fgasparini INFN roma 30/3/2006

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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

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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”

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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


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


•HV/LV test

•Noise

•Current stability for 48 hours

•HV/LV test

•Noise

•Current stability for 48 hours

Sector test

In SX5

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Commissioning Commissioning Current stability and noise


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

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Cabling Cabling


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


• 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


• 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

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Technical trigger Technical trigger Introduction


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


• 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

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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


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


µGC

F- specific electr.

pH-meter

HPLC



µG Cromatog.

F- specific electr.

pH-meter

HPLC



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Gas system Gas system Design of the gas calibration system


Very similar to the DT gas controlmade by small drift chambers(Aachen)

42

Organization and manpower Organization and manpower Manpower


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

43

Conclusion RPCConclusion RPC Manpower


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

fgasparini INFN roma 30/3/2006

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