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<TITLE>How is the channel number coverted into angle?</TITLE>
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<H1><A NAME="SECTION00610000000000000000"></A><A NAME="sec:angcal"></A>
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<BR>
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How is the channel number coverted into angle?
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</H1>
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<P>
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Mythen II modules are composed by 1280 pixels, each having width p=0.05 mm, and numbered with j=0,..,1279.
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Angles are counted counterclockwise from the beam direction. For the m-th module, the angle <!-- MATH
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$\alpha_{jm}$
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-->
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<IMG
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WIDTH="33" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img41.png"
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ALT="$ \alpha_{jm}$">
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of its j-th pixel center
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can be determined using the three geometric parameters <IMG
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WIDTH="29" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img42.png"
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ALT="$ R_m$">
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[mm], <IMG
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WIDTH="28" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img43.png"
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ALT="$ \Phi_m$">
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[deg], <IMG
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WIDTH="30" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img44.png"
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ALT="$ D_m$">
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[mm], as in Fig. <A HREF="#acon"><IMG ALIGN="BOTTOM" BORDER="1" ALT="[*]"
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SRC="file:/usr/share/latex2html/icons/crossref.png"></A>.
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The detector group uses instead the 3 parameters center <IMG
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WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img45.png"
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ALT="$ c_m$">
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[ ], offset <IMG
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WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img46.png"
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ALT="$ o_m$">
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[deg], conversion <IMG
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WIDTH="25" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img47.png"
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ALT="$ k_m$">
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[ ].
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The law with the 3 geometric parameter is
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<P></P>
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<DIV ALIGN="CENTER"><!-- MATH
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\begin{equation}
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\alpha_{jm}=\Phi_m-{\ensuremath{\left({{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{180}}}}{{\ensuremath{\displaystyle{\pi}}}}}}}}\right)}}\arctan{\ensuremath{\left({{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{D_m-pj}}}}{{\ensuremath{\displaystyle{R_m}}}}}}}}\right)}}
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\end{equation}
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-->
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<TABLE CELLPADDING="0" WIDTH="100%" ALIGN="CENTER">
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<TR VALIGN="MIDDLE">
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<TD NOWRAP ALIGN="CENTER"><IMG
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WIDTH="285" HEIGHT="54" ALIGN="MIDDLE" BORDER="0"
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SRC="img48.png"
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ALT="$\displaystyle \alpha_{jm}=\Phi_m-{\ensuremath{\left({{\ensuremath{\displaystyle...
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...remath{\displaystyle{D_m-pj}}}}{{\ensuremath{\displaystyle{R_m}}}}}}}}\right)}}$"></TD>
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<TD NOWRAP WIDTH="10" ALIGN="RIGHT">
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(5.1)</TD></TR>
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</TABLE></DIV>
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<BR CLEAR="ALL"><P></P>
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The corresponding law using DG's parameters is
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<P></P>
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<DIV ALIGN="CENTER"><!-- MATH
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\begin{equation}
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\alpha_{jm}=o_m+{\ensuremath{\left({{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{180}}}}{{\ensuremath{\displaystyle{\pi}}}}}}}}\right)}}c_mk_m+{\ensuremath{\left({{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{180}}}}{{\ensuremath{\displaystyle{\pi}}}}}}}}\right)}}\arctan{\ensuremath{\left[{{\ensuremath{\left({j-c_m}\right)}}k_m}\right]}}
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\end{equation}
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-->
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<TABLE CELLPADDING="0" WIDTH="100%" ALIGN="CENTER">
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<TR VALIGN="MIDDLE">
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<TD NOWRAP ALIGN="CENTER"><IMG
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WIDTH="391" HEIGHT="54" ALIGN="MIDDLE" BORDER="0"
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SRC="img49.png"
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ALT="$\displaystyle \alpha_{jm}=o_m+{\ensuremath{\left({{\ensuremath{\displaystyle{\f...
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...t)}}\arctan{\ensuremath{\left[{{\ensuremath{\left({j-c_m}\right)}}k_m}\right]}}$"></TD>
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<TD NOWRAP WIDTH="10" ALIGN="RIGHT">
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(5.2)</TD></TR>
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</TABLE></DIV>
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<BR CLEAR="ALL"><P></P>
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One can convert the two forms by equating separately the term out of the arctan and the argument of arctan for two different values of j.
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It results
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<BR>
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<DIV ALIGN="CENTER">
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<!-- MATH
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\begin{eqnarray}
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c_m&=&{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{D_m}}}}{{\ensuremath{\displaystyle{p}}}}}}};\\
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k_m&=&{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{p}}}}{{\ensuremath{\displaystyle{R_m}}}}}}};\\
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o_m&=&\Phi_m-{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{180}}}}{{\ensuremath{\displaystyle{\pi}}}}}}}{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{D_m}}}}{{\ensuremath{\displaystyle{R_m}}}}}}}.
