----------------------------------------- Hall A CC Meeting Minutes - March 17 2000 ----------------------------------------- Present: Kees de Jager, Ron Ransome, Ed Brash By Conference Phone: Christian Cavata, Franco Garibaldi 1. Status Report - Kees de Jager -------------------------------- The decision was made March 16th to delay the installation of the septum magnets until July/August, 2001. The reason was based on delays that have been experienced by the company manufacturing the magnets. Paul Brindza, who is the JLab contact person for the magnets, felt that it was unlikely that the company would be able to deliver the magnets in time for the originally scheduled February/March, 2001 installation. Thus, the schedule for 2001 has been adjusted as follows: Jan 2001 - mid Feb - Run Gao/Holt gamma + n --> pi- p mid Feb - March 5 - Run Markowitz/Baker/Garibaldi Kaon production March 5 - April 5 - Install polarized 3He target April 5 - mid May - Run Meziani high X proposal mid May - end June - Run Everett/Korsch g2 higher twist proposal July - August - install septum magnets Fall 2001 - Run Hypernuclear experiments and Forward angle GDH Notes: 1. There is a possibility that during the M/B/G Kaon production time that the RICH detector could be installed. The time for this would come out of the time scheduled for this experiment. Also, the kinematics during this period are limited due to the strict requirements of Gen in Hall C. 2. The March 5 - April 5 period is set to coincide with the end of Gen in Hall C, and thus is essentially a hard limit. 3. For 2002, two scenarios were offered: (i) leave the septa installed, and run Happex II and Pb-parity immediately. (ii) remove the septa, installed the real photon calorimeter, and run RCS and perhaps some other experiments, and then reinstall the septa in summer 2002 to run Happex II and Pb-parity. Kees noted that G0 in Hall C might be expected to run in Summer 2002, and there may be concerns with accelerator being able to provide to two parity experiments running simultaneously. This may be a factor which weighs heavily in the decision on how to proceed in 2002 in Hall A. The final design review for the septum magnets is expected during the summer of 2000, and will only proceed once certain milestones are met, specifically the manufacturing of the first magnet, and its fitting in the yoke. The present experiment is running smoothly, and there is a good probability that they will finish the program of measurements by the end of the scheduled beam time. For summer 2000, there are three important things scheduled for the shutdown in Hall A: (i) swapping of detector stacks necessary for Gep-II (ii) replacing an upstream girder which will be necessary for septum magnets. (iii) install a new heat exchanger in order to be able to run the He target with high current. 2. Jeopardy Proposals ---------------------- The CC discussed the possibility of allowing jeopardy experiments to submit essentially their original proposals with a short update for collaboration approval, if the spokespeople wished to do this. The CC unanimously agreed that this would not be acceptable, and strongly recommends that all of the proposals which will be reviewed for the upcoming PAC should be in their essentially final form at the time of submission. The CC agreed that due to the large expected number of proposals, and hence the large number of reviewers that would be necessary, that individual members of the collaboration may simply be "assigned" proposals to review, rather than trying to solicit volunteers. Kees informed the CC that at current count, including conditionally approved experiments, that there may be as many as 16 proposals which fall under jeopardy. Presumably, these would be spread evenly across the next two PACs, meaning that as many as 8 jeopardy proposals could be assigned to the summer 2000 PAC. The current estimate is that each of the next two PACS will have approximately 120 days of beamtime to assign. Kees reminds that if not all of this time is allotted at the summer 2000 PAC, it will NOT be carried over to the winter 2001 PAC. 3. Next Collaboration Meeting ------------------------------- The dates are set for May 18-20, with the possibility of extending to the 21st if necessary. The CC felt that having scheduled meetings in the evenings was not a good idea since it made for too long a day. The upcoming meeting will focus largely on proposal reviews, the 12 GeV upgrade, and the working group meetings. The CC discussed the perhaps unsuccessful attempt that was made at the last collaboration meeting to focus on problems and future developments, rather than past accomplishments in the presentations. For the upcoming meeting, the session coordinators will be strongly encouraged to allow for significantly more time for discussion periods, as opposed to presentations. The CC would like to see the meeting be more of a workshop on new ideas, that than a conference presenting accomplishments. For the 12 GeV upgrade portion of the workshop, as a suggested avenue to pursue, Kees gave some details