Temperature Regime of a Radiating Plate with an Internal Heat Source

V. V. IVANOV, A. V. FURMAN
Submitted 1966 | SovietRxiv: ru-196601.09412 | Translated from Russian

Abstract Generated abstract

This paper analyzes the transient temperature field in a radiation-cooled plate with uniform internal heat generation. It formulates the heat-conduction problem with a nonlinear radiative boundary condition, separates the steady component, and introduces a variable transformation to obtain an approximate linearized solution expressed as series formulas for different parameter ranges. The proposed procedure is compared with numerical finite-difference integration for moderate values of the heat-generation and radiation criteria, showing errors of about 7 to 8 percent in the tested range and improved accuracy as these criteria decrease. The results are intended for estimating temperature fields and warm-up times in heat-generating elements cooled by radiation.

Full Text

TEMPERATURE REGIME OF A RADIATION-TRANSMITTING PLATE WITH AN INTERNAL HEAT SOURCE

V. V. IVANOV, A. V. FURMAN

Presented by Professor G. I. Fuks

The mathematical formulation of the problem under consideration has the following form:

\[ \frac{\partial \Theta(X,F_0)}{\partial F_0} = \frac{\partial^2 \Theta(X,F_0)}{\partial X^2} + P_0, \tag{1} \]

\[ \frac{\partial \Theta(1,F_0)}{\partial X} = S_{k_*}\,[1-\Theta^4(1,F_0)], \tag{2} \]

\[ \frac{\partial \Theta(0,F)}{\partial X}=0, \tag{3} \]

\[ \Theta(X,0)=\Theta_{\mathrm{H}}, \tag{4} \]

where

\[ -1 \le X=\frac{x}{R} \le 1,\qquad 0 \le F_0=\frac{a\tau}{R^2}<\infty, \]

\[ \Theta(X,F_0)=\frac{T(X,F_0)}{T_c},\qquad S_{k_*}=\frac{\sigma_{\mathrm{B}}T_c^3}{\lambda}\cdot R, \]

\[ P_0=\frac{q_v\cdot R^2}{\lambda\cdot T_c}. \]

We represent the sought temperature distribution \(\Theta(X,F_0)\) in the form of the sum

\[ \Theta(X,F_0)=\vartheta(X,F_0)+t(X)-D, \tag{5} \]

in which the function \(t(x)\) is the solution of the system (1)–(4) as \(F_0\to\infty\), i.e., the steady-state temperature,

\[ t(X)=\frac{P_0}{2}(1-X^2)+D, \]

\[ D=\sqrt[4]{1+P_0/S_{k_*}}. \]

To determine the nonstationary temperature \(\vartheta(X,F_0)\), it is necessary to integrate the heat-conduction equation

\[ \frac{\partial \vartheta(X,F_0)}{\partial F_0} = \frac{\partial^2 \vartheta(X,F_0)}{\partial X^2}, \tag{6} \]

with boundary conditions

\[ \frac{\partial \vartheta(1,F_0)}{\partial X} = S_{K_*}\,[D^4-\vartheta^4(1,F_0)], \tag{7} \]

\[ \frac{\partial \vartheta(0,F_0)}{\partial X}=0, \tag{8} \]

\[ \vartheta(X,0)=\Theta_{\mathrm{H}}+P_0/2\,(X^2-1). \tag{9} \]

Finding an exact analytical solution of the system (6)–(9) is difficult because of the nonlinearity of the boundary condition (7). Linearization of condition (7) can be carried out with the aid of a new variable \(W(X,F_0)\), defined by the relation

\[ W(X,F_0)= \frac{1}{2D^3} \left[ \operatorname{Arth}\frac{\vartheta(X,F_0)}{D} + \operatorname{arctg}\frac{\vartheta(X,F_0)}{D} \right]. \tag{10} \]

For the new variable \(W(X,F_0)\), the system (6)–(9) is written in the form:

\[ \frac{\partial W(X,F_0)}{\partial F_0} = \frac{\partial^2 W(X,F_0)}{\partial X^2} - \varphi(X,F_0); \tag{11} \]

\[ \varphi(X,F_0) = 4\, \frac{ \vartheta^3(X,F_0) \left[ \dfrac{\partial \vartheta(X,F_0)}{\partial X} \right]^2 }{ \left[D^4-\vartheta^4(X,F_0)\right]^2 }, \]

\[ \frac{\partial W(1,F_0)}{\partial X}=S_{K_*}, \tag{12} \]

\[ \frac{\partial W(0,F_0)}{\partial X}=0, \tag{13} \]

\[ W(X,0)= \frac{1}{2D^3} \left[ \operatorname{Arth} \frac{\Theta_{\mathrm{H}}+P_0/2\,(X^2-1)}{D} + \operatorname{arctg} \frac{\Theta_{\mathrm{H}}+P_0/2\,(X^2-1)}{D} \right] = f(X)^{1)}. \tag{14} \]

