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STATO BARREL MU: DT & RPC Costruzione e installazione fgasparini SW,commissining e analisi ugasparini Elettronica e Cosmic challenge mdallavalle fgasparini Roma 4/4/06. SOMMARIO DT: - PowerPoint PPT Presentation
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STATO BARREL MU: DT & RPC
Costruzione e installazione fgaspariniSW,commissining e analisi ugaspariniElettronica e Cosmic challenge mdallavalle
fgasparini Roma 4/4/06
SOMMARIO DT:
HVB e il ritardato avvio di Torino e della produzione dei MC non hanno introdotto ritardi che si siano ripercossi su sequenza e tempi di installazione.
Tutte le finestre di installazione disponibili sono state utilizzate.
Commissioning e test di settore (vedi Ugo e Marco) senza problemi.
Notevole mobilitazione di personale.
Elementi critici per installazione dopo Mag.Test:-Certificazione camere agli ISR (dipende da DT)-Disponibilita’ dei cavi (solo parzialmente dip. da DT)-Disponbilita’ di personale
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TORINO Torino rate 6 SL/month
Stato 14/3/2006
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24 installate
Inst. 22
203/250 Minicrates al CERN al feb 6/06 135 installati fine prod. Maggio/Giugno152 da Giu a Feb = 17/ mese ( 6 in Agosto) 18/mese escludendo Agosto 18,5/mese da ottobre a fine anno (nom. 12~16)
Produzione nuove HVB finita in Settembre. Sostituzione agli ISR completata
Assemblaggio DT finito in tutti I siti (To in Maggio) : ultime camere (Aachen 8,LNL 5,To 8) attese al CERN a meta’ maggio.
MINICRATES
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YB+1 is complete 42 stations DT+RPC installed
YB+2 has 40 stations installed ,feet chambers missing(A. Benvenuti, M, Benettoni ,A Colaleo, A. Clemente and crew)All DT commissioned before Xmas (with MCrates) (E.Conti.M.Zanetti,K.Hoepfner +…)31 DT tested after cabling in YB+1 : only one problem (a disconnected pin ) (3/4/06)
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12 MB4 To.
INSTALLAZIONE E COMMISSIONING DI DT+RPC Sector commissioning
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51 DT+RPC (10 MB4 To) (+ 2 feet ch. in YB+1) installed before Mag.Test
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YB0 chambers commissioning before Mag. Test.3 sectors commissioned up to now : no problem (3/4/06)
Installation in YB0Test for Inst. In UX
4 ch./day
2 ch/day in the cavern
(31 ch)
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SX 5 Thursday March 2 nd
fgasparini INFN roma 30/3/2006
Festa in SX5 per 135 DT+ RPC installati, (115 da installare)
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AB 14/3/06
AB14/3/06115 DT+RPC
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AB14/3/06
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Might be mid august
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Una serie di azioni e’ stata intrapresa ad inizio anno per far fronte a questo piano di installazione
Tutta l’attivita’ e’ stata divisa in 12 settori ,con uno o piu’ responsabili/settore
Settori critici sono stati rinforzati,con immissione di personale e/o nuovi strumenti
ELEMENTI CRITICI >> trasp. seguenti
PMs FG , Iaselli , Rodrigo
Local TBAB, ,
Reithler Benettoni,Puerta,Montecass.,Hoepfner,Checchia,Gonella,Giacomelli,Dattola,Piccolo,Colaleo(RPC),Bencze(Alignment)
All task responsibles are physicists or engineersin bold RED are new engineers, (P means permanent since beg. of March) . I n red are new technicians :Francia perm. Torino is 1 FTE out of 3 people, 1 + 1 part time from Aachen
I nstallation I SR I SR I SR CABLI NG I ntegration DT prep. Commiss Rack Connex MC connex MC Testing Bat904
certification ch.dressing MC inst/ test & bulk cabl YB0,cables for commiss cabl./ ppanels during cabl. after cabling HV/LV testhandling etc.. services SX 5 SX 5 SX5/ UX/ SC SX 5 SX 5
Benettoni Puerta Benvenuti Gonella Montecassiano Dattola Benvenuti Hoepfner Checchia Gonella GiacomelliConti
Local tech.boardDT+RPC+Align AB chair
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Jesus Puerta Pelayo March CMS Week CERTIFICAZIONE DT AGLI ISR
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The main source of uncertainties is the identification of HV problems (chambers are “new” after HVB replacement). Some of them appear after a long time under HV, some cannot be cured by simple replacement, some are due to single Cells hence very difficult to localize . HV test and Cosmic test must be repeated after any intervention. There are ideas and actions to improve the procedure…………..
