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SCT Operation in 2008 - an eventful year of commissioning and first running -. Early Commissioning and Detector Sign-off…………2 First SCT Run in ATLAS……………………………….4 Commissioning without cooling……………………….7 Barrel sector in SR1……………………………………10 Training………………………………………………….13 - PowerPoint PPT Presentation
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A. Ciocio LBNL ATLAS Meeting - Jan 2009 1
SCT Operation in 2008- an eventful year of commissioning and first running -
1. Early Commissioning and Detector Sign-off…………2
2. First SCT Run in ATLAS……………………………….4
3. Commissioning without cooling……………………….7
4. Barrel sector in SR1……………………………………10
5. Training………………………………………………….13
6. Preparation for Beam…………………………………..14
7. First Beam……………………………………………….17
8. Run with Cosmics ……………………………….….…25
9. Final Calibration …………………………………….…43
10. Schedule - plan for 09 ……………………………..…50
A. Ciocio LBNL ATLAS Meeting - Jan 2009 2
• Barrel signed-off (May) - 5 days commissioning until cooling heaters failure
• Cooling crises: heater repair, extension of pipes to make heaters accessible• Integration in ATLAS central of DAQ ,DCS, Monitoring and run with 4 SCT test modules• ROD and Power Supplies upgrades
Recap of 2007
Noise Occupancy 5.7 e-51700 ENC
All uniform across barrel
Barrel Defect channel %
Dead/noisy channels after SR1 tests 6712 0.206
2 modules lost after installation 2x1536 0.095
13 individual chips lost after installation 13x128 0.051
Total 11451 0.353
Number of defect channel / module (1module = 1536 channels)
1. Early Commissioning and detector sign-off
Avg chip noise vs chip number
Noise
Defect Channels
HV test
A. Ciocio LBNL ATLAS Meeting - Jan 2009 3
Endcap Sign-off
– Endcap A: Jan 9-20 2008
– Endcap C: Feb 8-11,2008
– One very leak loops: 13 modules • leak needs repair
– One “moderately” leaky loop • OK at low backpressure
Endcap A ENC (Temp = 25deg)Outers: 1707 eMiddles: 1653 eInners: 1149 eShort Middles: 1002 e
Endcap C ENC (Temp = 25deg)Outers: 1767 eMiddles: 1704 eInners: 1182 eShort Middles: 1013 e
Outers
MiddlesInners
Short Middles
Defect channel %
Endcap A 3960 0.26
Endcap C
+ 2 leaky loopsD9
4040
2x13 modules
0.266
2.6%
1. Early Commissioning and detector sign-off
February 15, 2008 we completed the sign-off of SCT endcaps,
officially marking the complete sign-off of whole SCT
NoiseDefect channels
A. Ciocio LBNL ATLAS Meeting - Jan 2009 4
SCT first RUN
• February 18 to 20, 2008 the SCT (barrel) pre-M6 run in ATLAS – Technical RUN mainly to verify integration and do first timing
in the ATLAS readout and control and prepare for the next ATLAS M6 combined run
– A chance to try global ATLAS integration with a large fraction of the real detector cooled and powered
– Used ROS monitoring to count module coincidences
for various timing offsets
2. First SCT RUN in ATLAS
First SCT pit cosmic on 20 Feb
A. Ciocio LBNL ATLAS Meeting - Jan 2009 5
M6 Run
• In M6 (March) first operation of SCT in combined ATLAS run
– TRT scintillator trigger + RPC– Operation was limited to Barrel by the number
of compressors available in the cooling plant– 3 barrel cooling loops off
(3x48 modules out of 2112)because running “warm” at high back pressure and these loops have small leaks
– Detector operation and Evaporative Cooling/Heater stable for whole period (24 hour operation)
– All RODs and HV/LV Power Supplies were available– One day standalone running to test ROD firmware upgrade– Online monitoring including DQMF– First check of the OFFLINE/Alignment algorithms– Few “noisy” module observed in M6 due to individual noisy strips not masked and
occasional HV trips
2. SCT First RUN2. First SCT RUN in ATLAS
A. Ciocio LBNL ATLAS Meeting - Jan 2009 6
Tracks reconstructed in SCT
• ID + RPC tracks
SCT residuals (No Alignment applied)~ 5000 tracksSCT residuals (GlobalChi2) ~65mCompares well with results from SR1
2. First SCT RUN in ATLAS
A. Ciocio LBNL ATLAS Meeting - Jan 2009 73. Commissioning without Cooling
Cooling Plant Failure May 1st, 2008
• 3 of 6 compressors damaged due to prolonged slippage of magnetic coupler between compressor section and motor
– In case of slippage for a long time, Eddy currents will heat inner metallic parts and damage (decompose, break) neighboring plastic parts.
