A First Application for the Scalable Readout System: Muon Tomography with GEM Detectors RD51...

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A First Application A First Application for the Scalable for the Scalable Readout System: Readout System: Muon Tomography Muon Tomography with GEM Detectors with GEM Detectors RD51 Collaboration Meeting RD51 Collaboration Meeting WG5 - May WG5 - May 25, 2010 25, 2010 Marcus Hohlmann with Kondo Gnanvo, Lenny Grasso, J. Ben Locke, and Amilkar Quintero Florida Institute of Technology, Melbourne, FL, USA

Transcript of A First Application for the Scalable Readout System: Muon Tomography with GEM Detectors RD51...

Page 1: A First Application for the Scalable Readout System: Muon Tomography with GEM Detectors RD51 Collaboration Meeting WG5 - May 25, 2010 Marcus Hohlmann with.

A First Application for the A First Application for the Scalable Readout System:Scalable Readout System:

Muon Tomography Muon Tomography with GEM Detectorswith GEM Detectors

RD51 Collaboration Meeting RD51 Collaboration Meeting WG5 - May 25, 2010WG5 - May 25, 2010

Marcus Hohlmannwith Kondo Gnanvo, Lenny Grasso, J. Ben Locke, and Amilkar Quintero

Florida Institute of Technology, Melbourne, FL, USA

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Muon Tomography Principle

56FeΘ

Θ

Incoming muons (μ±)

μ

Θ

Θ

μ

Note: angles are exaggerated !

(from natural cosmic rays)

Cargo container

hidden &shieldedhigh-Znuclearmaterial

μ tracks

Regular material:small scattering angles

HEU: Big scattering angles!

μQ=+92e

Q=+26e

Main ideas:

• Multiple Coulomb scattering is ~ prop. to Z and could discriminate materials by Z• Cosmic ray muons are ubiquitous; no artificial radiation source or beam needed• Muons are highly penetrating; potential for sensing shielded high-Z nuclear contraband• Cosmic Ray Muons come in from many directions allowing for tomographic 3D imaging

235U92

26

)1( 1

with)]/ln(038.01[MeV6.13

00

00 ZZ

XXx

X

x

cp

Approx. Gaussian distribution of scattering angles θ with width θ0:Tracking Detector

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Fl. Tech Concept: MT w/ MPGDs

Use Micro Pattern Gaseous Detectors for tracking muons

ADVANTAGES:

small detector structure allows compact, low-mass MT station

• thin detector layers • small gaps between layers• low multiple scattering in detector itself

high MPGD spatial resolution (~ 50 m) provides good scattering angle measurement with short tracks

high tracking efficiency

CHALLENGES:

need to develop large-area MPGDs

large number of electronic readout channels needed (→ SRS)

ΘΘ

~ 1.5 cme-

μ

Readout electronics

Cargo container

hidden &shieldedhigh-Znuclearmaterial

μ tracks

MPGD, e.g. GEM Detector

F. Sauli

MPGD Tracking Detector (GEMs)

GEMDetector

Small triple-GEM under assembly

Gas ElectronMultiplierDetector

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General StrategyGeneral Strategy• Build first prototype of GEM-based Muon Tomography station

& evaluate performance (using ten 30cm 30cm GEM det.)– Detectors– Mechanics – Readout Electronics → SRS !– HV & Gas supply– Data Acquisition & Analysis

• Help develop large-area (1m 0.5m) Triple-GEMs and SRS electronics within RD51

• Build final 1m1m1m GEM-based Muon Tomography prototype station

• Measure performance on shielded targets and “vertical clutter” with both prototypes

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2009/10 Strategy2009/10 StrategyTwo-pronged approach:

1. Build and operate minimal first GEM-based Muon Tomography station:

– only four Triple-GEM detectors (two at top and two at bottom) – temporary GASSIPLEX electronics (~800 ch., borrowed from Saclay – THANKS !!!)– minimal coverage (read out only 5cm 5cm area in each detector)– preliminary data acquisition system (LabView; modified from MAMMA – THANKS !!!)

– Objectives: • take real data as soon as possible and analyze• demonstrate that GEM detectors work as anticipated for cosmic ray muons• → produce very first experimental proof-of-concept for GEM MT

2. Simultaneously prepare for 30cm 30cm 30cm Muon Tomography Station:

– Top, bottom, and side detectors (10 detectors)– Mechanical stand with flexible geometry, e.g. variable gaps b/w detectors– Final SRS front-end electronics (15,000 ch.) with RD51 – Final data acquisition with RD51 & analysis

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Hardware ProgressHardware Progress• Detector Assembly:

– 7 30cm 30cm Triple-GEM detectors assembled in CERN clean rooms – 1 30cm 30cm Double-GEM detector assembled in CERN clean rooms (b/c one foil was lost)– 2 30cm 30cm Triple-GEM detectors awaiting assembly at Fl. Tech– 2 10cm 10cm Triple-GEM detectors assembled at Fl. Tech (for R&D purposes)