AZIONI INTRAPRESE:Cordero da Torino a tempo pieno a ISR , rinforzo del team di tecnici a rotazione (da inizio Marzo)
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Amedeo
7800
3600
Other forks achen
CERN
CERN
= done
AZIONI INTRAPRESE:Motorizzazione di culle di inst.Extra telai di trasportoExtra elementi di fissaggio culle.Piu’ persone per installazione
fgasparini INFN roma 30/3/2006
TORINO
CERN (20?)
STRUMENTI PER RIDURRE I TEMPI DI INSTALLAZIONE DT+RPC
TORINO
ABenvenuti
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YB0, YB-1 and YB-2
A lot of missing items needed to finalize cutting lengths• YB-1 and YB-2
– Peripheral paths are almost the same as in the positive wheels. No major work is required there. I can adapt what I already done for positive wheels.
– Radial layouts (ZmL and ZmR) has still to be designed and verified
• YB0
– it is not yet defined from the point of view of peripheral paths. D. Dattola is working on this subject.
– also radial layout ZmL and ZmR are needed
• Also there are many other urgent work pending
– Cables in the chains :PRR, procurement, cutting lengths
– cable chain patch panels
– racks layout update (LV/RPC/ALIGN requested changes in the last months)
– Detailed design of each single rack with cables ....
AZIONI INTRAPRESE: in collaborazione con RPC rinforzato il team Dattola/Montecassiano(Colonna (RPC), Abajiev(RPC), + disegnatori Pd e Na, P.Checchia resp. per cablaggio nei racks e balconate)
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DT +RPC : Integrazione YB0, cavi, cablaggi
Montecassiano/Dattola
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Personale per installazione/cablaggi/commissioning (DT)fg
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available tech CIEMAT Aachen Padova Bologna Torino IHEP CERN
Ahjiado FullT 1+ 1 mech Barcellan(I SR/SX)Cafaro 0,5 1 mech FTE 2 FTE FT Divincenzo FTFrancia Full T Schulz+ 1 electrTemporin(SX) Giordano 0,5 (out of3 part time)
for ISR part time X (SX) X 0,2 1 electr o,25X (cabling) 0,25 following needs Y (SX)
Borsato (SX)Fetchenhauer Modenese(SX)(full time) Pedrotta (mech)
Colombo (mech)all part time= 0,25 installation crew
total FTE Technicians + Physicists
2,25 2 2 1,2 1,25 10,5 crew 1 Hoepfner 0,5 Gonella 0,7 Giac o,7 Nervo
3 certification 0,5 Crew 0,5 Checchia 1 Benv 0,5 Crew 0,3 Montecass
0,09 Giunta 0,12 Giunta 0,7 Montecass. 0,3 Giunta 0,7 Mariotti 0,5 Dattola
0,3 install. 0,5 Crew 0,5 Crew 0,8 Cordero 0,5 Colonna
0,5 benettoni 0,7 Masetti 0,5 Dattola 0,5 Giunta
1 install. 0,3 install
TOTAL 5,84 3,9 5,7 4,5 4,6 3,8
people supported TOTAL 9,74 14,2 by CERN
(tech. 4,25 + phys 5,5) (tech ~5,8+ phys.~ 8,4)
TOTAL I/ G/ S = 23,96 FTE
(Crew= physicists for commissioning and MC test after cabling)
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Sblocchi SJ richiesti su CABologna 40 KE ( new HVB >>> hired mp) (Accordo di compensazione con la Germania)Padova 20 KE (cavi)32 KE (crate& ctr >>> cavi + fibre+ connettori + montaggio) (accordo con Spagna)
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NO EXTRACOSTI CORE (salvo sorprese)
Maggiori,non drammatiche,spese per tools e hired manpower ( M&O B )
Missioni estere insufficienti : a settembre sblocco SJ + …………….)
