Consider one-dimensional transient heat conduction in a plane wall with variable heat generation and variable thermal conductivity. The nodal network of the medium consists of nodes 0,1 , and 2 with a uniform nodal spacing of \(\Delta x\). Using the energy balance approach, obtain the explicit finite difference formulation of this problem for the case of specified heat flux \(\dot{q}_{0}\) and convection at the left boundary (node 0 ) with a convection coefficient of \(h\) and ambient temperature of \(T_{\infty}\), and radiation at the right boundary (node 2 ) with an emissivity of \(\varepsilon\) and surrounding temperature of \(T_{\text {surr }}\).

Short Answer

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**Question:** Find the explicit finite difference formulation for one-dimensional transient heat conduction in a plane wall with variable heat generation and variable thermal conductivity. The boundary conditions consist of specified heat flux and convection at the left boundary and radiation at the right boundary. **Answer:** The explicit finite difference formulation for the given problem is as follows: $$\frac{T_0^{n+1} - T_0^n}{\Delta t} = \frac{1}{\rho c_p\Delta x}\left[\dot{q}_{0} - h(T_0^n - T_{\infty})\right]$$ $$\frac{T_1^{n+1} - T_1^n}{\Delta t} = \frac{1}{\rho c_p\Delta x}\left[-k_1\frac{T_1^n - T_0^n}{\Delta x} - k_2\frac{T_2^n - T_1^n}{\Delta x}\right]$$ $$\frac{T_2^{n+1} - T_2^n}{\Delta t} = \frac{1}{\rho c_p\Delta x}\left[-k_2\frac{T_2^n - T_1^n}{\Delta x} - \varepsilon\sigma(T_2^{n^4} - T_{\text{surr}}^4)\right]$$ These equations represent the future temperatures at each node based on the current temperatures and the given boundary conditions.

Step by step solution

01

Energy balance equation for node 0

For node 0, we have convection and specified heat flux as boundary conditions. Write the energy balance equation considering these conditions: $$\dot{q}_{0} - q_{c} = \frac{dT_0}{dt}\rho c_p\Delta x$$ Where \(q_{c} = h(T_0 - T_{\infty})\) is the convective heat flux, \(\rho\) is the density, and \(c_p\) is the specific heat. The left side of the equation represents the net heat flux entering the node, and the right side represents the rate at which the temperature of the node changes.
02

Energy balance equation for node 1

For node 1, we consider the heat fluxes from node 0 and from node 2. Write the energy balance equation considering these heat fluxes: $$q_{02} + q_{12} = \frac{dT_1}{dt}\rho c_p\Delta x$$ Where \(q_{02}\) and \(q_{12}\) represent the heat fluxes from node 0 to node 1 and from node 1 to node 2, respectively. These heat fluxes can be calculated using Fourier's law: $$q_{02} = -k_1\frac{T_1 - T_0}{\Delta x}, \qquad q_{12} = -k_2\frac{T_2 - T_1}{\Delta x}$$ \(k_1\) and \(k_2\) represent the thermal conductivities at the midpoint of node 0 and node 1, and node 1 and node 2, respectively.
03

Energy balance equation for node 2

For node 2, we have radiation as the boundary condition. Write the energy balance equation considering this condition: $$q_{12} - q_r = \frac{dT_2}{dt}\rho c_p\Delta x$$ Where \(q_r = \varepsilon \sigma(T_2^4 - T_{\text{surr}}^4)\) is the radiative heat flux, \(\varepsilon\) is the emissivity, and \(\sigma\) is the Stefan-Boltzmann constant. The left side of the equation represents the net heat flux entering the node, and the right side represents the rate at which the temperature of the node changes.
04

Finite difference formulation

Convert each energy balance equation into finite difference form by replacing the temperature time derivatives with forward difference approximations: $$\frac{T_0^{n+1} - T_0^n}{\Delta t} = \frac{1}{\rho c_p\Delta x}\left[\dot{q}_{0} - h(T_0^n - T_{\infty})\right]$$ $$\frac{T_1^{n+1} - T_1^n}{\Delta t} = \frac{1}{\rho c_p\Delta x}\left[-k_1\frac{T_1^n - T_0^n}{\Delta x} - k_2\frac{T_2^n - T_1^n}{\Delta x}\right]$$ $$\frac{T_2^{n+1} - T_2^n}{\Delta t} = \frac{1}{\rho c_p\Delta x}\left[-k_2\frac{T_2^n - T_1^n}{\Delta x} - \varepsilon\sigma(T_2^{n^4} - T_{\text{surr}}^4)\right]$$ Where \(n\) represents the current time step and \(n+1\) represents the future time step. Now we have obtained the explicit finite difference formulation for the given problem with the specified boundary conditions.

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Most popular questions from this chapter

What are the limitations of the analytical solution methods?

Using EES (or other) software, solve these systems of algebraic equations. (a) \(4 x_{1}-x_{2}+2 x_{3}+x_{4}=-6\) $$ \begin{aligned} x_{1}+3 x_{2}-x_{3}+4 x_{4} &=-1 \\ -x_{1}+2 x_{2}+5 x_{4} &=5 \\ 2 x_{2}-4 x_{3}-3 x_{4} &=-5 \end{aligned} $$ (b) $$ \begin{aligned} 2 x_{1}+x_{2}^{4}-2 x_{3}+x_{4} &=1 \\ x_{1}^{2}+4 x_{2}+2 x_{3}^{2}-2 x_{4} &=-3 \\ -x_{1}+x_{2}^{4}+5 x_{3} &=10 \\ 3 x_{1}-x_{3}^{2}+8 x_{4} &=15 \end{aligned} $$

Consider steady one-dimensional heat conduction in a plane wall with variable heat generation and constant thermal conductivity. The nodal network of the medium consists of nodes \(0,1,2,3\), and 4 with a uniform nodal spacing of \(\Delta x\). Using the finite difference form of the first derivative (not the energy balance approach), obtain the finite difference formulation of the boundary nodes for the case of uniform heat flux \(q_{0}\) at the left boundary (node 0 ) and convection at the right boundary (node 4) with a convection coefficient of \(h\) and an ambient temperature of \(T_{\infty}\).

Consider a medium in which the finite difference formulation of a general interior node is given in its simplest form as $$ T_{\text {node }}=\left(T_{\text {left }}+T_{\text {top }}+T_{\text {right }}+T_{\text {bottom }}\right) / 4 $$ (a) Is heat transfer in this medium steady or transient? (b) Is heat transfer one-, two-, or three-dimensional? (c) Is there heat generation in the medium? (d) Is the nodal spacing constant or variable? (e) Is the thermal conductivity of the medium constant or variable?

Consider steady one-dimensional heat conduction in a plane wall with variable heat generation and constant thermal conductivity. The nodal network of the medium consists of nodes \(0,1,2\), and 3 with a uniform nodal spacing of \(\Delta x\). The temperature at the left boundary (node 0 ) is specified. Using the energy balance approach, obtain the finite difference formulation of boundary node 3 at the right boundary for the case of combined convection and radiation with an emissivity of \(\varepsilon\), convection coefficient of \(h\), ambient temperature of \(T_{\circ}\), and surrounding temperature of \(T_{\text {surr }}\). Also, obtain the finite difference formulation for the rate of heat transfer at the left boundary.

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