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CMS Torino meeting, 4 th June, 2007 R. Castello on behalf of Torino Tracker’s group Tracker Alignment with MillePede

Tracker Alignment with MillePede

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Tracker Alignment with MillePede. Why we need alignment? Alignment with MillePede Algorithm Alignment with TIF trigger configuration on simulated cosmics data Preliminary results Status of the alignment with TIF real data Conclusions and outlook. Outline. Why we need alignment?. - PowerPoint PPT Presentation

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Page 1: Tracker Alignment with MillePede

CMS Torino meeting,

4th June, 2007

R. Castello on behalf of Torino Tracker’s group

Tracker Alignment with MillePede

Page 2: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

Outline

• Why we need alignment?

• Alignment with MillePede Algorithm

• Alignment with TIF trigger configuration on simulated cosmics data

• Preliminary results

• Status of the alignment with TIF real data

• Conclusions and outlook

Page 3: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

Why we need alignment?

• The CMS tracker is build in order to optimize the particle momenta resolution.

• It depends on two factors:

21 CpCp

p

C2 depends on MCS

C1 is geometry -dependent

B = magnetic field

L = track length

n = # hit of the track

σx = resolution on the measured point

sistx2

int2

21LBn

C x

~ 10 μm (Si)

Systematic error can be minimized by a correct alignment

Page 4: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

The tracker alignment

1. Survey measurements (during assembly) = 100-200 m2. Laser Alignment System (LAS) : alignment of TIB vs TOB etc ...3. Track Based Alignment (cosmics, Z→ etc) = 10 m

The problem16k microstrip modules

6 d.o.f per moduleO (100k) unknowns

• Complex system of equation to solve efficient and fast algorithm

• For CMS tracker alignment 3 algorithms:

HIP MillePede Kalman Filter

(Helsinki, Milano, Perugia) (Hamburg, Torino) (Wien)

Page 5: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

MillePede Algorithm

MILLE PEDE ( V. Blobel )

• A measurement can be written as

• Linearised least square combined fit of alignment parameters (global) and track parameters (local)

• MIllePede uses the Method of the Least Squares

residuum, where mk is the

measurement with uncertainty k and dk is the

coefficient vector.

the idea : minimize square of residuum.

fitk

hitkk

Tkk uudamr

kk

kT

k dama

2

2 )(

jj

ji

n

ii daz

11

global

local

Page 6: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

Alignment with MillePede

• Interested to the n global parameters.• For a set of N measurements: from (n+N) equations to n

• C’ matrix inversion (Computational time ~ n3 )

• With MillePede you can align @ different levels (Detectors, String, Layer level, etc…)

• 6 degrees of freedom for each alignable structure (6 parameters):

3 shifts (respectively along local x,y, z) and 3 rotations (around x,y,z)

the aim it’s to find a with good uncertainty

),,,,,( wvua

baC '' baC global

Page 7: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

MillePede Algorithm in CMSSW(implemented by G. Flucke, Hamburg)

- CMSSW 1_3_1 version - Alignment/MillePedeAlignmentAlgorithm (tag branchV00-07-0X-01) - Cfg file: AlignmentTrackSelectorModule:- selection of Tracking algorithm

- set APE - set cut for tk selection

(pt, #hits,..)

AlignmentProducer: - selection of alignment parameters - geometrical selection in eta, phi,z

- selection of misalignment scenario - set solving method ( inversion, etc.) - set 2 range acceptance PoolSource: - selection of dataset - set number of events

Page 8: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

Cosmics simulation @TIF (Tracker Integration Facility)

Old scintillator configuration ( 36k events)

New scintillator configuration ( 20k events)

Since Feb.’07 the 25% of the tracker system is under commissioning

Page 9: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

RMS =263 rad

Rod Level (79 alignment

parameters)

RMS =151 m

Results on TIF cosmics simulated sample (old trigger configuration)

with Short Term misalignment scenario (~100 pb-1)

Page 10: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

u (Strings level)

Good correlation between u at the start (misaligned) and at the end (after the alignment)

Global correlation : largest correlation of a parameter with any linear combination of all other parameters. A value close to 1 means solution not well determined.

Page 11: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

Simulated cosmic sample with old scintillator configuration (x axis)

Sim

ula

ted c

osm

ic s

am

ple

wit

h n

ew

sci

nti

llato

r co

nfig

ura

tion (

y a

xis

)

agreement for u

Old and new MC configuration

To be understood..

Page 12: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

u and for real data (10th March run)

RMS =21 m

RMS =79 rad

Rod Level (71 alignment

parameters)

Too precise if compared with the “expected” results

under studying…

Page 13: Tracker Alignment with MillePede

CMS Torino meeting R.Castello4th June 2007

Conclusions & outlook

• Preliminary results obtained running MIllePede alignment algorithm on TIF simulated sample for u and parameters at two different hierarchical levels (Strings & Layer )

• No relevant differences between new and old scintillator configuration on simulated data (a first indication of algorithm stability)

• The exercise on real data is going on

• Good impression and relevant hints from recent Hamburg workshop:

http://indico.cern.ch/conferenceDisplay.py?confId=16095