GEM Development in India, test beam analysis and plan for next test beam Anand Kumar Dubey for VECC...
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Transcript of GEM Development in India, test beam analysis and plan for next test beam Anand Kumar Dubey for VECC...
GEM Development in India, test beam analysis and plan for next
test beam
Anand Kumar Dubey for VECC group, Kolkata
CBM Muon detector requirements:
Main issues: The first plane(s) has a high density of
tracks -- detector should be able to cope up with high rate. ~ 10 MHz/cm2
good position resolution Should be radiation resistant Large area detector – modular
arrangement suitable options: micropattern gas detectors such as GEMs, Micromegas, and more recenlty THGEMs.
Multi GEM configurations
For MUCH R&D : we have assembled and tested double and triple GEMs prototypes
Schematic of prototype GEM chamber assembly
GEMS1 2 3
Drift plane (inner side copper plated)
12 x cm 12 cm x 10 mm
Readout PCB
CERN made GEM foils obtained fromArea: 10cm x 10cm
Drift gap: ~7mmInduction gap: 1.5mmTransfer gap: 1mm
Detector fabrication at VECC for Sep08 beam test
Readout plane 256 Pads 8 mm x 3.5 mm
10 ohm Resistors for protection
Outer side of the readout PCB
DeltaV (GEM)ADC
Test with Fe55 + nXYTER using 3GEM
ADC
AD
C
Pulse height from Pad#20
nXYT
ER
ADC
Subt
ract
ed A
DC
Testing of GEM chambers @GSI At the SIS 18 beam line using proton beams of 2.5 GeV/c Aim being : -- to test the response of the detector to charged particles. -- efficiency, cluster size, gain uniformity, rate capability, position resolution and dynamic range study.
-- testing with actual electronics for CBM : nXYTER -- testing with the actual DAQ -- Aug08-- first successful test with n-XYTER(with 64 channels bonded ) + GEM was performed. MIP spectra for 2GEMs and 3 GEMs were obtained. -- Aug-Sep 09, In 2009 a fuller version of nXYTER with all the 128 channels bonded was available. this offered a better configuration for efficiency estimation and also for cluster size estimation.
Beam Region fired (2008)
Only alternate channels hit, efficiency estimate couldn’t be possible
BEAM SPOT
3-GEM
Main Features: --- more number of days as compared to last test beam --- A new fully connected nXYTER board--- An X--Y movement facility was provided exclusively for the GEM ch. --- A better trigger arrangement for efficiency studies.
--- STS, RICH + Panda (parasitic run with Panda) Summary of data taken: 2 ROCs connected to one half of each detector• small cell size in det1 and large cell size in det 2• one day data: Both large pad sizes --- First Day – Problem with SY1527 calibration --- Movement in both X and Y (Beam spot moved and went away)
Aux signals: 2 days data where Aux from different detectors can be correlated (can be used for position resolution) One day data for good AUX (crucial for eff) Trigger data: One run for 10 minutes
Test beam Aug-Sep: 2009
Readout Board for Test beam Aug-Sep 09
Inside view
Outside view
Two triple GEM chambers were built :
det 01 – with two different pad sizes(shown above)
det02 -- same size pads but with larger induction gap
MIP distribution of hit cell
Correlation between GEM1 and GEM2
Position of spots (cell units) from 2 detectors Shown (well-correlated)
ADC distribution of main cell and variation with HV
4 fold increase in ADC for a deltaV(GEM) increase by 50V
PAD multiplicity
• Two back to back detectors similar pad multiplicity..
• No effect of increased induction gap?
(Last day’s data, det2 had low eff, went bad after 3500V)
Depends on beam profile, needs correlating with beam tracker
(Same granularity but different induction gap)
-- no effect of induction gap on the cluster size
Time difference between trigger(aux) and GEM ROC
Offset + Drift time(~150 ns) -- why this large spread ??
Procedure: Select fired GEM cells in 900-1200 nsec after last Aux.
All Aux channels: eff:10% Aux-Channel=2 (4 fold) eff = 71%
---- copied from Sauli’s slides
Efficiency of detector 1 (large pad size)
Using STS hits as reference
-- slides from Bipasha Bhowmick (Calcultta University, India)
Eff_66
Efficiency
HV= 3650 HV= 3750
Looks like the detector takes some time to become stable,-- for HV scan, maybe 2 hours is perhaps short.
-- slides from Bipasha Bhowmick (Calcultta University, India)
Cosmic Ray test setup at VECC
1. Detector+Ortec_142IH +572A+SCA+CFD2. Detector+Ortec_142IH+TFA+CFD3. Using MANAS coupled to PCI CFD card4. Cosmic + Aux and nXYTER
MiddlePMT(3)
TOP PMT(1) LOWER PMT(2)
GEM(4)
P.AMP TFAMANAS
Translator Board Patch Bus cable DAQ
(PCI CFD Card)
Quad COINCQuad CFD
Ch1
Ch2
Ch3
Ch4
2FOLD OUT
Ch1
Ch2
Ch3
Ch4
IN
IN
IN
INOUT
OUT
IN
IN
3FOLD OUT
4FOLD OUT
NIM – TTL Converter
Trigger to DAQ
1.2 micro sec
Delay
Dual Timer
3FOLD IN
Quad Counter
HV is from CAEN N470
Cosmic Setup and test with MANAS
Pedestal
GEM signal connected to Channel 56 of FEE (MANAS)
After pedestal subtraction -
ADC of Channel 56
No of triggers( from 3 FOLD) = 187 Entries =158 => 85%
Results with MANAS
64 channels for 4 MANAS
Thick GEM (THGEM) fabrication and testing first attempt in India
0.5mm thick double-sided copper clad FR4 material. hole size is 0.3mm and the pitch is 1.2mm. made locally.