The quantity \(\varphi(X,F_0)\) entering equation (11) is always positive; moreover, \(\varphi(0,F_0)=0\) (condition 7), \(\varphi(1,F_0)=4\vartheta^3(1,F_0)S_{K_*}^2\) (condition 8). We estimate \(\varphi(X,F_0)\) by the expression

\[ \varphi(X,F_0)\simeq \frac{1}{2}\,[\varphi(0,F_0)+\varphi(0,0)] = 2\Theta_{\mathrm{H}}^{3}S_{K_*}^{2}. \]

\(^{1}\) We note that, since \(\operatorname{Arth}\,D^{-1}\left[\Theta_{\mathrm{H}}+P_0/2\,(X^2-1)\right]\) exists when

\[ \left| \frac{\Theta_{\mathrm{H}}+P_0/2\,(X^2-1)}{D} \right|<1, \]

substitution (10) may be used in the case when

\[ |\Theta_{\mathrm{H}}-P_0/2|<D. \]

\(^{2}\) The error caused by this assumption will be indicated below.

Then the solution of the system (11)–(14) takes the form [1]:

\[ \begin{aligned} W(X,F_0) = S_{K_*}\Bigg\{& F_0-\frac{1-3X^2}{6} +\sum_{m=1}^{\infty}\frac{2(-1)^{m+1}}{\mu_m^2}\cdot \cos \mu_m X \cdot \exp[-\mu_m^2 F_0]\Bigg\} \\ &-2\Theta_{\mathrm{H}}^3 S_{K_*}^2 \cdot F_0+\int_0^1 f(\xi)\,d\xi \\ &+\sum_{m=1}^{\infty}2\cos\mu_m X\cdot \exp[-\mu_m^2 F_0]\int_0^1 f(\xi)\cdot \cos\mu_m \xi\cdot d\xi . \end{aligned} \tag{15} \]

The integrals entering equation (15) can be evaluated in the following way.

In the region \(W(X,F_0)\cdot D^3 \leqslant 0.6\), dependence (10) has a linear character (Table 1), i.e.

\[ f(X)\simeq \frac{1}{D^4}\left[\Theta_{\mathrm{H}}\,\frac{P_0}{\varepsilon}(X^2-1)\right]. \]

Dependence

\[ W(X,F_0)D^3=\frac{1}{2}\left[ \operatorname{Arth}\frac{\vartheta(X,F_0)}{D} +\operatorname{arctg}\frac{\vartheta(X,F_0)}{D} \right], \]

Table 1

\(\dfrac{\vartheta}{D}\) \(W\cdot D^3\) \(\dfrac{\vartheta}{D}\) \(W\cdot D^3\) \(\dfrac{\vartheta}{D}\) \(W\cdot D^3\) \(\dfrac{\vartheta}{D}\) \(W\cdot D^3\)
0,00 0,000 0,25 0,250 0,50 0,506 0,75 0,808
0,01 0,010 0,26 0,260 0,51 0,517 0,76 0,823
0,02 0,020 0,27 0,270 0,52 0,528 0,77 0,838
0,03 0,030 0,28 0,280 0,53 0,539 0,78 0,854
0,04 0,040 0,29 0,290 0,54 0,550 0,79 0,870
0,05 0,050 0,30 0,300 0,55 0,561 0,80 0,887
0,06 0,060 0,31 0,311 0,56 0,572 0,81 0,904
0,07 0,070 0,32 0,321 0,57 0,583 0,82 0,922
0,08 0,080 0,33 0,331 0,58 0,594 0,83 0,940
0,09 0,090 0,34 0,341 0,59 0,605 0,84 0,960
0,10 0,100 0,35 0,351 0,60 0,617 0,85 0,980
0,11 0,110 0,36 0,361 0,61 0,628 0,86 1,002
0,12 0,120 0,37 0,371 0,62 0,640 0,87 1,024
0,13 0,130 0,38 0,382 0,63 0,652 0,88 1,049
0,14 0,140 0,39 0,392 0,64 0,664 0,89 1,074
0,15 0,150 0,40 0,402 0,65 0,676 0,90 1,102
0,16 0,160 0,41 0,412 0,66 0,688 0,91 1,133
0,17 0,170 0,42 0,423 0,67 0,701 0,92 1,166
0,18 0,180 0,43 0,433 0,68 0,713 0,93 1,204
0,19 0,190 0,44 0,443 0,69 0,726 0,94 1,246
0,20 0,200 0,45 0,454 0,70 0,739 0,95 1,296
0,21 0,210 0,46 0,464 0,71 0,752 0,96 1,355
0,22 0,220 0,47 0,475 0,72 0,766 0,97 1,431
0,23 0,230 0,48 0,485 0,73 0,780 0,98 1,536
0,24 0,240 0,49 0,496 0,74 0,794 0,99 1,713