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1. RO/trigger electronics Global view --responsibilities
DT front endBarrel
DT Track Finder
WedgeSorter Barrel Sorter
GLOBAL MUON TRIGGER
Detector in
UXC55
Counting
room in USC55
LVDS copp
er link
Opto
link
Towers in
UXC55
DT station
(minicrate)
CCB
Trigger BoardsReadOut Boards
Sector Collector ROS
Server Board Link Board
DDU
FEB PadovaTRB Padova,BolognaROB CiematSB BolognaLB,CCB PadovaLVDS link BolognaDCS,TTC link Padova
Trig SC BolognaROS CiematOptolink Bologna
DDU TorinoDTTF ViennaWS BolognaBS Bologna
M Dallavalle
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4. trig Sector Collector board
trig Sector Collector opto-rx
Slow control Master:Final prototype readyCrates and Controllers
1 procured for the magnet testVME controllers
First prototype workingMust be tested for radiation tolerance
PHTF-ETTF-WS-BS integration test
SBSWedgeSorter
ETTFPHTFTIMBarrelSorter
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5. DDU (FED)
Final system: 1 VME 64x crate with 5 boards (1 per DT wheel)
G.Dellacasa, V.MonacoINFN-Torino 29/3/2006
• 1 pre-production board has been debugged in the previous months.
• The DDU functionalities required for the Magnet Test have been tested
• The DDU board is now (mid March) in Legnaro to be integrated with the DT DAQ.
• It will be moved to CERN in the first half of April for the preparation of the• Magnet Test. in order to validate the design and start the final production • (5 DDU boards+spares)
Inst/Commission Trigger crates Apr. 06- Sept. 06Integrate detector electronics May 06- Oct 06Integrate Central Trig.&DAQ Oct. 06 – Mar. 07System commissioning Apr. 07- Aug. 07Ready for Data Aug. 07
TRIGGER INSTALLATION SCHEDULE
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9. Production-installation-commissioning(production after validation in the Mag.Test Cosmic Challenge
Boards Q.ty (+ spares)
Prod start Prod End
Opto Tx piggy 60 (15) Mar Q1 – 2006
Jun Q1 – 2006
Opto Rx board 96 (24) Apr Q1 – 2006
Aug Q1 – 2006
LVDS Rx 2 ch piggy 200 (30) Mar Q1 – 2006
Jun Q1 – 2006
Mother board 60 (15) Apr Q1 – 2006
Aug Q1 – 2006
LVDS Rx 4 ch piggy 10 (8) May Q1 – 2006
Oct Q1 - 2006
Production Critical items: •Trigger sector collector : ~8 months from start
•ROS25 : ~6 months from start (CIEMAT)
DCS production Schedule
• UXC55 fibres and cables:
– Cut and connectorize as soon as
cutting lengths become available
• USC55 fibres (slow control + TTC)
– Finalized during Q4-05
Slow control Master:Production to be started in April-06
VME controllers2nd prototype ready in April-06Radiation test in June-06Production launched in June/July -06
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MTCC workplan -- LNL-tests
Inst/Commission Trigger crates Apr. 06- Sept. 06Integrate detector electronics May 06- Oct 06Integrate Central Trig.&DAQ Oct. 06 – Mar. 07System commissioning Apr. 07- Aug. 07Ready for Data Aug. 07
TRIGGER INSTALLATION SCHEDULE
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• DT MTCC project ramp-up in steps: Sector Commissioning•goal: autotrigger on one chamber and acquire data from 4 chambers, DAQ synchronisation, first look at cosmics traversing a sector
•Sector Test –local mode•goal: final tower electronics, local autotrigger logic with 4(5) chambers, read ROS25 with local DAQ (no FED)
Sector Test –regional mode \•goal: provide trigger to CMS, integrate regional trigger, use final TTC system
•Sector Test•goal: cosmics trigger with three sectors•FED Integration•goal: data flow from ROS through DDU to global DAQ
Sector commissioning
Two sectors
M DallaValle