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\end{eqnarray}
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-->
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<TABLE CELLPADDING="0" ALIGN="CENTER" WIDTH="100%">
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<TR VALIGN="MIDDLE"><TD NOWRAP ALIGN="RIGHT"><IMG
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WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img50.png"
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ALT="$\displaystyle c_m$"></TD>
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<TD WIDTH="10" ALIGN="CENTER" NOWRAP><IMG
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WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img51.png"
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ALT="$\displaystyle =$"></TD>
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<TD ALIGN="LEFT" NOWRAP><IMG
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WIDTH="38" HEIGHT="53" ALIGN="MIDDLE" BORDER="0"
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SRC="img52.png"
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ALT="$\displaystyle {\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{D_m}}}}{{\ensuremath{\displaystyle{p}}}}}}};$"></TD>
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<TD WIDTH=10 ALIGN="RIGHT">
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(5.3)</TD></TR>
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<TR VALIGN="MIDDLE"><TD NOWRAP ALIGN="RIGHT"><IMG
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WIDTH="25" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img53.png"
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ALT="$\displaystyle k_m$"></TD>
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<TD WIDTH="10" ALIGN="CENTER" NOWRAP><IMG
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WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img51.png"
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ALT="$\displaystyle =$"></TD>
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<TD ALIGN="LEFT" NOWRAP><IMG
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WIDTH="37" HEIGHT="45" ALIGN="MIDDLE" BORDER="0"
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SRC="img54.png"
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ALT="$\displaystyle {\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{p}}}}{{\ensuremath{\displaystyle{R_m}}}}}}};$"></TD>
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<TD WIDTH=10 ALIGN="RIGHT">
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(5.4)</TD></TR>
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<TR VALIGN="MIDDLE"><TD NOWRAP ALIGN="RIGHT"><IMG
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WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img55.png"
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ALT="$\displaystyle o_m$"></TD>
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<TD WIDTH="10" ALIGN="CENTER" NOWRAP><IMG
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WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img51.png"
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ALT="$\displaystyle =$"></TD>
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<TD ALIGN="LEFT" NOWRAP><IMG
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WIDTH="109" HEIGHT="53" ALIGN="MIDDLE" BORDER="0"
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SRC="img56.png"
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ALT="$\displaystyle \Phi_m-{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyl...
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...\frac{{\ensuremath{\displaystyle{D_m}}}}{{\ensuremath{\displaystyle{R_m}}}}}}}.$"></TD>
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<TD WIDTH=10 ALIGN="RIGHT">
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(5.5)</TD></TR>
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</TABLE></DIV>
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<BR CLEAR="ALL">
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Conversely,
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<BR>
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<DIV ALIGN="CENTER">
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<!-- MATH
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\begin{eqnarray}
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\Phi_m&=&o_m+{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{180}}}}{{\ensuremath{\displaystyle{\pi}}}}}}}c_mk_m;\\
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R_m&=&{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{p}}}}{{\ensuremath{\displaystyle{k_m}}}}}}};\\
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D_m&=&c_m p.
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\end{eqnarray}
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-->
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<TABLE CELLPADDING="0" ALIGN="CENTER" WIDTH="100%">
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<TR VALIGN="MIDDLE"><TD NOWRAP ALIGN="RIGHT"><IMG
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WIDTH="28" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img57.png"
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ALT="$\displaystyle \Phi_m$"></TD>
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<TD WIDTH="10" ALIGN="CENTER" NOWRAP><IMG
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WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img51.png"
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ALT="$\displaystyle =$"></TD>
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<TD ALIGN="LEFT" NOWRAP><IMG
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WIDTH="115" HEIGHT="50" ALIGN="MIDDLE" BORDER="0"
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SRC="img58.png"
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ALT="$\displaystyle o_m+{\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{180}}}}{{\ensuremath{\displaystyle{\pi}}}}}}}c_mk_m;$"></TD>
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<TD WIDTH=10 ALIGN="RIGHT">
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(5.6)</TD></TR>
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<TR VALIGN="MIDDLE"><TD NOWRAP ALIGN="RIGHT"><IMG
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WIDTH="29" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img59.png"
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ALT="$\displaystyle R_m$"></TD>
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<TD WIDTH="10" ALIGN="CENTER" NOWRAP><IMG
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WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img51.png"
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ALT="$\displaystyle =$"></TD>
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<TD ALIGN="LEFT" NOWRAP><IMG
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WIDTH="33" HEIGHT="45" ALIGN="MIDDLE" BORDER="0"
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SRC="img60.png"
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ALT="$\displaystyle {\ensuremath{\displaystyle{\frac{{\ensuremath{\displaystyle{p}}}}{{\ensuremath{\displaystyle{k_m}}}}}}};$"></TD>
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<TD WIDTH=10 ALIGN="RIGHT">
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(5.7)</TD></TR>
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<TR VALIGN="MIDDLE"><TD NOWRAP ALIGN="RIGHT"><IMG
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WIDTH="30" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img61.png"
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ALT="$\displaystyle D_m$"></TD>
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<TD WIDTH="10" ALIGN="CENTER" NOWRAP><IMG
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WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img51.png"
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ALT="$\displaystyle =$"></TD>
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<TD ALIGN="LEFT" NOWRAP><IMG
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WIDTH="36" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
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SRC="img62.png"
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ALT="$\displaystyle c_m p.$"></TD>
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<TD WIDTH=10 ALIGN="RIGHT">
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(5.8)</TD></TR>
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</TABLE></DIV>
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<BR CLEAR="ALL">
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Thattil Dhanya
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2018-09-28
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