– In addition excessive wear on piston rings was found
• As a result the C3F8 and plant was contaminated by both the incident and, over a longer period of time, by the wear of piston rings
– Subsequent analysis of samples indicated that the part of the plant in UX15 was not exposed to pollution coming from the accident.
– ~100-200 kg C3F8 were lost
– New C3F8 (1000kg) was received and additional 1000kg have been ordered
• The damaged compressors were repaired by Haug– The other 3 were cleaned and checked in-situ
• Implementation of the measures that would protect the system– An additional buffer tank was installed to prevent any loss of C3F8
– Compressors equipped with slippage sensors. The PLC will then stop a compressor if it starts to slip
– New mechanical filters needed to be installed, to protect the plant from the debris emitted from the piston rings and isolate the distribution racks (and the silicon detectors)
– Regular maintenance to replace piston rings (~1000hrs interval)
A. Ciocio LBNL ATLAS Meeting - Jan 2009 8
Crack in the crank cover (puts clean and dirty part of the
circuit in contact)
Burnt plastics, main source of pollution
Magnetic Coupling Motor 1450 RPM
Damaged parts
3. Commissioning without Cooling
A. Ciocio LBNL ATLAS Meeting - Jan 2009 93. Commissioning without Cooling
SCT Commissioning without Cooling: Off-Detector
• HV communication error (bad current readings) that was causing fake HV trips– Often occurs when card masked or interlocked off. Also occurs randomly, ~ 1/hour – For M6, auto recovery implemented as part of FSM– When channel is masked on to recover from the trip, neighbouring channels may start
oscillating– Power cycle all 8 channels of an HV board not possible during a run!– Had to suppress current trip in crate controller software (change thresh)
• Firmware upgrade for all boards to solve communication problem (May 19)
– Oscillation problem remains and will be solved next year with another major upgrade of the system
• Started to investigate “death of vcsels” as observed by pixel– TX vcsel array (12-way) sends optical clock and control signals to modules
• Situated in DAQ racks in USA15
– SCT barrel tests showed 5 of 1941 TX with no pin current and too low optical power– possibly related to ESD damage during production at the factory
• Since M6 had an SCT integration run in ATLAS readout ~ once/month to test new features and improvements of DAQ, DCS & monitoring chain
A. Ciocio LBNL ATLAS Meeting - Jan 2009 104. SCT Barrel Sector in SR1
SCT Barrel Sector in SR1
• Barrel sector refurbishment started at the beginning of March 2008
– 48 modules, 1 cooling loop, B3
• Cooling– Used the C3F8 cooling plant
• DAQ Software and Hardware• Detector backplane resistance tests• DCS Software Interlock and Power supply
– Environmental sensors:• 4NTCs for the cooling interlock• 10 NTCs for the mechanical and air temperature• 2 Xeritrons + 2 (HIH + NTC)s
for RH and dew point measurements
• Sector mechanics and service preparation• Reroute of cables for barrel and EC tests• Re-labeling • Fibres were disentangle• Harness installation • Plug-in• TEST
• SR1 space and cleanliness • Test box preparation
Started operation July 10
Huge involvement in the various areas of the detector construction and good opportunity for students and new post-docs to learn about SCT
Used for TRAINING and DAQ development
A. Ciocio LBNL ATLAS Meeting - Jan 2009 11
4. SCT Barrel Sector in SR1
SCT Barrel Sector in SR1
Harness testing in the box
Harness test before module mounting with loop back cards
Harness installed
A. Ciocio LBNL ATLAS Meeting - Jan 2009 12
Sector with cooling loop
•
4. SCT Barrel Sector in SR1
inlet/return side
A. Ciocio LBNL ATLAS Meeting - Jan 2009 13
Training
• SCT training started in May• By June 36 people took training courses in DCS and DAQ in ID SCR, Monitoring in ACR• Training shifts with H8 test box (4 modules)
• List of trainees• Started with residents (mostly student and post-docs)• List updated with information from GLs (in July) or directly from people
• Training Scheme and method to keep track of training progress• End of June started regular training shifts with Barrel Sector in SR1