THGEM – a thicker variant of GEMs(>0.4mm) with 0.3 mm holes and annular etching region of 0.1 mm Main advantages:-- Can be made from normal PCB’s using simple mechanical drilling technique. It “can” be damn cheap relative to GEMs !
-- is free from the complex operation of framing and stretching unlike thin GEMs -- easy to handle and hence more robust Constraints: position resolution ~ 500 microns
10 cm x 10 cm Obstacles: Accuracy in drilling holes and etching of the annular region
0.1 mm 0.5 mm
A closer view of THGEM holes
1.2 mm
The position of the rim is not concentric with the G10 holes and the gap is too little at some places. Lost few boards during tests Fresh Boards ordered – tests going on
“eccentricity” problems
Fe55 Signal from Double THGEM
Not all THGEM boards could give a reasonable energy resolution. --- this could be because of the eccentricity problems. --- we are trying to think of different ways to improve on this.
Preparation for the next beam test
-- Two 3 GEM chambers with following granularity: -- 3 mm x 3 mm 512 pads -- 4 mm x 4 mm 512 pads
-- Get the efficiency problem fully understood using cosmic trigger in lab
-- detector design: The top cover would be sealed via an O-ring instead of the present two component RTV.
Top copperPad area-67*73 Sq mm For 3mm. For 4mm - 88*97 sq mm
Main Features : Both 3 and 4mm square pad sizes Not Staggered (‘09 test beam module) Symmetric Square Pads Multi Layers ( 4) with GND Planes Signal Tracks are distributed in 3 planes
• Reduce the capacitance• Track to Track spacing increases• Reduce Cross talk
Blind Vias for gas integrity Gnd Tracks between Signal Tracks
Bottom copper
Connector with resistors
Top copper
GND Plane
Bottom copper
GND Plane
GND Plane
Connectors for FEBs
Inner 1
Inner 2
33
Chamber PCBS for Test beam 2010
Connectivity Between FEB and ROC
Radiation dose• ROC boards may be affected by this radiation environment• Plan to put the ROC boards 3mt apart from the 0-axis• Detail dose calculation is needed at that point (seems to be falling fast)• The breakdown value of TID is also to be investigated for ROC components
Cable Type• Length of the cable to be known for error free communication• Shielded twisted pair flat type may be a good choice
TID: Total Ionizing Dose at the outer edged of thedetector is around 10krad
Ref : http://cbm-wiki.gsi.de/cgi-bin/viewauth/Radiationstudies/WebHome?CGISESSID=2bce338388a71f099de8d3ca43e0f2b7
10 March 2010 37Physics With FAIR: Indian Perspective,
Susanta K Pal
Tracking station plane
2m
ROC stack
3mt (approx)
Placement of ROC BoardsROC stack
10 March 2010 38Physics With FAIR: Indian Perspective,
Susanta K Pal
Inner 1 Inner-2 Bottom CopperTop copper
Blind vias from inner layers( blue)
Blind vias (red ) to inner layer
2.6 mm square pads
Pads arranged in one block of 32*8=256.
Connected to 300 pin connector.
Tracks - shorter and not closer . can be easily duplicated for
bigger sizes. 40 such FEE Boards for One Slat
of 1mt. Length..
Each block read by 1 FEB with 2/4 n-XYTERs ( 128/64 Channels)
FEBs can be mounted horizontal or vertical
Modular Approach
MUCH PCB design
10 March 2010 39Physics With FAIR: Indian Perspective,
Susanta K Pal
Gas out
Conceptual sketch of Triple GEM chamber module
Gas in
Segmented LV power line/power plane on Detector PCB each power line is feeding 5-FEBs ground plane of LV line is in other layer of PCB
HV
1 mt
10cm
To be decided
LV connector
40 FEBs in one module in 1mt slat with about 10240 channels
10 March 2010 40Physics With FAIR: Indian Perspective,
Susanta K Pal
Chamber PCB4 sq mm pads. 32*32 Array(1024 pads).PCB active area is 135mm *135 mm.Read by 2 chip FEB(256 channels)Basic block=32*8 array. Track lengths are short.
Bottom side
Inner 2 layer
Inner 1 layer
Top side
GND Plane
Sa SAMTEC-300 Pin connectors
2chipFEBs
Chamber PCB with 4 FEBs
Top view with 4 sq mm pads Bottom view –Connectors for FEBs
FEB 1 FEB 4
FEB 2 FEB 3
Bottom view of FEB
Double and Triple GEMs have been assembled at VECC.
Tests performed with radioactive sources as well with proton beams. We are also trying to develop THGEM boards
locally.
Test with proton beams: Double GEM and triple GEMs
coupled to the first prototype of n-XYTER readout chip. – preliminary response looked encouraging. -- charged particle detection efficiency needs to be still higher. investigations underway, using tests with cosmic rays. cross talks issues to be resolved.
Next test beam: two chambers of 3x3 sq. mm 4x4 sq. mm chamber
would require 8 FEBs. May also skip resistor protection
Several layout s of the actual design of the Muon Chamber
are under discussion.
SUMMARY
A 2-GEM ASSEMBLY at VECC – A FIRST ATTEMPT
Frame for GEM gluing(0.5 mm in thickness)
10 cm x 10 cm GEM foil
stretching and gluing Jig
Readout plane-bottom Copper
68 Pin connectorsfor FEB 1nXGen
68 Pin connectors
for FEB 1nXGen
Resistors for input Protection
ERNI Part no 1148054 No –68Pins
Questions remaining from last test beam• Absolute efficiency and HV dependence• Beam intensity dependence • Absolute gain estimate• Uniformity over small zone
New questions:Pad multiplicity/cluster sizePosition resolutionRequired dynamic range before saturation
Induction gap (does it increase cluster size?)