Minutes of HERA/Experiment Coordination
Meeting 30.11.2004
Agenda
- Brief summary reports
- Schedule and operation
- machine studies
- luminosity operation Dec04/2005
- operation over Christmas and new year holidays
- Shutdown plans (What is the earliest date?
When do we have to fix the date?)
- Polarization Task Force
- Date of next meeting
- AoB
Minutes:
- The re-commissioning schedule was kept until 11.11.2004 when a GN magnet
coil was severely damaged. Six working days were needed to replace
the defective magnet. Further problems were: ground fault of a QQ
magnet east left, vacuum leak at a new proton beam position monitor,
several water leaks and network problems. There is now a 5 to 7 day
delay in the schedule.
- Staging the switch to electrons was very successful. Electron beam
was stored within 2 hours. The beam optics was checked and
empirically corrected. A concern is the electron injection efficiency,
which will be more important if the luminosity lifetime is lower
with electrons instead of positrons. There are indications for a
large optical mismatch between the electron transfer beam line and
HERA. This has to be improved.
- Beam-based alignment studies were performed. Everything looks fine in the
south IP. An additional 2mrad orbit kick is needed in the north IP.
This could
be explained by a 7-10 mm misplacement of the GO magnet at the
IP side. A 30% stronger dipole field (GG magnet) is needed to
correct for this. Trying to move the GO magnet by 7mm on Friday failed.
GO hit the H1 cryostat after 1mm movement.
There will be a meeting this afternoon to discuss
whether the H1 detector will be moved by 5mm. If yes, it will be
done tomorrow or on Thursday.
- The sensitivity of the new temperature sensors at the GI vacuum
chambers was checked with electron beam. The south IR looks
fine. The space for vertical bumps is very limited in the north IR.
More studies are needed.
- The present schedule is:
- Complete beam-based alignment and temperature studies.
- Set up luminosity running.
- Start luminosity run end of this week.
- Maintenance day 8.12.2004
- Christmas break 23.-27.12.2004
- There have been quite a number of problems with normal conducting magnets
in HERA.
- All coils of the QS and QR magnets were already exchanged sometime
ago.
- Two BU magnet developed ground faults. Six BU coils were
exchanged during the last shutdown. All had water leaks.
It is possible that all other BU coils will fail sooner of later.
During operation one ground fault can be tolerated by shifting the
ground of the electrical circuit. Operation would not be possible in
case of a second short. 24 further spare coils were therefore ordered.
Delivery is scheduled to start in May 2005. 13 coils should be here
by July, the rest until the end of 2005.
Replacing one magnet would take about 10 days, without moving HERMES
if necessary. Exchanging all magnets in one section would require
about 4 weeks. So far there are no
concrete plans which coils will be replaced first.
- Two QC magnet have failed so far (1996 and 2001). 12 spares are
available.
- One GN magnet (vertically focusing proton septum quadruple with very
high field) failed last month due to insufficient water cooling.
It is not clear why the cooling was interrupted. No anomalies have been
found so far. The failure occurred during tests at the maximum
current of 1600A. The current of the power supply is now limited to
1400A. In case of another failure there is a spare set of coils,
no complete magnet.
- Ground faults have appeared at several QQ magnets (super-ferric proton
correction quadrupoles). A possible cause for the shorts is
radiation damage of the wiring boxes. Usually the shorts did not
happen during luminosity operation, only when the magnets are
run at higher current during the cycling procedure, Some of the
defective quads are already connected to ground free power supplies.
The remaining power supplies will be installed during the maintenance
day 8.12.2004.
- From the machine point of view the preferred date of the 2005
shutdown is after the summer school vacation, i.e. starting middle
of August. The annual interlock tests have to be done.
- The detector is ready for data taking. All components are operational
except the STT. Two hours without beam are still needed every
week for calorimeter calibration.
- Large background spikes have been observed, mainly at injection.
The dark current of the radiation monitor has increased. HERA should
not continue injecting if the efficiency is very poor.