on a new spectrometer design, being worked on currently by J.P. Chen, John Lerose, and Paul Brindza. This spectrometer, known as the Medium Acceptance Device, or MAD, would be a device capable of +/-15% deltap/p, with 30msr acceptance, 25 degree bend angle, and capable of 6 GeV/c. Given that the deadline of submission of new proposals for Hall A review is April 22nd, about 4 weeks before the meeting, the decision was made to wait until after the submission deadline to publish a firm schedule for the meeting. That is, we will wait until we see exactly how many proposals we are getting before fixing the schedule. The CC notes that the annual Users' Group Meeting is set for June 21-23, 2000. We need to discuss and finalize what will be presented from Hall A at this meeting during the collaboration meeting. 4. CC Elections ---------------- The CC will hold elections as soon as possible for the two members that will be replaced. The usual e-mail voting procedure will be followed. An open discussion on the expected participation of CC members was held. In the end, it was felt that an elected CC member should certainly be expected to attend both collaboration meetings, and the associated CC meetings, each year. In addition, the member should be expected to attend at least one of the other two CC meetings annually. In soliciting nominations, the CC will attempt to make this policy clear to the collaboration. 5. Technical Publications -------------------------- At the last CC meeting, it was encouraged that the collaboration should endeavour to publish technical (NIM) articles on the Hall A instrumentation. In a recent JLab Hall A staff meeting, it was agreed that the staff would begin work on a general paper on the Hall A instrumentation. The goal is to have an outline submitted by each staff member by April 1, a draft paper by July 1, and to submit the paper for publication by October 1. Kees notes that the author list for this paper will be very open, including technicians and any others who have made significant contributions to the Hall A instrumentation. In addition, there will also be technical papers on individual instrumentation systems (Compton, Moller, FPP, VDC, etc.). The CC feels that these papers need not contain the entire collaboration as authors, but rather should only list those who made a significant contribution to those specific systems. Also, the CC feels that commissioning data could and should certainly be included and that the authors should acknowledge the collaboration in obtaining the data used for commissioning. 6. Other Business ----------------- J.P. Chen has requested the 97-110 (small angle GDH) be accepted as a Hall A collaboration experiment. This was unanimously endorsed by the CC. The Glasgow group (G. Rosner + 5 other researchers) has requested membership in the Hall A collaboration. Because of a funding proposal by this group, in which they wish to mention the Hall A program and their membership explicitly, the CC recommends that an e-mail vote be carried out as soon as possible, rather than waiting for the next collaboration meeting. Ransome will organize this in the next few days. Kevin Fissum has resigned as chair of the Many-Body Working Group. Kees notes that there is already a correlations working group, and the issue of whether to continue a separate many-body working group should be decided at the next collaboration meeting. The CC discussed briefly the notion of requiring certain numbers of shifts per year from either individuals in the collaboration, or from institutions in the collaboration, as is the practice in Hall B, for example. At this time, it was felt that while some longer experiments have difficulty in filling shifts, especially as the experiments draws to a close, that this practice is not necessary in Hall A. Kees informed that the DOE has instituted significant cuts to travel budgets, both for staff members and for visiting users. As a result, JLab may not be able to conform to some of its MOU commitments in this area. The effects particularly the French and Italian groups. Kees also pointed out that stipends (currently $74.50 per day for hotel and food) are not subject to the DOE cuts, and may be an alternative. Office space allocation is now being handled entirely through the user liaison office. Kees notes that if any users feel that they have been treated very unfairly and unjustly with respect to assignment of office space, that they should be encouraged to contact him directly. It is current practice at JLab that once experiments are finished the data analysis of an experiment, that they should present a seminar on the results of the analysis at JLab prior to the submission of a paper. It was noted that this applies to the first publication of the experiment, and would not apply to subsequent longer physics papers or technical publications. The issue of graduate students from out of state being able to take courses at local universities during extended stays is currently being discussed by the Users' Group BOD and JLab management. There is no firm decision as of yet.