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Figure: Example of typical energy level diagrams for PHOENIX model atoms
\begin{figure} \psfig {file=All-Grots.ps,width=\hsize,clip=,angle=0} \end{figure}


 
Figure: Flowchart 1
\begin{figure} \psfig {file=flow1.ps,width=\hsize,clip=,angle=0} \end{figure}


 
Figure: Flowchart 2
\begin{figure} \psfig {file=flow2.ps,width=\hsize,clip=,angle=0} \end{figure}


 
Figure: Flowchart 3
\begin{figure} \psfig {file=flow3.ps,width=\hsize,clip=,angle=0} \end{figure}


 
Figure: Scalability of line calculation (non PIOFS).
\begin{figure} \psfig {file=lte.fig.ps,width=\hsize,clip=,angle=90} \end{figure}


 
Figure: Scalability of nova models using cluster technology.
\begin{figure} \psfig {file=nova.ps,width=\hsize,clip=,angle=90} \end{figure}


 
Figure: Scalability of supernova models using cluster technology.
\begin{figure} \psfig {file=sn.ps,width=\hsize,clip=,angle=90} \end{figure}


 
Figure: Scalability of static models (compute & memory intensive) using cluster technology.
\begin{figure} \psfig {file=static.ps,width=\hsize,clip=,angle=90} \end{figure}


 
Figure: Results for the Sun.
\begin{figure} \psfig {file=sun-details.ps,width=\hsize,clip=,angle=90} \end{figure}


 
Figure: Results for Vega.
\begin{figure} \psfig {file=vega-special.ps,width=\hsize,clip=,angle=90} \end{figure}


 
Peter H. Hauschildt
4/27/1999