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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 \(\dot{q}_{0}\) 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 \(T_{\infty}\) -

Short Answer

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Question: Write down the finite difference formulations for the boundary nodes of a plane wall with variable heat generation and constant thermal conductivity, given uniform heat flux at the left boundary (Node 0) and convection at the right boundary (Node 4). Answer: For Node 0: \(k \frac{0 - 2T_0 + T_1}{(\Delta x)^2} = -q_{gen}\) For Node 4: \(k \frac{T_3 - 2T_4 + 0}{(\Delta x)^2} = -q_{gen}\)

Step by step solution

01

Write down the general heat conduction equation

The general one-dimensional heat conduction equation with heat generation is given by: \(\frac{d}{dx}\left( k \frac{dT}{dx} \right) = -q_{gen}\) Where \(k\) is the constant thermal conductivity, \(T\) is the temperature and \(q_{gen}\) is the heat generation. Since the thermal conductivity is constant, we can rewrite the above equation as: \(k \frac{d^2 T}{dx^2} = -q_{gen}\)
02

Apply Finite Difference Formulation on the conduction equation

Now, apply the central finite difference approximation for the second derivative, \(\frac{d^2 T}{dx^2}\), as follows: \(\frac{d^2 T}{dx^2} \approx \frac{T_{i-1} - 2T_i + T_{i+1}}{(\Delta x)^2}\) Where \(T_i\) is the temperature at node \(i\), and \(Δx\) is the uniform nodal spacing. Substitute the finite difference formula for the second derivative in the general heat conduction equation: \(k\frac{T_{i-1} - 2T_i + T_{i+1}}{(\Delta x)^2} = -q_{gen}\)
03

Apply boundary conditions

We need to apply the given boundary conditions at node 0 and node 4. Node 0: uniform heat flux \(\dot{q}_{0}\) \(\dot{q}_{0} = -k \frac{dT}{dx}\Big|_{x=0}\), use forward finite difference approximation of first derivative, \(\dot{q}_{0} \approx -k \frac{T_1 - T_0}{\Delta x}\) Node 4: convection with convection coefficient \(h\) and ambient temperature \(T_{\infty}\) Due to convection, \(\dot{q}_{conv} = h(T_{\infty} - T_4)\) At node 4, the outward heat flow due to conduction \(\dot{q}_{cond}\), is equal to the heat removed due to convection \(\dot{q}_{conv}\): \(-k \frac{dT}{dx}\Big|_{x= x_4} = h(T_{\infty} - T_4)\) Using a backward finite difference approximation of the first derivative, \(-k \frac{T_4 - T_3}{\Delta x} = h(T_{\infty}- T_4)\)
04

Finite Difference Formulation for boundary nodes

Using the above equations, we can now write the finite difference formulations for the boundary nodes. Node 0: \(k\frac{T_{i-1} - 2T_i + T_{i+1}}{(\Delta x)^2} = -q_{gen}\) Substituting the known values, we get: \(k \frac{0 - 2T_0 + T_1}{(\Delta x)^2} = -q_{gen}\) Node 4: \(k\frac{T_{i-1} - 2T_i + T_{i+1}}{(\Delta x)^2} = -q_{gen}\) Substituting the known values, we get: \(k \frac{T_3 - 2T_4 + 0}{(\Delta x)^2} = -q_{gen}\) Finally, we have obtained the finite difference formulation for the boundary nodes of the plane wall with given boundary conditions.

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Most popular questions from this chapter

Solar radiation incident on a large body of clean water $\left(k=0.61 \mathrm{~W} / \mathrm{m} \cdot \mathrm{K}\right.\( and \)\left.\alpha=0.15 \times 10^{-6} \mathrm{~m}^{2} / \mathrm{s}\right)$ such as a lake, a river, or a pond is mostly absorbed by water, and the amount of absorption varies with depth. For solar radiation incident at a \(45^{\circ}\) angle on a \(1-\mathrm{m}\)-deep large pond whose bottom surface is black (zero reflectivity), for example, \(2.8\) percent of the solar energy is reflected back to the atmosphere, \(37.9\) percent is absorbed by the bottom surface, and the remaining \(59.3\) percent is absorbed by the water body. If the pond is considered to be four layers of equal thickness \((0.25 \mathrm{~m}\) in this case), it can be shown that \(47.3\) percent of the incident solar energy is absorbed by the top layer, \(6.1\) percent by the upper mid layer, \(3.6\) percent by the lower mid layer, and 2.4 percent by the bottom layer [for more information, see Cengel and Ozi?ik, Solar Energy, 33, no. 6 (1984), pp. 581-591]. The radiation absorbed by the water can be treated conveniently as heat generation in the heat transfer analysis of the pond. Consider a large \(1-\mathrm{m}\)-deep pond that is initially at a uniform temperature of \(15^{\circ} \mathrm{C}\) throughout. Solar energy is incident on the pond surface at \(45^{\circ}\) at an average rate of $500 \mathrm{~W} / \mathrm{m}^{2}$ for a period of 4 h. Assuming no convection currents in the water and using the explicit finite difference method with a mesh size of \(\Delta x=0.25 \mathrm{~m}\) and a time step of \(\Delta t=15 \mathrm{~min}\), determine the temperature distribution in the pond under the most favorable conditions (i.e., no heat losses from the top or bottom surfaces of the pond). The solar energy absorbed by the bottom surface of the pond can be treated as a heat flux to the water at that surface in this case.

Suggest some practical ways of reducing the roundoff error.

In the energy balance formulation of the finite difference method, it is recommended that all heat transfer at the boundaries of the volume element be assumed to be into the volume element even for steady heat conduction. Is this a valid recommendation even though it seems to violate the conservation of energy principle?

Consider steady heat conduction in a plane wall whose left surface (node 0 ) is maintained at \(40^{\circ} \mathrm{C}\) while the right surface (node 8 ) is subjected to a heat flux of \(3000 \mathrm{~W} / \mathrm{m}^{2}\). Express the finite difference formulation of the boundary nodes 0 and 8 for the case of no heat generation. Also obtain the finite difference formulation for the rate of heat transfer at the left boundary.

Consider an aluminum alloy fin $(k=180 \mathrm{~W} / \mathrm{m} \cdot \mathrm{K})\( of triangular cross section whose length is \)L=5 \mathrm{~cm}$, base thickness is \(b=1 \mathrm{~cm}\), and width \(w\) in the direction normal to the plane of paper is very large. The base of the fin is maintained at a temperature of \(T_{0}=180^{\circ} \mathrm{C}\). The fin is losing heat by convection to the ambient air at \(T_{\infty}=25^{\circ} \mathrm{C}\) with a heat transfer coefficient of $h=25 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}$ and by radiation to the surrounding surfaces at an average temperature of \(T_{\text {sarr }}=290 \mathrm{~K}\). Using the finite difference method with six equally spaced nodes along the fin in the \(x\)-direction, determine \((a)\) the temperatures at the nodes and (b) the rate of heat transfer from the fin for \(w=1 \mathrm{~m}\). Take the emissivity of the fin surface to be \(0.9\) and assume steady onedimensional heat transfer in the fin. Answers: (a) \(177.0^{\circ} \mathrm{C}\), $174.1^{\circ} \mathrm{C}, 171.2^{\circ} \mathrm{C}, 168.4^{\circ} \mathrm{C}, 165.5^{\circ} \mathrm{C} ;\( (b) \)537 \mathrm{~W}$

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