https://twiki.cern.ch/twiki/bin/view/Atlas/SctSR1Tutorial• DCS and DAQ• 2 people/shift (4h)
• Regular Training Courses in DAQ, DCS, and DQM• 1 hour with instructors• Documentation and tutorial at:
https://twiki.cern.ch/twiki/bin/view/Atlas/SctCommissioningDocumentation
• Average time to complete training 2 weeks• Qualification overlap shift with experts going through a shift check list (later)• Training info, progress, links to documentation at:
https://twiki.cern.ch/twiki/bin/view/Atlas/SctTraining
• Started to use the ATLAS Shift Booking Tool OTP (August)
5. Training
A. Ciocio LBNL ATLAS Meeting - Jan 2009 146. Preparation for Beam
Commissioning before Beam (I)
• Cooling plant repair finished on July 14
• Needed to be able to cool down pixel for beam pipe bake-out
• No operation of SCT modules before end of bake-out
• Beam pipe bake-out successfully completed 29-31 July– This was a very tense operation - on critical path for LHC to open vacuum valves.
• ATLAS went to full shift mode on July 28
• Started of SCT commissioning with cooling on Aug 11
• Once we restarted, running the SCT colder than before, had control problems– Some loops only stable with modules powered up– Some loops also needed modules to be configured and clocking.– Restarting the system was taking long time but got better on synchronizing cooling, SCT
DCS and SCT DAQ, after many unwanted shutdowns (power cut, etc.)
A. Ciocio LBNL ATLAS Meeting - Jan 2009 156. Preparation for Beam
Commissioning before Beam (II)
• Frantic effort to get the detector into good shape before first beam– Commissioning cooling loops and basic module control on barrel and endcap– In parallel to Pixel commissioning – Started 24/7 mode (operational shifts and calibration)– Radical DAQ improvements needed completion– Intense calibration: Noise occupancy and equivalent noise charge good for most
modules– A few modules still untrimmed (EC-C) giving noisy spots
Calibration ENC noise on barrel is ~1560e- Noise Occupancy is ~4.4 x 10-5 at 150V Endcap ENC outer/middle ~1650e- Noise Occupancy outer/middle ~ 5 x10-5
Inner Modules much lower due to short strip length
• Starting Aug 29/30 had SCT on full power and started to adjust opto readout setting first on barrel then on endcaps
A. Ciocio LBNL ATLAS Meeting - Jan 2009 16
• Decided that it was safe to run the detector at 20V bias during first beam, with electronics on
– Threshold raised to 1.2fC.– Well below 100V limit above which implant damage has been observed– Lowest voltage possible where HV and DAQ stable– Hybrid experts consider LV on to be safer– Pixels stayed off
• Then we learned that first beams would be stopped just before ATLAS at the collimator
– Worries that many particles going parallel to barrel tracks could deposit even more charge (no simulation of this available)
– Reduced barrel HV to 5V and left it out of the DAQ– Endcaps set at 20V - with expected lower (and unmeasured) efficiency
Voltage setting
6. Preparation for Beam
A. Ciocio LBNL ATLAS Meeting - Jan 2009 17
September 10
• Run 87764 event 40050
7. First Beam
A. Ciocio LBNL ATLAS Meeting - Jan 2009 18
People clapping in the ACR
7. First Beam
A. Ciocio LBNL ATLAS Meeting - Jan 2009 19
People (and reporters) in the ACR
7. First Beam
A. Ciocio LBNL ATLAS Meeting - Jan 2009 20
People at the SCT desk in the ACR
7. First Beam
A. Ciocio LBNL ATLAS Meeting - Jan 2009 217. First Beam
First Beam “Splash” Event
A. Ciocio LBNL ATLAS Meeting - Jan 2009 227. First Beam
Space points in EC in one “splash”
• SCT roughly timed in to crudely optimize hit occupancy in the central time bin
• SCT can time in ‘on the fly’ - invoke SCT busy during timing adjustments
• Endcaps running at 20V
A. Ciocio LBNL ATLAS Meeting - Jan 2009 237. First Beam
SCT People in the ACR
A. Ciocio LBNL ATLAS Meeting - Jan 2009 247. First Beam
More SCT People in the ACR
A. Ciocio LBNL ATLAS Meeting - Jan 2009 25
After September 19
• With no prospect of beam, but the full ID available with cooling for the first time, everyone was very positive to start commissioning with cosmics (right away!)
