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