M. Begemann-Blaich, A. Ferrero (since 14:25), S. Fritz, C. Groß,
X. Hongfei, U. Kleinevoß, M. Mahi, T. Odeh, J. Pochodzalla,
C. Schwarz, V. Serfling, W. Trautmann (since 14:25), Andrzej Trzcinski,
B. Zwieglinski.
Topics:
1. Setup:
A Picture of the setup for the people
who are not so familiar with the experiment.
2. ZDO:
The channels are tested, broken cables are changed, one Pm has to be exchanged.
A Cosmics run in vacuum is forseen, as soon as the DAQ is working.
3. Si-Strip:
3 channels on different detectors are broken and have to be repaired. Givoanni
will bring 4 additional Si-Strip detectors.
4. Catania:
3 channels do not work, 8 channels are noisy.
5. TOF:
A second cooling circuit for the TOF will be installed. Some broken cables have
to be soldered.
6. MSU:
The hodoscope chamber will be opened today. The misalignment of the angle has
to be adjusted. An additional NIM crate forr the bias is needed in the hut.
7. Scattering chamber:
The vacuum was better than 10^-4 without using the kryostatic pump.
8. General discussion:
The alignment of the chamber will be done after the MSU hodoscope is mounted in
the chamber again (Thursday morning).
For every detector group a written manual has to be provided until the start of
the experiment. The detector and the general logbooks have to be kept in the
hut and not at home!