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- Il software generale di simulazione/ricostruzione/analisi di CMS e’ nel mezzo di una fase di transizione al nuovo Framework (CMSSW)
Stato del software
- Come per gli altri sub-detectors, e’ in corso il “porting” del codice ObjectOriented di simulazione (OSCAR, basato su Geant4) e ricostruzione (ORCA) ,
- il porting delle varie componenti e’ prevista per l’ analisi dei dati del “Magnet test/cosmic challenge” (Maggio-Luglio 2006)
U Gasparini
[ slides/materiale dal DT sw group: - F.Cavallo (Bologna) - A.Meneguzzo, S.Lacaprara, P.Ronchese, M.Zanetti ( Padova) - N.Amapane, R.Bellan, G.Cerminara (Torino)]
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Muon DT Software
Esempio: - analisi dati del primo “test di settore” compiuto con 4 camere nel Dicembre 2005(auto-trigger dato da MB3 )
Evento ricostruitoin CMSSW e visualizzatodal pacchetto grafico di CMS (IGUANA)
r- view r-z view
MB3
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DT clients forDQM application Developed in CMSSW:
- Digi client- TestPulse client- Data integrity
DT software: Data Quality Monitoring
La parte piu’ avanzata riguarda il DQM degli oggetti di ‘bassolivello’ (raw data/digi), gia’ attualmente inserita nel software generale
e utilizzata nel commissioning delle camere con i cosmici
Oggetti di‘alto livello’ (tracce…)per l’ analisi delle prestazionidel rivelatore sono tuttorain costruzione…
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Sono stati analizzati i dati di cosmici relativi a 82 camere installate (42 Wheel+1 , 40 Wheel +2) commissionate (delle 134 installate in CMS):
Analisi dati del “DT commissioning”
Effic. per cella Celle morte (10 MB1 ruota +1) 18/6500 ~ 0,27 %
99,9%2
SL1
SL2
SL3
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mm
=540m =230m
Con una correzione temporale off-line evento per evento (il tempo dei MU e’casualei…e l’elettr.funziona a 40 MHz)si ottiene una risoluzione spaziale,mediata su tutta lacamera e su tutti gli angoli di 230 ~ 280 micron (il valore nom.e’ 250)compatibile con quella osservata nei testbeam ( ~ 200 m )(Mu sincroni,localizzati & ad alto momento)
Hit residuals:not 0 correction
t0 correction applied
25
MB1
MB2
<>=-124 14 m
<>=568 12 m
<>=-0.1 0.1 mrad
<>=0.4 0.1 mrad
Extrapolations of segments builtin single SL’s:
-Sensitive to displacements between SL’s
- depend also on internal mis- alignments between single layers
“Internal geometry”
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SlopeDifference,R- view:
MB1 vs MB2
MB3 vs MB4
MB2 vs MB3<>=0.20.1 mrad<>=0.70.1
mrad
<>=2.40.1 mrad
1-2
Analisi del primo “sector test”
27
Selection:-MB3 auto-trigger (HH+HL);- 1 clean track reconstructed in both r-phi & r-z views in MB3, predicted to be inside MB1 (MB2) geometrical acceptance
Nhits>5
Nhits>5
Nhits 3
Nhits 3
MB1
MB2
Track reconstruction efficiency
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MB1 MB2/SL1
MB1
MB2
<>=-1210 30 m
<>=-1360 40 m
<>=-1260 40 m
<>=-1240 30 m
Sector test: extrapolation to individual layers
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SommarioIl Software del DT detector e’ in continuo sviluppo;sostanzialmente “on track” per l’analisi del rivelatorenel test col magnete e l’ integrazione nel sw generaledi CSM
L’ analisi dei dati del Commissioning delle camere e laricostruzione (parziale) nei primi test di settore mostranorisultati sulle prestazioni compatibili con le attese e notevoli potenzialita’ per la comprensione dettagliatadel comportamento del rivelatore nel suo complesso(utili anche in vista della comprensione del comportamentoin campo magnetico ,
(prima e unica possibilita’durante il Mag.Test.)