Then

\[ \begin{aligned} W(X,F_0)\cdot D^4={}&\Theta_{\mathrm{H}}-P_0/2-2\Theta_{\mathrm{H}}^3\left(S_{\kappa_*}^2+P_0S_{\kappa_*}\right)F_0+{}\\ &+\left(S_{\kappa_*}+P_0\right)\left[F_0-\frac{1-3X^2}{6}\right]+{}\\ &+S_{\kappa_*}\sum_{m=1}^{\infty}\frac{2(-1)^{m+1}}{\mu_m^2}\cos \mu_m X\cdot \exp[-\mu_m^2F_0]. \end{aligned} \tag{16} \]

In the region \(W(X,F_0)D^3>0.6\), dependence (14) may be approximated by the function

\[ f(X)\simeq f(0)+[f(1)-f(0)]X^2 . \]

In this case

\[ \begin{aligned} W(X,F_0)\cdot D^3={}&\frac{1}{6}\left(\operatorname{Arth}\frac{\Theta_{\mathrm{H}}}{D}+\operatorname{arctq}\frac{\Theta_{\mathrm{H}}}{D}\right)+{}\\ &+\frac{1}{3}\left(\operatorname{Arth}\frac{\Theta_{\mathrm{H}}-P_0/2}{D} +\operatorname{arctq}\frac{\Theta_{\mathrm{H}}-P_0/2}{D}\right)-{}\\ &-2\left(D\Theta_{\mathrm{H}}^3S_{\kappa_*}^{\,2}F_0 +D^3S_{\kappa_*}\left[F_0-\frac{1-3X^2}{6}\right]\right)+{}\\ &+\left[S_{\kappa_*}D^3-\left(\operatorname{Arth}\frac{\Theta_{\mathrm{H}}}{D} +\operatorname{arctq}\frac{\Theta_{\mathrm{H}}}{D}\right) +\left(\operatorname{Arth}\frac{\Theta_{\mathrm{H}}-P_0/2}{D}\right)+{}\right.\\ &\left.+\operatorname{arctq}\frac{\Theta_{\mathrm{H}}-P_0/2}{D}\right] \sum_{m=1}^{\infty}\frac{2(-1)^{m+1}}{\mu_m^2}\cos\mu_m X\cdot \exp[-\mu_m^2F_0]. \end{aligned} \tag{17} \]

Having determined \(W(X,F_0)\) from (16) or (17), from Table 1 we find \(\vartheta(X,F_0)\).

An investigation of the error of the proposed method was carried out by numerical integration of system (1)–(4) [2] for \(P_0<2.1\), \(S_{\kappa_*}<0.15\). As the numerical calculations showed, in the indicated range of variation of the criteria \(P_0\) and \(S_{\kappa_*}\), the error for all points of the plate does not exceed \(7\text{–}8\%\). With decreasing \(P_0\) and \(S_{\kappa_*}\), the accuracy of the calculation increases.

As an example, let us consider the heating of a ray-absorbing plate \((2R=0.5\ \text{m},\ \lambda=17.45\ \text{W}/\text{m}\cdot\text{deg},\ \sigma_{\mathrm{B}}=4.54\ \text{W}/\text{m}^2\,^\circ\text{K}^4,\ q_v=183460\ \text{W}/\text{m}^3)\) in a medium with \(T_c=313^\circ\text{K}\).

Table 2 compares the values of \(\Theta(X,F_0)\) obtained on the basis of the proposed calculation method and by numerical integration.

Comparison of the results of determining the temperature by different methods.

Table 2

\(F_0\) By the finite-difference method, \(\Theta_{X=1}\) By the finite-difference method, \(\Theta_{X=0}\) By the proposed procedure, \(\Theta_{X=1}\) By the proposed procedure, \(\Theta_{X=0}\)
0.00 1.000 1.000 1.000 1.000
0.84 2.427 2.685 2.497 2.704
1.32 2.819 3.373 2.942 3.490
1.80 3.016 3.791 3.114 3.993
2.16 3.093 3.974 3.175 4.132
2.52 3.210 4.260 3.210 4.260

The results obtained in this work may be used to calculate temperature fields in heat-generating elements cooled by radiation, and also to estimate the time required for individual parts to warm up to a specified temperature, which is especially important for the start-up period and for intermittent operation.

REFERENCES

  1. M. S. Smirnov. On the study of unsteady heat exchange in baking ovens. Proceedings of MTIIP, issue 6. 78, 1956.

  2. L. Kollatz. Numerical Methods for Solving Differential Equations. IL. Moscow, 1953.

Submission history

Temperature Regime of a Radiating Plate with an Internal Heat Source