– TRT just completed change to Xenon active gas– Pixels detector operational for the first time
• Started Combined ATLAS Run until 27 October (almost 6 weeks!) Alternating calibration periods
Understand of how to time-in the various ATLAS triggers, and how to synchronize the SCT
Propagate configuration and calibration results to the offline Solved several problems (ROD, TX) and calibrated the detector the best we could Had several stops due to power cuts, interventions, incidents with cooling, but we always
recovered and improved our recovery procedures Shifts were filled, training in progress and people continued to be active and involved 24/7 Lots of cosmic events, with and without solenoid on
8. Run with Cosmics
RPC: mostly “100” hits trigger arrives slightly late by ~1BC
MBTS: mostly “001” or “010” hits trigger arrives slightly early
A. Ciocio LBNL ATLAS Meeting - Jan 2009 26
Number of SCT tracks
• Over 1 million SCT tracks
• ~250 thousand tracks with at least 1 pixel hit
0
200000
400000
600000
800000
1000000
1200000
90000 90500 91000 91500 92000 92500
Run Number
N SCT tracks
All SCTTracks
solenoid off
solenoid on
8. Run with Cosmics
200K solenoid off800K solenoid on
A. Ciocio LBNL ATLAS Meeting - Jan 2009 27
Cosmic event
• Cosmic ray event
• Solenoid on
8. Run with Cosmics
A. Ciocio LBNL ATLAS Meeting - Jan 2009 288. Run with Cosmics
“Data” is taken after BCID problem fixed•“Reference” from a long run, so many modules gave BCID errors by the end
Problems solved in October (I)
• SCT efficiency degraded over the course of a run– Much more obvious as ATLAS stability improved and we recorded many-hour long runs– Observed an increasing number of L1ID and BCID errors– By the end of some runs up to ~22% of modules showed errors– Also saw a decrease in the number of tracks over time (in a run).
• Synchronization errors– Once a module got out of synch, its efficiency was zero– John Joseph (arrived on Oct 15) traced the problem
to inconsistent treatment of timeouts in the FPGA code
...…..and FIXED IT!
Before
After
A. Ciocio LBNL ATLAS Meeting - Jan 2009 298. Run with Cosmics
Problems solved in October (II)
• Already started to see signs of TX failures last July.
• The number of working TX channels had been gradually deteriorating at the rate of 2 or 3 per day, reaching ~5% dead channels at the end of October.
• Original intention was to replace the defective plugins from the batch of50 new plugins received from Taiwan, but the new plugins failed the QA at Cambridge
• Made the decision to replace TX plugins with existing (old) spares:
• Replaced 8 BOCs, 22 plugins in 17 different BOCs (completed on Nov 12)
• Work took 2 days to complete, 25 BOCs needed extraction
BPMChipBPMChip
VCSEL arrayVCSEL array
VCSEL converts electrical signal into light and sends it to the on-detector side.
