%\mag 2074
\input www2.lt
%1/2.487=0.4020908725
%1/2.074=0.4821600771
%\textheight=0.4822\textheight
%\textwidth=0.4822\textwidth


\Large \sffamily
\ifthenelse{\boolean{BlackPage}}
           {\newcommand{\cole}{\color{white}}}
           {\newcommand{\cole}{}}

\vspace*{\fill}



\pht=600
\yi=270 \xi=210
\standardhyphens

\newcommand{\colb}{\color{black}}
\newcommand{\gwp}[1]{& \colb #1}

\begin{center}


\ifthenelse
 {\boolean{BlackPage}}
 {\pagecolor{black}}
 {}
\color{textgr}
%\renewcommand{\colb}{\color{white}}
\renewcommand{\gwp}[1]{& \colb #1}


\vspace*{\fill}
{\huge P��m�si, kter� pohlcuj� infra�erven� z��en�} \\
   {\LARGE \cole(sklen�kov� plyny)} \\[3mm]
\begin{tabular}{cccc}  % Skl. plyny s ��innost�
 \hline
\\
     &   &\LARGE   pod�l na objemu  &\LARGE  \colb relativn� \\
     &    &\LARGE  / 1 \%           &\LARGE  \colb ��innost
 \\[3mm] \cline{3-4} \\
\parbox{2cm}{\cright{}{}{\O}{S}{\H}{S}{\H}} &\LARGE  vodn� p�ra
 &\LARGE  0,2 -- 3 \gwp{\LARGE 1}\\
\parbox{2cm}{\cright{}{}{\C}{D}{\O}{D}{\O}} &\LARGE  oxid uhli�it�
 &\LARGE  0,036 \gwp{\LARGE \bfseries 1}\\
\parbox{2cm}{\cbranch{\H}{S}{\H}{S}{\C}{S}{\H}{S}{\H}} &\LARGE  metan
 &\LARGE  0,000 2 \gwp{\LARGE 21}\\
\parbox{2cm}{\cright{}{}{\O}{S}{\N}{S}{\N}} &\LARGE  oxid dusn�
 &\LARGE  0,000 03 \gwp{\LARGE 310}\\[3mm]
 \hline\\%[5mm]

\end{tabular}

{\colb Relativn� ��innost}
%\emph{Relativn� ��innost}
 je zv��en� �hrnu energie dopadl� na povrch Zem�
za sto let \\
v~pom�ru ke zv��en� p�soben�mu stejn�m objemem \C\O_2.

%\vspace*{\fill}

\end{center}

\end{document}