La preparazione per il Cosmic Challenge e’ a buon punto
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SG & DG Production
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
About 3000 Single gaps built: production ended
1080 DG produced ~ 60 DG more, end production April-May 06
420 Chamber produced : 60 chamber more, end production June 06
1080 DG produced ~ 60 DG more, end production April-May 06
420 Chamber produced : 60 chamber more, end production June 06
0
200
400
600
800
1000
1200
1400
Dec-02
Feb-03
Apr-03
Jun-03
Aug-03
Oct-03
Dec-03
Feb-04
Apr-04
Jun-04
Aug-04
Oct-04
Dec-04
Feb-05
Apr-05
Jun-05
Aug-05
Oct-05
Dec-05
Feb-06
Apr-06
DG produced
DG planning
Chamber construction Chamber construction
0
100
200
300
400
500
600
Dec-02
Feb-03
Apr-03
Jun-03
Aug-03
Oct-03
Dec-03
Feb-04
Apr-04
Jun-04
Aug-04
Oct-04
Dec-04
Feb-05
Apr-05
Jun-05
Aug-05
Oct-05
Dec-05
Feb-06
Apr-06
Jun-06
all produced
all planning
Double gap
Chamber
Total lot 480
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ISR storage and test area ISR storage and test area Long term test/coupling
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
Detector control •Gas leak •Gas input overpressure test•Threshold setting and reading•Current vs HV•Long stability test (15-20 days @ 9200 V)
Performance 15 chambers can be tested at same time•Single rate (hits count.) vs. HV •Noise rate (cluster count.) vs. HV•Cluster size vs. HV
Detector control •Gas leak •Gas input overpressure test•Threshold setting and reading•Current vs HV•Long stability test (15-20 days @ 9200 V)
Performance 15 chambers can be tested at same time•Single rate (hits count.) vs. HV •Noise rate (cluster count.) vs. HV•Cluster size vs. HV
117 chambers now at ISR.254 installed
DT-RPC coupling. The following functionality tests are performed: gas leak, HV integrity, threshold setting/reading/ strips connectivity. The cooling circuit (RPC, DT FE, MC) is checked at 20 bar overpressure.
DT-RPC coupling. The following functionality tests are performed: gas leak, HV integrity, threshold setting/reading/ strips connectivity. The cooling circuit (RPC, DT FE, MC) is checked at 20 bar overpressure.
After DT+RPC COUPLING
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Commissioning Commissioning Activities
•Commissioning the final gas distributor
• Gas line equalizationEach CMS gas line supplies in parallel 2 chambers in same station. Very important to equalize the gas flow between the chambers
•Gas mixture monitoring and HV interlock system
•Commissioning the final gas distributor
• Gas line equalizationEach CMS gas line supplies in parallel 2 chambers in same station. Very important to equalize the gas flow between the chambers
•Gas mixture monitoring and HV interlock system
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
•HV/LV test
•Noise
•Current stability for 48 hours
•HV/LV test
•Noise
•Current stability for 48 hours
Sector test
In SX5
33
Commissioning Commissioning Current stability and noise
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
HV 9200 VHz/strip
Strip = 420 cm2
Current
Noise/strip
HV 9200 V
Ordinata: micro amp/2 gaps/ Ascissa 48 ore.Limiti di rigetto 5 micro. Richiesta di stabilita della corrente
100/420 cm2=0,25 Hz/cm2Limite qualche Hz/cm2
34
Cabling Cabling
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
Status
• Cables on the detector
– trigger cables 4720 (average length 15 mt, total length 75 km)
– HV cables 480 (total length 10 km)
– LV cables 360 (total length 7 km)
– DCS cables 420 (total length 8 km)
• Cables between detector and counting room
– Long HV cables 60 (total length 6 km)
– LV controls about 20 (total length 2 km)
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HV/LV/DCS HV/LV/DCS Status
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
• 10% boards, 50% crates available• Total 60 boards A3512, 14 EASY crates• HV cables in production • System for cosmic challenge ready at 904
• 25% board, 50% crates available • Total: 60 boards + 20 EASY crates • LV cable in production• System for Cosmic Challenge in test at building 904
HV LV
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HV/LV/DCS HV/LV/DCS DCS/Monitoring
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
• Control and monitoring of HV-LV system OK• Control and monitoring of gas system, cooling, temperature in progress
• Front-end configuration (threshold and width) ex-warsaw in progress
• Detector monitoring ( current, HV) OK• Detector monitoring (noise, occupancy…) ex-warsaw in progress
• Integration with CMS DCS OK• Integration with Run Control to be started
Gas monitoring planned• Gas system monitoring