BOC
A. Ciocio LBNL ATLAS Meeting - Jan 2009 308. Run with Cosmics
SCT efficiencies from later runs
• More fixes for conditions
and holes on tracks algorithms
• Apply a track incidence angle cut
• Efficiency for barrel ~99%
• More to be understood, especially for the end caps
EC A EC C
Barrel
A. Ciocio LBNL ATLAS Meeting - Jan 2009 318. Run with Cosmics
Data Quality Offline Web tools
• SCT bytestream check webpageNoise & Error Summaries
A. Ciocio LBNL ATLAS Meeting - Jan 2009 32
SCT Barrel Residuals
• SCT (Barrel) residuals ~20-30 m
8. Run with Cosmics
A. Ciocio LBNL ATLAS Meeting - Jan 2009 33
• Detector conditions– Tx replacements and fine opto-tuning
• From 200 modules to ~10• TX channel death rate still 1-2/day
– About 70 modules excluded (over 4088 - HV, LV, Ipin=0, Cooling, Misc.)• Including the 36 of ECC
– DAQ fixes• one ROD replaced• Calibration and Conditions DB
– Online monitoring• more histos• Stability
• Shifts– TDAQ Run Control tutorial (~10 people)– RPC (DCS) tutorial– RC+SL shift plan
• discussed among run coordinators• In addition to regular shifts• RC and SL shifts in OTP
– SCT Detector Operation• DAQ + DCS and DQM• DQM• On call: DAQ, DCS, DQM
8. Run with Cosmics
Preparation for ID Combined RUN (5 days - TXG WE)
Also: DSS tests as an exercise to prove that the detector and the cooling can be turned off under different circumstances
A. Ciocio LBNL ATLAS Meeting - Jan 2009 34
ID Combined Run List
8. Run with Cosmics
TRT only
TRT +RPC}
}
TRT +RPC
} TRT only
Sp
eci
al r
un
s
Recovery due to mixed-water cooling failure
Recovery due to power cut in US15
Run transition test
HV=50V
HV=20V
Bad configuration Runs
Good Run
{
A. Ciocio LBNL ATLAS Meeting - Jan 2009 35
Tracks and rates
8. Run with Cosmics
Runs with >300 time-out errors after power cut no good configuration
A. Ciocio LBNL ATLAS Meeting - Jan 2009 368. Run with Cosmics
Run 96903
• Mostly “010”
followed by “011” hits
Barrel
ECA ECC
“010”
“011”
Time Bins
Summary Time Bins
A. Ciocio LBNL ATLAS Meeting - Jan 2009 37
Mean Noise Occupancy for all runs
8. Run with Cosmics
A. Ciocio LBNL ATLAS Meeting - Jan 2009 38
Noise Occupancy (Barrel) Run 96903
8. Run with Cosmics
A. Ciocio LBNL ATLAS Meeting - Jan 2009 39
8. Run with Cosmics
Hit Efficiency
Efficiency depends on layer
ECA ECC
Barrel
A. Ciocio LBNL ATLAS Meeting - Jan 2009 40
Special Runs at 50 V and 20 V
– ~0.5% drop in efficiency for 50 V– ~37% drop in efficiency for 20 V
8. Run with Cosmics
@ 50 V
@ 20 V(1.2 fC)
(barrel 4 and disk 2)
ECCECA Barrel
A. Ciocio LBNL ATLAS Meeting - Jan 2009 41
• Detector was operated by shifters and experts on call (and present)– DAQ, DCS, and DQM tasks (in OTP) over 3 shifts: 7h-15h, 15h-23h, 23h-7h
– The last week of running these three shift tasks were merged in one: • SCT Operation task
– Plus 2-3 experts on call shifts
– Plus 1 shifter for DQM (75% of the time)
– DQ checks Offline shift 7h-15h
– Overlap shifts • qualification • before first shift period
• After Oct 27 (back to commissioning)– DCS watch shifts 24h
– Calibration (DAQ expert) day-time shift
– Daily meeting at 9h15
• Nov 26 - Dec 1 ID Combined Run– SCT Operation + DQM shifts
• Training continued until ~end of November• SR1 was unavailable “only” for 3 weeks
for cooling plant maintenance in October
All about shifts information at:https://twiki.cern.ch/twiki/bin/view/Atlas/SctShifterInfo
Shifts
8. Run with Cosmics
>5 months
Daily meetings at 15h during cosmic run (including weekends) to discuss current issues between shifts and with data quality offline shifter. At 9h15 after Oct 27.
