cathode strip chambers status report

28
22 Sept. 2008 G. Rakness (UCLA) 1 Cathode Strip Chambers Status Report Greg Rakness University of California, Los Angeles CMS week plenary session CERN 22 Sept. 2008

Upload: tait

Post on 27-Jan-2016

28 views

Category:

Documents


0 download

DESCRIPTION

Cathode Strip Chambers Status Report. Greg Rakness University of California, Los Angeles. CMS week plenary session CERN 22 Sept. 2008. Sources of Muons Used for CSC Commissioning (I). Cosmic rays Expansion of the system from few  468 chambers - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 1

Cathode Strip Chambers

Status Report

Greg RaknessUniversity of California,

Los Angeles

CMS week plenary sessionCERN

22 Sept. 2008

Page 2: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 2

Sources of Muons Used for CSC Commissioning (I)

• Cosmic rays– Expansion of the system from few 468

chambers• Asynchronous muons over the full angular

spectrum

Page 3: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 3

Intra-CSC Trigger Synchronization Cosmic Rays

ChamberId = SectorId*100+StationId*10+CSCID

Synchronize chambers on one endcap w.r.t. a reference chamber on that endcap

Synchronization of (most) chambers to better than 0.2bx

ME+

ME

D. Wang (UF)

Use chamber overlaps with cosmic rays to synchronize the chambers to each other on average

Page 4: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 4

Run 57795 (CRUZET-4):

ME+1 ME+2 ME+3 ME+4

ME3 ME4ME2ME1

Recall: Chamber Illumination with Cosmic Rays

Plots by A. Kubik and M. Schmitt (Northwestern)

Page 5: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 5

Sources of Muons Used for CSC Commissioning (II)

• Single beam bunch in LHC (~2x109 protons)– Beam passes through CMS beam

dump• Synchronous muons approximately parallel

to beam

– Beam captured several turns• Synchronous muons approximately parallel

to beam

Page 6: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 6

CSC “Halo Muon” Trigger Single Beams

x

ME+ ME

TOF 2 bx

(Beam-1) halo muon

Normal proton

collisions

LHC mode: both endcaps trigger simultaneously on IP muons

“Halo Muon” trigger: CSC Track Finder selects tracks with small

• Trigger on outgoing endcap (i.e., ME for Beam-1)

Approximate timing of muons from IP

• [Note: for first beams, the incoming endcap was also included in the trigger (delayed by 2bx). This is no longer true…]

Page 7: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 7

Chamber Illumination: Beam-2 Halo

http://lotus.phys.northwestern.edu/~kubik/newdata/run62096/

Run 62096:

ME4ME3ME2ME1

ME+1 ME+2 ME+3 ME+4

Page 8: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 8

Beam Halo Event through Both Endcaps

More event displays are stored athttp://www.nuhep.northwestern.edu/~schmittm/CMS/TEMP/event_displays/

Run 62384Event 56199

Page 9: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 9

Zoom in..

Most beam halo events look like this…

Page 10: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 10

3-Muon Event in the CSC’s

http://www.nuhep.northwestern.edu/~schmittm/CMS/RESULTS/results.html

Page 11: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 11

Sources of Muons Used for CSC Commissioning

• Single beam bunch in LHC (~2x109 protons)– Dumps into collimators ~150m away

from CMS• Synchronous “splashes” of muons + stuff

Page 12: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 12

Coincident with collimator dumps:“Monster” CSC events

• Some numbers:– Event size 3MB (normal size ~few kB)– 160k/200k strips with data

• Causes (irrecoverable) error somewhere in CSC DCC Global DAQ Myrinet chain – Forced to stop and restart run…

• Local DAQ took event with no errors – Local readout through different path…

• To avoid this DAQ problem: remove CSC from Global DAQ during beam dumps into upstream collimator

Under investigation…

Page 13: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 13

Collimator dump “Monster” CSC event

Reconstructed segments from Local DAQ data…

Page 14: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 14

Data Analysis

Halo muons: angles of muons and beam structure

Page 15: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 15

Reasonable description of beam ON data: combination of • beam halo • cosmic rays

(Separate normalization of blue and black curves not quantitative…)

Cosmic rays

Beam halo

Single beam: reconstructed track angle w.r.t. the transverse plane

http://www.nuhep.northwestern.edu/~schmittm/CMS/RESULTS/results.html

Page 16: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 16

Cosmic rays do not care about beam structure…

~ Cosmic rays~ Beam halo

A. Kubik (Northwestern)

Separate Beam Halo and Cosmic Rays by Track Angle

look at the BX distribution

Beam halo muons come in single bx number, as expected…

Page 17: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 17

Beam-2: Distribution of BX valueshttps://cmsdaq.cern.ch/elog/shift/3528

For BEAM-1 (19 Sept):

“… CSC remains [the] reference…” I.Mikulec (Trigger elog 680)

For BEAM-2 (10 Sept):

CSC Halo measured to be in time with HF technical trigger…

Delayed BPTX2 to be in time with HFTT and CSC Halo…

Page 18: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 18

Data Analysis (II)

Chamber performance with Beam Halo Muons

Page 19: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 19

Number of hits on a reconstructed segment.In MC we assume 100% efficiency for fiducial hits.

A. Kubik (Northwestern)

Page 20: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 20

Efficiency to obtain a recHit in each given layer, for all chambers in ME+2/2

S. Stoynev (Northwestern)

Page 21: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 21

Towards Alignment Constants…

Page 22: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 22

Endcap z-positions with magnet at 0T, 3T

First reconstructions:• ME+2,3,4 stations at

B=0T, 3T• Simultaneous Rφ fit for

all SLMs in ME+2, ME+3 at B=0T, 3T

Compression comparable to MTCC at equivalent

magnetic field

XSLM [mm]

ZC

MS [

mm

]

• Integration of Barrel-Endcap-Link systems underway• Initial integrated model of link+endcap available

• Provide an integrated, global muon geometry• Upload geometry in ORCON/ORCOFF to be used in reconstruction • Combine/Compare with track-based alignment

G. Gomez (Cantabria)

Page 23: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 23

Track Based AlignmentJ. Pivarski (Texas A&M)

Use simultaneous solution of fits to residuals from overlapping regions to align chambers to each other (For details, see alignment meeting Wednesday)

Page 24: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 24

Summary Q: Is CSC ready for beam?

A: Yes (but we still have a lot to do!)

Online DQM “EMU status00” plot: Green = system able to provide at least two muon stubs

Page 25: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 25

Backup slides

Page 26: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 26

LHC Beam Notation

CMS

+x

+z+y

LHC “Beam 1”:

• Enters p5 from p4

• Traverses CMS from ME+ to ME

LHC “Beam 2”:

• Enters p5 from p6

• Traverses CMS from ME to ME+

Page 27: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 27

CSC Inter-Endcap Synchronization with HE

ME+ and ME endcaps synchronized with each other

Avg = 6.3 Avg = 5.2

Avg = 5.1Avg = 5.2

Accurate TTC CCB fiber lengths implemented (Jay Hauser

[UCLA])

Before:CRUZET-3

After: CRUZET-4

Page 28: Cathode Strip Chambers Status Report

22 Sept. 2008 G. Rakness (UCLA) 28

Separate beam halo and cosmic rays by track angle (previous slide)

look at the BX distribution

The beam halo comes mostly at a single bx, while the cosmic rays

are everywhere, as expected.

(zoom-in)

~ Cosmic rays

~ Beam halo

A. Kubik (Northwestern)