mass of a substance by one degree Celsius (or one Kelvin). Its value varies depending on the material and is crucial for thermal energy calculations in heating and cooling processes.

In the context of the textbook problem, specific heat is assumed to be constant with pressure changes, which simplifies the calculation of thermal diffusivity for air at different pressures. Specific heat plays a vital role in thermodynamics and heat transfer, as it defines how much thermal energy a substance can store, thus affecting how it heats up or cools down.
Heat Transfer

Understanding Thermal Diffusivity

Heat transfer is a field of thermal engineering that concerns the generation, use, conversion, and exchange of thermal energy between physical systems. The thermal diffusivity \(\alpha\) in the original exercise is a measure of how quickly a material can conduct heat relative to its ability to store heat and is given by the formula \(\alpha = \frac{k}{\rho c_{p}}\) where \(k\) is the thermal conductivity.

In engineering applications, knowledge of thermal diffusivity is essential for analyzing heat transfer problems where temperature changes over time, such as the cooling or heating of objects. The exercise illustrates this by calculating thermal diffusivity at different pressures, which influences the transition point on a flat plate exposed to airflow at a certain velocity and temperature.

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Most popular questions from this chapter

A fan that can provide air speeds up to \(50 \mathrm{~m} / \mathrm{s}\) is to be used in a low-speed wind tunnel with atmospheric air at \(25^{\circ} \mathrm{C}\). If one wishes to use the wind tunnel to study flatplate boundary layer behavior up to Reynolds numbers of \(R e_{x}=10^{8}\), what is the minimum plate length that should be used? At what distance from the leading edge would transition occur if the critical Reynolds number were \(R e_{x, c}=5 \times 10^{5}\) ?

If laminar flow is induced at the surface of a disk due to rotation about its axis, the local convection coefficient is known to be a constant, \(h=C\), independent of radius. Consider conditions for which a disk of radius \(r_{o}=100 \mathrm{~mm}\) is rotating in stagnant air at \(T_{\infty}=20^{\circ} \mathrm{C}\) and a value of \(C=20 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\) is maintained. If an embedded electric heater maintains a surface temperature of \(T_{x}=50^{\circ} \mathrm{C}\), what is the local heat flux at the top surface of the disk? What is the total electric power requirement? What can you say about the nature of boundary layer development on the disk?

Experiments have been conducted to determine local heat transfer coefficients for flow perpendicular to a long, isothermal bar of rectangular cross section. The bar is of width \(c\) parallel to the flow, and height \(d\) normal to the flow. For Reynolds numbers in the range \(10^{4} \leq R_{d} \leq 5 \times 10^{4}\), the face-averaged Nusselt numbers are well correlated by an expression of the form The values of \(C\) and \(m\) for the front face, side faces, and back face of the rectangular rod are found to be the following: \begin{tabular}{llll} \hline Face & cld & \(\boldsymbol{C}\) & \(\boldsymbol{m}\) \\ \hline Front & \(0.33 \leq\) cld \(51.33\) & \(0.674\) & \(1 / 2\) \\ Side & \(0.33\) & \(0.153\) & \(2 / 3\) \\ Side & \(1.33\) & \(0.107\) & \(2 / 3\) \\ Back & \(0.33\) & \(0.174\) & \(2 / 3\) \\ Back & \(1.33\) & \(0.153\) & \(2 / 3\) \\ \hline \end{tabular} Determine the value of the average heat transfer coefficient for the entire exposed surface (that is, averaged over all four faces) of a \(c=40\)-mm-wide, \(d=30\)-mm-tall rectangular rod. The rod is exposed to air in cross flow at \(V=10 \mathrm{~m} / \mathrm{s}, T_{x}=300 \mathrm{~K}\). Provide a plausible explanation of the relative values of the face-averaged heat transfer coefficients on the front, side, and back faces.

An object of irregular shape has a characteristic length of \(L=1 \mathrm{~m}\) and is maintained at a uniform surface temperature of \(T_{s}=325 \mathrm{~K}\). It is suspended in an airstream that is at atmospheric pressure \((p=1 \mathrm{~atm})\) and has a velocity of \(V=100 \mathrm{~m} / \mathrm{s}\) and a temperature of \(T_{x}=275 \mathrm{~K}\). The average heat flux from the surface to the air is \(12,000 \mathrm{~W} / \mathrm{m}^{2}\). Referring to the foregoing situation as case 1 , consider the following cases and determine whether conditions are analogous to those of case 1. Each case involves an object of the same shape, which is suspended in an airstream in the same manner. Where analogous behavior does exist, determine the corresponding value of the average convection coefficient. (a) The values of \(T_{s}, T_{x}\), and \(p\) remain the same, but \(L=2 \mathrm{~m}\) and \(V=50 \mathrm{~m} / \mathrm{s}\). (b) The values of \(T_{x}\) and \(T_{\infty}\) remain the same, but \(L=2 \mathrm{~m}, V=50 \mathrm{~m} / \mathrm{s}\), and \(p=0.2 \mathrm{~atm}\). (c) The surface is coated with a liquid film that evaporates into the air. The entire system is at \(300 \mathrm{~K}\), and the diffusion coefficient for the air-vapor mixture is \(D_{\mathrm{AB}}=1.12 \times 10^{-4} \mathrm{~m}^{2} / \mathrm{s}\). Also, \(L=2 \mathrm{~m}\), \(V=50 \mathrm{~m} / \mathrm{s}\), and \(p=1 \mathrm{~atm}\). (d) The surface is coated with another liquid film for which \(D_{\mathrm{AB}}=1.12 \times 10^{-4} \mathrm{~m}^{2} / \mathrm{s}\), and the system is at \(300 \mathrm{~K}\). In this case \(L=2 \mathrm{~m}, V=250 \mathrm{~m} / \mathrm{s}\), and \(p=0.2\) atm.

In flow over a surface, velocity and temperature profiles are of the forms $$ \begin{aligned} &u(y)=A y+B y^{2}-C y^{3} \quad \text { and } \\ &T(y)=D+E y+F y^{2}-G y^{3} \end{aligned} $$ where the coefficients \(A\) through \(G\) are constants. Obtain expressions for the friction coefficient \(C_{f}\) and the convection coefficient \(h\) in terms of \(u_{z}, T_{x}\), and appropriate profile coefficients and fluid properties.

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