A. Ciocio LBNL ATLAS Meeting - Jan 2009 428. Run with Cosmics
Full List 136
Trainees
Shifters 92
Experts 25
(Include experts)
Shifters statistics
• 30 residents at CERN
plus ~ 1/2 of experts residents
DCS 8
DAQ 10
DQM 9
SCT Institutes (34):Academia Sinica, Bergen, Birmingham, Cambridge, CERN, Cracow-AGH, Cracow-INP, Freiburg, Geneva, Glasgow, KEK, Kyoto, Lancaster, LBL, Liverpool, Ljubljana, Manchenster, MPI, NIKHEF, Okayama, Osaka, Oslo, Oxford, Prague-CU, Prague-CTU, QMW, RAL, Sheffield, Tsukuba, UC-Santa Cruz, UCL, Uppsala, Valencia, Winsconsin
(overlap)
0
10
20
30
40
50
60
ACR DCS DAQ DQM IDGen
QualifiedAlmost QualifiedCourse
SCT trained
> 2000 shifts
A. Ciocio LBNL ATLAS Meeting - Jan 2009 439. Final Calibration
Final Calibration in 2008
After ID combined run:• Full SCT ON
– Adjusted readout configuration• Latest list of number of modules in default readout configuration
– Response curve of SCT barrel and endcaps• Update with tuned thresholds based on gain curve measurement• Expected to improve noise occupancy
– Opto survey after end of calibration
• SCT sections ON to look at systematic dependencies of SCT Noise as reference for future studies
– Noise versus HV scan• Done on barrel side C and Endcap A
– Influence of FSI on noise (and leakage current)• Done on barrel at different power levels
– Noise versus cooling temperature: bp settings 3.0 (normal), 2.5, 2, 1.5, 1.2 bara
• Done on ~500 barrel and ~500 endcap modules
• DAQ improvements for calibration: – Speed (faster data archival and faster response from online GUI)
– Robustness (found/debugged reason of ROD failing to complete a scan due to errors)
• Faulty HV and LV boards replaced
SCT OFF December 12
A. Ciocio LBNL ATLAS Meeting - Jan 2009 44
• Barrel modules in readout 99.3% 14 of 2112 removed
• Endcap A modules in readout 98.7% 13 of 988 removed
• Endcap C modules in readout 95.3% 10+36 of 988 removed
98.9% 10 of 952 with loops 1C-TR and 9C-TR
removed from statistics
Modules excluded
9. Final Calibration
Modules in Default Readout
A. Ciocio LBNL ATLAS Meeting - Jan 2009 45
Noise versus bias voltage
• Obtain reference of noise dependence (detector capacitance) on bias voltage
• Measured ENC noise with 3ptgain scans
at 150, 120, 90, 70, 60, 50, 40, 30, 20 V bias voltage
Barrel module with 12cm strips Endcap Inner with ~6cm strip
9. Final Calibration
A. Ciocio LBNL ATLAS Meeting - Jan 2009 46
Noise occupancy at different voltages
• noise occupancy scan (new thresholds) in calibration mode at 150, 50 & 20V
9. Final Calibration
150V50V 20V
(x 10-5) 150V 50V 20V
Barrel 1.9 7.6 25.5
Endcap 3.5 ~11 ~35
A. Ciocio LBNL ATLAS Meeting - Jan 2009 47
Noise on barrel with FSI laser running
• Tested detector leakage current up to max 200mW (fibre 0)
• Tested barrel NO without and with 70mW (using chopper)– Using old thresholds and asynchronous L1A trigger
• Tests to be continued with FSI and L1A synchronousNo change in noise occupancy
9. Final Calibration
70mW with 50Hz chopper FSIMean = 3.755 x 10-5
No FSIMean = 3.748 x 10-5
A. Ciocio LBNL ATLAS Meeting - Jan 2009 48
ENC noise in calibration
9. Final Calibration
Barrel Noise ~ 1550 e-
Endcap noise ~ 1650 e- (outer/middle)and inner ~1100e- (950 short middle)
A. Ciocio LBNL ATLAS Meeting - Jan 2009 49
Noise Occupancy - New threshold setting
• Noise occupancy in calibration mode with new thresholds applied to chip configuration• New noise occupancy is ~2x 10-5
• ~ factor 2 improvement on barrel and less tail!