• Control and monitoring of the for mixture analysis devices ( gas-chromatograph
• Control, monitoring and read-out of the gas calibration system
37
Technical trigger Technical trigger Introduction
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
Goal of this project is to produce an RPC-based cosmic ray trigger for the Commissioning of RPCs, the Cosmic Challenge and later running of CMS as Technical Trigger
Local trigger (RBC): based on 1 Sector, will be used to test RPCs (and DTs) during Commissioning and Cosmic Challenge
Global trigger (RBC + TTU): based on the whole Barrel, will be used during the off-beam periods for the detector calibration
LBBox
RBCLBBox
LBBox
RBCLBBox
LBBox
RBCLBBox
LBBox
RBCLBBox
LBBox
RBCLBBox
LBBox
RBCLBBox
UXC area
Barrel Wheel
USC area
TT
U
6 Fibers/wheel
Fiber GL
OB
AL
TR
IGG
ER
RBC (RPC Balcony Collector) Technical Trigger Unit
TT
UT
TU
TT
UT
TU
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Technical trigger Technical trigger Status
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
• The RBC is housed in the Link Board Boxes around the detector and produces 2 Sector Triggers, making coincidences among OR signals of 96 strips (half RPC) received by the Link Boards
• 3 prototypes of RBC were produced last autumn and recently tested. They are ready to be used during the Cosmic Challenge
• The Technical Trigger will be implemented in the Technical Trigger Unit (TTU), housed in the Trigger Crate in Counting Room
• It will receive the ORs from 1 Barrel Wheel and find cosmic patterns, providing Wheel-level Trigger
• These features can be exploited by the Trigger Board (Warsaw), loading the cosmic patterns in the Pattern Comparator
RBC
+ TTU
39
Gas system Gas system Commissioning the gas system at SX5
• Wheels +2 and +1 completed
• Currently working on:– Flux entire wheels +2 and +1 (need
careful equalization at the channel level)– Set up of wheel 0 distributor rack
• Check flow cells (found sometimes mis-calibrated ,CERN responsibility)
• Sectors under flux (and test) for 3-4 days each
• Monitoring of the gas mixture • Mass flow-meters read out by ADC + T
and RH probe• Interface with the HV kill system
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
40
Gas system Gas system Design of the gas quality monitoring system
µGC
F- specific electr.
pH-meter
HPLC
General purposesampling point
2 lines (up. and lw. part) × Wheel (or Endcap) on the output … multiplexed
In addition, T and RH sensors on the input lines and close to some RPCs
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
µGC
F- specific electr.
pH-meter
HPLC
General purposesampling point
In addition, T and RH sensors on the input lines and close to some RPCs
µG Cromatog.
F- specific electr.
pH-meter
HPLC
General purposesampling point
In addition, T and RH sensors on the input lines and close to some RPCs
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Gas system Gas system Design of the gas calibration system
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
Very similar to the DT gas controlmade by small drift chambers(Aachen)
42
Organization and manpower Organization and manpower Manpower
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
Production
2 physicist + 2 technicians at Bari*1 physicist + 1 technicians at Pavia1 physicist + 1 technician at GT
* 1 physicist funded with FAI 1 technician funded with ex 2222
Certification ISR 4fte2 physicist + 2 technicians 2 physicist funded by CERN
Installation 1fte1 physicist + 2 technicians
Commissioning gas 0,5 fte2 physicist
Commissioning detector2 sect/week 2 fte2 physicist + 2 technicians 1 physicist funded with FAI
Cabling 2,5 fte1 physicist + 1 technician 2 engineers
HV/LV/DCS1 fte3 physicist + 1 technician
11 fte tot.for inst./commiss
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Conclusion RPCConclusion RPC Manpower
Roma 30/3/2006, meeting with INFN referees CMS Barrel RPC
1. Production end by June 2006
2. ISR test and Installation on schedule (254 RPC) (4+1 FTE)
3. Commissioning without relevant problems (2 FTE)
4. Big effort on Cabling (new people from Frascati) (2.5 FTE)
5. HV-LV in production (20% under test blg 904) (0.5 FTE)
6. DCS ready for Cosmic Challenge (0.5 FTE)
7. Gas system: 3 wheels are ready (CERN resp.)
• But need a permanent overview from RPC side (0.5 FTE)
• Gas monitoring system under design (Frascati)
8. Technical trigger ready for MTCC
9. 11 FTE needed for Installation/Commissioning/Cabling..ONLY
NOT INCLUDED: Cosmic Challenge, Control Room inst., Trigger, DAQ and DCSIntegration and commissioning, Underground work (since sept 06)..etc etc
Recommended