- ZEUS is prepared to take data over New Year. Shifts will stop 23.12. and
will continue 27.12.2004.
- The cooling of the STT is insufficient. Temperature changes in the
safety volume, switching the STT on or off, lead to temporary leaks
in the insulation vacuum of the solenoid, and were causing magnet
discharges during the last running period. Removal of the STT for
improving the cooling and tightening of the insulation vacuum
flange is planned for the next shutdown.
Using the present installation fixtures removal and re-installation
of the STT would take 4 months, requiring opening of the vacuum
system and removal of the GO and GG magnets. A new installation
jig is in preparation, which allows to slide the FDET over the GO
magnet. The main challenge will be to guarantee that the central
beam pipe will not be damaged. A repair should be possible within
7 weeks. The plan is to be ready in May 2005 in case of an early
shutdown.
- The backward and forward silicon detectors were removed during the
shutdown. The central silicon detector is fully operational.
The most radiation sensitive electronics is now the CIP readout.
A new radiation monitor (scintillation counter) was installed. It has
to be calibrated. Shifts started 29.11.2004. Flammable gases for
tracking detectors will be ready early next week.
- The position of the GO magnet towards the IP is only known to about 5mm.
The whole detector is about 5mm too far ring inwards. The GO tip
could only be moved by 1mm last Friday until it hit the cryostat.
In principle the H1 detector can be moved horizontally by 5mm. This
will take a full day.
- The base pressure at NR6m is presently 10**-8 mbar. An improvement
of 2 orders in needed in order to operate the tracking detectors.
Beam currents must be limited to prevent radiation damage of the
CIP electronics. Dedicated electron beam bake-out might accelerate
the vacuum conditioning. It is not requested now.
- H1 will be operated over New Year if some reasonable data taking can
be expected.
- The FST and BST repair plan aims for installation in early
September 2005. The shutdown should start 1 week earlier and should
last 6 weeks if there is no further repair work.
Milestones of the FST/BST repair should be presented and reviewed
regularly.
- Maintenance work was performed during the shutdown. The spectrometer
and DAQ are fully operative. Shifts started yesterday. No dramatic
background spikes have been observed during injection.
The LPOL calorimeter has not yet been installed to prevent
radiation damage. Installation will take a few hours.
Christmas break: shifts will stop 20.12. and restart 29.12.2004.
- The preferred beginning of the 2005 shutdown is middle on July to
mid August, total length of 6 weeks. An earlier shutdown will cut
into the physics program.
- The low polarization compromises the HERMES physics program.
A polarization task force is strongly required.
- Several glass dissociator tubes broke last year. The dissociator tube
will now be replaced during every monthly maintenance day.
- There were no major modifications of the polarimeters during the
shutdown. A short access is required of reinstall the LPOL calorimeter.
- The serious problem with the LPOL cavity during the last running
period are hopefully solved. Shielding was installed. The electronics
was move to a radiation safe location. All damaged components were
repaired. The cavity was locked successfully during the shutdown.
Commissioning the cavity with beam will take a few weeks.
- The design of the new radiation hard calorimeter is almost finished.
A brief note on the design should be distributed. Fabrication of the
calorimeter will start early next year.
Polarization "Task Force"
- Several members of the experiments (HERMES, ZEUS and polarimeters) are
interested to get involved in improving polarization. A list of items,
including simulation of polarization tuning, beam based alignment and
depolarization, will be prepared. Ties Behnke will organize a meeting.
Ferdi Willeke asked about the priorities and whether dedicated
machine time should be spent on polarization tuning.
Schedule
- Complete beam-based alignment and temperature studies.
- Set up luminosity running.
- Start luminosity run end of this week.
Luminosity operation until 20.12.2004
- Maintenance day 8.12.2004
- Machine studies 20.-23.12.2004
- Christmas break 23.-27.12.2004
- Resume luminosity operation 27.12.2004
Date of next meeting
The date of the next coordination meeting is Tuesday, 11.01.2005 10:00hrs,
building 30b room 459.
Uwe Schneekloth