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\begin{document}

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\fbox{
\parbox[t]{5cm}{
{\large {\bf Agenda}}\\[2mm]
Charissa Group Meeting
}}\\[7mm]
\makebox[3.5cm][l]{To be held on:} 25 November 1992, 11.30 am\\[2mm]
\makebox[3.5cm][l]{To be held at:} York\\[2mm]
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\psfig{figure=char-encap.ps,height=3cm}}\\ [1mm]

\noindent
Distribution: \parbox[t]{12cm}{
WNC,NMC,RAC,BRF,GJG,SJAH,RAH,JSL,ACM,\\VP,WDMR,GT,RPW,DLW\\
}%\\[2mm]

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\begin{center}
%{\large {\bf Agenda}} \\[0.5cm]
\begin{tabular}{l@{\hspace{1cm}}l@{\hspace{1cm}}l}
1.  & Minutes of Meeting of 7 October 1992            &   \\   [1.5mm]
 
2.  & Matters Arising/ Actions                       &   \\   [1.5mm]
 
3.  & Update on NSC/SERC matters                    & (DLW) \\   [1.5mm]
 
4.  &  Progress  on silicon detectors                 & (BRF) \\   [1.5mm]
 
5.  & Progress  on scintillators              & (NMC) \\   [1.5mm]
 
6.  & Progress  on chamber \&  detector assemblies          & (JSL) \\   [1.5mm]
 
7.  & Progress  on gas  supply   & (RAC) \\   [1.5mm]
 
8.  & Progress  on electronics \& data acquisition         & (RAH)  \\   [1.5mm]
 
9.  & Developments on hybrid detectors               &  (RAC) \\   [1.5mm]
 
10.  & Developments on event manager \& GEC emulator &   (VP) \\   [1.5mm]
 
11.  & Documentation of Experimental Setup    & (BRF) \\   [1.5mm]
 
12.  & Completion of Programme at NSF    & (BRF) \\   [1.5mm]
 
13.  & Responsibilities for ANU Preparation    & (BRF) \\   [1.5mm]
 
14.  & Student Training    & (DLW) \\   [1.5mm]
 
15.  & Future of DL Detector Laboratory    & ~ \\   [1.5mm]
 
16.  & Disposal of NSF radioactive sources    & ~ \\   [1.5mm]
 
17.  & Disposal of NSF ``minor'' equipment    & ~ \\   [1.5mm]
 
18. & Any other business                            &  ~ \\   [1.5mm]
 
19. & Date of next meeting                          &  ~\\
 
\end{tabular}

%\mbox{}\\[7mm]
\noindent
W.N. Catford (Secretary)\\
18 October 1992

\end{center}

\newpage


{\bf Item 11: Documentation}\\[1mm]

From BRF:

At the recent run (\mg + \mg ) it became clear that we need to collect
together and update the documentation on Charissa experiments
and make it available to all.   We have had information available
in the past, but it has been prepared on a rather {\it ad hoc} basis
and not everyone has received copies.   With the large number
of new people joining the collaboration, and the addition of 
new equipment (gas detectors and strip detectors) there is a need
to prepare an up-to-date and comprehensive set of notes covering
all aspects of the experiments.   This will be particularly useful
for those out at the ANU during the setup phase.

I would like to see a single manual containing sections on all
areas of the experiment.  A copy would be available for every
member of the group.

A suggested contents list is:
\begin{itemize}
\item {\it Chamber:} beamline, collimation,detector mounts, cables,
		chamber control
\item {\it Electronics:} setups for strip-strip runs and hybrid-hybrid runs
\item {\it Data Acquisition:} hardware setup and software control
\item {\it Running:} checklist of proceedures (stages to go through pre-beam,
             during calibration runs and during reaction runs)\\[1mm]
\end{itemize}


ACTION:  Discuss this.  Agree contents.  Delegate people to produce
           drafts.  

Set timetable.  (WDMR has already agreed to do 2)\\[3mm]

{\bf Item 12: Completion of Programme at NSF}\\[1mm]

From BRF:

It now appears likely that we will be able to fit in
two more runs on the NSF before it closes (with a few
extra shifts added to each run for detector tests).  At
present we have four approved experiments:

  Seven alpha chain state

  High resolution run

  Angular distribution measurement

  C---C* decay search

\noindent
and we need to decide which to plan for.   One of the main
considerations is to ensure everyone (esp.\ students) has
data to work on between March and September (when we run
at the ANU).

This year we have had new students starting at York (Steve
Chappel), Surrey (Steve Singer) and Birmingham (Neil Curtis)
as well as a new RA at Birmingham (Roger Ward).   Steve Chappel
will have the Orsay experiment to plan for and analyse, and
Steve Singer has started on the analysis of the \cc +\mg\  experiment.
I would suggest, therefore, that we run the high resolution
experiment for Neil Curtis and the C---C* search for Roger Ward.

The alpha chain experiment and the angular distribution measurement
then form the basis of our first running period at the ANU (plus
any other experiments which arise between now and then).

There is likely to be a recommendation to the scheduling committee
that Charissa be given priority for any additional NSF time (for
example if an experiment fails or if the machine performs
better than anticipated).  We need to be ready to step in with
another run and should decide which to go for.\\[1mm]

ACTION:  Discuss these suggestions and agree action.\\[3mm]


{\bf Item 13: Responsibility for ANU Preparations}\\[1mm]

From BRF:

A number of things need to be done in preparation for
our running at the ANU.   The jobs at the moment are as listed
below, but more will undoubtedly arise in the following
months.
\begin{enumerate}
\item  New detector mounts and collimation for chamber
\item  New chamber feedthroughs
\item  New cable runs from chamber to control room
\item  Electronics and DA shipped out and installed
\item  Beamline acquired and shipped out.
\end{enumerate}

In order to ensure these are carried out it would
seem sensible for one group to take responsibility
for a particular job. I would offer the following suggestions:
\begin{enumerate}
\item  York (machine shop personel)
\item   York (ditto)
\item   Surrey (most familiarity with layout)
\item   Birmingham/Oxford (Experience in shipping and setting up)
\item   Birmingham (ditto)
\end{enumerate}


ACTION:  Discuss these ideas.  Identify any other jobs.
         Agree responsibilities.  

 Agree completion dates.



\end{document}

