root/trunk/matml/transport/problems/factarg/factarg-solution.tex

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New problem: Radiation in facing target sputtering

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1\documentclass{article}
2\usepackage{fullpage}
3\newcommand{\PSbox}[3]{\mbox{\rule{0in}{#3}\special{psfile=#1}\hspace{#2}}}
4\begin{document}
5\begin{enumerate}
6\item Radiation in facing target sputtering
7
8  \begin{enumerate}
9  \item There are two ways to use the diagrams to calculate $F_{21}$, one is by
10    the paralell rectangles method:
11
12    \begin{center}
13      \PSbox{factarg1.eps hscale=25 vscale=25}{333pt}{178pt}
14    \end{center}
15
16    $$F_{21}=\frac{F_{2A}-F_{2B}}{2}$$
17    For $F_{2A}$, $x=b/c=10{\rm cm}/10{\rm cm}=1$, and $y=a/c=10{\rm cm}/10{\rm
18    cm}=1$, so the graph gives $F_{2A}=0.2$.  For $F_{2B}$, $x=b/c=10{\rm
19    cm}/20{\rm cm}=0.5$, and $y=a/c=10{\rm cm}/20{\rm cm}=0.5$, so the graph
20    gives $F_{2B}=0.07$.  These and the equation above result in
21    $F_{21}=0.065$.
22
23    The other way is by the common-edge rectangles method, using
24    $\phi=90^\circ$:
25
26    \begin{center}
27      \PSbox{factarg2.eps hscale=25 vscale=25}{336pt}{178pt}
28    \end{center}
29
30    $$F_{21}=2(F_{2C}-F_{2D})$$
31    For $F_{2C}$, $N=a/b=20{\rm cm}/10{\rm cm}=2$ and $L=c/b=10{\rm cm}/10{\rm
32    cm}=1$, so the graph gives $F_{2C}=0.24$.  For $F_{2D}$, $N=a/b=10{\rm
33    cm}/10{\rm cm}=1$, and $L=c/b=10{\rm cm}/10{\rm cm}=1$, so the graph
34    gives $F_{2D}=0.20$.  These and the equation above result in
35    $F_{21}=0.080$, which is, well, somewhat close to the parallel rectangles
36    viewfactor.
37
38    Now use the reciprocity rule to calculate $F_{12}$:
39    $$A_1F_{12}=A_2F_{21}$$
40    $$F_{12}=\frac{A_2F_{21}}{A_1}$$
41    $S_1$ includes two $10\times10$ squares, so $A_1={\rm200cm^2=0.02m^2}$;
42    $S_2$ is one $10\times10$ square, so $A_2={\rm100cm^2=0.01m^2}$.  These and
43    the $F_{21}$s calculated by the two methods above give $F_{12}=0.032$ to
44    0.040.
45
46  \item This is the total power emitted by the targets multiplied by the
47    viewfactor and by the absorptivity of the substrate:
48    $$Q_{12} = \alpha_2 F_{12} A_1\epsilon_1\sigma T_1^4$$
49    Using $\alpha_2=\epsilon_2$ and $F_{12}\simeq0.035$ gives us:
50    $$Q_{12} = {\rm 0.7 \cdot 0.035 \cdot 0.02 m^2 \cdot 0.4 \cdot
51      5.67\times10^{-8}\frac{W}{m^2K^4} \cdot (1200K)^4 = 23W}$$
52    Not a whole lot of power, but for a small substrate, enough to get it
53    decently hot.
54
55  \item This is a similar situation; using $F_{21}=0.07$ gives us:
56    $$Q_{21} = {\rm 0.4 \cdot 0.07 \cdot 0.01 m^2 \cdot 0.7 \cdot
57      5.67\times10^{-8}\frac{W}{m^2K^4} \cdot (900K)^4 = 7.3W}$$
58    Note that the ratio $Q_{12}/Q_{21}$ is simply $T_1^4/T_2^4$.
59
60    This method misses one thing, which is reflection of a surface's radiation
61    off another surface and back onto itself.  With viewfactors as small as
62    these, this secondary absorption of reflected radiation will be negligible.
63    But in general, this is the motivation for the total exchange viewfactors.
64  \end{enumerate}
65\end{enumerate}
66\end{document}
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