9. Final Calibration
Previously ~4x 10-5
Old thresholds
Full Barrel
Rms of vt50 point shows modules are well trimmed
1/2 Barrel
Endcap A
Mean ~2
A. Ciocio LBNL ATLAS Meeting - Jan 2009 50
Schedule
• Redesign of pipes around the compressors to be sufficiently strong to avoid fatigue cracks induced by vibrations.
• All compressors sent back to company for this rework.• Refurbishment of distribution racks in UX15 (until end of April)• Cooling will be off and SCT powered down with exception of DCS/DSS and
environmental monitoring.• TDAQ related development work will resume mainly in SR1• Power supply tests
– HV– PP3 debugging– LV pin current measurement (19.01 -- 3 weeks)
• FSI tests• Interlock system
– Last connections in the DSS system (Laser alarms + ATLAS emergency off signals)– Replacing plug-ins– Work on ID sensors and repair a few damaged pins in the Type II cables
• Opto tests • Training in SR1 can resume as early as mid/end of January (3 weeks interrupt in February)
and then again from March
10. Schedule 2009
January/February
A. Ciocio LBNL ATLAS Meeting - Jan 2009 51
• Endcap disk in SR1– Work almost completed
• 3 rings, 33 modules
• DAQ, DCS, Services,etc.
– Completion with Cooling
in January
Schedule (SR1)
10. Schedule 2009
January/February
Disk 1 (spare NIKHEF)
one quadrant
Barrel sector and Endcap disk in SR1
A. Ciocio LBNL ATLAS Meeting - Jan 2009 52
• Spring schedule remarkably tight– Due to maintenance/ interventions (Jan. – Feb.)– ATLAS cooling maintenance week 7-8-9
• 3-4 days no electricity in same period
– New TDAQ/HLT releases– Sub-systems migration to new TDAQ– TDAQ technical run (March)– Barrel and BW closed (end of March)– Work on detector (till April)
• April– Run slices of ATLAS to do debugging of s/w and infrastructure
• May – ATLAS in better shape than ever, combined run for:
• L1Calo, L1Mu trigger latency uniformity• Offline commissioning, alignment, calibration
• May – June– recurrent combined runs with defined purpose
• July – semi-continuous to continuous running transition
Schedule from run coordination point of view
10. Schedule 2009
Silicon ID working again
A. Ciocio LBNL ATLAS Meeting - Jan 2009 53
Summary
• SCT detector sign-off, integration in ATLAS and first cosmics last spring, cooling failures, recovery, off-detector commissioning without cooling, preparation for beam, first beam
• SCT detector run with cosmics (late September-October) ~1 million tracks • SCT detector improvements
– TX replacement: from ~96% to ~99% modules in default readout configuration – Much lower number of readout errors: typically 4-5 of ~8000 links– System more reliable in readout (in particular during calibration scans)
• Successful ID Combined Run (end of November) ~ 800K tracks • Completed calibration in December
– New configuration serves as reference point for spring startup– New thresholds have improved noise occupancy – Looked at systematic dependencies of SCT Noise as reference for future studies
• Trained ~100 SCT people for operation• Built Barrel sector and Endcap disk (to be completed in Jan) in SR1
Looking forward to: - complete off-detector parts: DAQ, DCS, Databases, Mon, TX, Power Supply upgrades
- resume training in SR1- integrate in ATLAS after cooling is working again (May)
* prepare for the 2009 beam *