
\section{Schedule} 


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\noindent This section lists all the variables which are assigned storage by thorn WVUThorns/FishboneMoncriefID.  Storage can either last for the duration of the run ({\bf Always} means that if this thorn is activated storage will be assigned, {\bf Conditional} means that if this thorn is activated storage will be assigned for the duration of the run if some condition is met), or can be turned on for the duration of a schedule function.


\subsection*{Storage}

\hspace{5mm}

 \begin{tabular*}{160mm}{ll} 

{\bf Always:}&  ~ \\ 
 ADMBase::metric[metric\_timelevels] ADMBase::curv[metric\_timelevels] ADMBase::lapse[lapse\_timelevels] ADMBase::shift[shift\_timelevels] & ~\\ 
~ & ~\\ 
\end{tabular*} 


\subsection*{Scheduled Functions}
\vspace{5mm}

\noindent {\bf HydroBase\_Initial} 

\hspace{5mm} fishbonemoncrief\_et\_grhd\_initial 

\hspace{5mm}{\it set up general relativistic hydrodynamic (grhd) fields for fishbone-moncrief disk } 


\hspace{5mm}

 \begin{tabular*}{160mm}{cll} 
~ & Language:  & c \\ 
~ & Reads:  & grid::x(everywhere) \\ 
~& ~ &grid::y(everywhere)\\ 
~& ~ &grid::z(everywhere)\\ 
~ & Type:  & function \\ 
~ & Writes:  & admbase::alp(everywhere) \\ 
~& ~ &admbase::betax(everywhere)\\ 
~& ~ &admbase::betay(everywhere)\\ 
~& ~ &admbase::betaz(everywhere)\\ 
~& ~ &admbase::kxx(everywhere)\\ 
~& ~ &admbase::kxy(everywhere)\\ 
~& ~ &admbase::kxz(everywhere)\\ 
~& ~ &admbase::kyy(everywhere)\\ 
~& ~ &admbase::kyz(everywhere)\\ 
~& ~ &admbase::kzz(everywhere)\\ 
~& ~ &admbase::gxx(everywhere)\\ 
~& ~ &admbase::gxy(everywhere)\\ 
~& ~ &admbase::gxz(everywhere)\\ 
~& ~ &admbase::gyy(everywhere)\\ 
~& ~ &admbase::gyz(everywhere)\\ 
~& ~ &admbase::gzz(everywhere)\\ 
~& ~ &hydrobase::vel(everywhere)\\ 
~& ~ &hydrobase::rho(everywhere)\\ 
~& ~ &hydrobase::eps(everywhere)\\ 
~& ~ &hydrobase::press(everywhere)\\ 
\end{tabular*} 


\vspace{5mm}

\noindent {\bf CCTK\_INITIAL} 

\hspace{5mm} fishbonemoncrief\_et\_grhd\_initial\_\_perturb\_pressure 

\hspace{5mm}{\it add random perturbation to initial pressure, after seed magnetic fields have been set up (in case we'd like the seed magnetic fields to depend on the pristine pressures) } 


\hspace{5mm}

 \begin{tabular*}{160mm}{cll} 
~ & After:  & seed\_magnetic\_fields \\ 
~ & Before:  & illinoisgrmhd\_id\_converter \\ 
~ & Language:  & c \\ 
~ & Type:  & function \\ 
\end{tabular*} 



\vspace{5mm}\parskip = 10pt 