• Basic performance parameters of triple-GEM detectors tested with X-rays and mips: – HV stability, sparks– Gas gain – HV plateau– Rate capability

– 55Fe and mip (cosmics) pulse height spectra

• => Six Triple-GEM detectors at CERN show good and stable performance

One Triple-GEM detector has bad HV section; to be fixed

• Built minimal prototype station for Muon Tomography; operated 2 weeks at CERN– Designed and produced adapter board for interfacing detector r/o board with Panasonic connectors

to preliminary “GASSIPLEX” frontend electronics with SAMTEC connectors (Kondo Gnanvo)– Used 8 GASSIPLEX frontend r/o cards electronics with ~800 readout channels for two tests

(Dec ’09 - Jan ’10 and April ’10, Kondo Gnanvo)– Developed LabView DAQ system for first prototype tests – lots of debugging work (Kondo Gnanvo)

• Developed GEANT4 simulation for minimal MT prototype station

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Triple-GEM Detector

768 y-strips

768

x-strips

High voltage board (voltage divider)

HV input (4kV)

Gasinlet

Gasoutlet

HV sections

On X-ray bench at GDD

Triple-GEM pulsesunder 8 keV X-rays

Gate pulsefor ADC

Argon escape

Photo peak

terminators

Single channel meas. with ORTEC pre-amp

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Basic Detector Performance

Results from commissioning test of Triple-GEM detectors using single-channel amp. & 8 kV Cu X-ray source at GDD

MTGEM-7

(lower threshold)

Charge sharing b/w x- and y-strips

Gas gain vs. HV

Rate plateau

2104

At this high voltage, the transfer gap becomes efficient for X-ray detection adding some pulses from the “double-GEM” structure. (Not discharges !)

equal sharin

g

Detector efficient

Anode current – horizontal strips [nA]

Anodecurrent verticalstrips [nA]

Applied Chamber HV [V]

Pulse height spectra

Argonescapepeak

8 keVX-raysMips

(cosmic ray muons)

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Pulse height distribution

Distribution of total strip cluster charge follows Landau distribution as expected

Minimum Ionizing Particles(Cosmic Ray Muons)

Landau Fit

[ADC counts]

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Minimal MT Station

• Pulse heights on x-strips and y-strips recorded by all 4 GEM detectors using preliminary electronics and DAQ

• Pedestals are subtracted• No target present; Data taken 4/13/2010

Setup of first cosmic ray muon run at CERN with four Triple-GEM detectors

Preliminary

Electronics

(GASSIPLEX)

Pb target

3-GEM

Top 1

3-GEM

Top 2

3-GEM

Bottom 2

3-GEM

Bottom 1

Event Display: Tracking of a cosmic ray muon traversing minimal GEM MT station

Top 1 Top 2 Bottom 1 Bottom 2

x

y

Strip Position [mm]

FIT interface board

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First Data: Strip Clusters

Sharing of deposited charge among adjacent strips is important for high spatial resolution by using the center-of-gravity of charge deposition when calculating the hit position:

All recorded strip clusters centered on highest bin & added together

=> Charge is shared between up to 5 strips

Width of Gaussian fitto 855 measured individual strip clusters

=> On the average, strip cluster is 3.2 strips wide (1)

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MT Targets

triggeredtriggered triggered

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Minimal MTS with Pb target

Event recorded with Pb target present in center of minimal MTS:

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Hits & TrackingEmpty Station

Station with Pb target

X-Z projection Y-Z projection

X-Z projection Y-Z proj.

Real Data

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Basic Scattering Reconstruction

• Simple 3D reconstruction algorithm using Point of Closest Approach (POCA) of incoming and exiting 3-D tracks

• Treat as single scatter

• Scattering angle:

(with >0 by definition)

aa

bbbb

aa MT stationMT station

ScatteringObject

μ track direction

Scatteringangle

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Muon Tomography with GEMs !Muon Tomography with GEMs !

16

Muons reconstructed:

Empty 558 Fe 809 Pb 1091 Ta 1617

First-ever experimental GEM-MT Data

Nominal target position

Fe

Pb Ta

empty

Mean scattering angles in x y z = 2mm 2mm 20mm voxels (x-y slices taken at z = 0mm)

It works !!!

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MT Front View (x-z) Empty Fe Pb Ta

<> [deg] <> [deg] <> [deg] <> [deg]

Imaging in the vertical not as good as imaging in x-y because triggered muons are close to vertical

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3D Target ImagingEmpty Fe Pb Ta

[deg]

Scattering points (POCA) colored according to measured scattering angle(Points with < 1o are suppressed for clarity)

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Comparison Data vs. MCComparison Data vs. MC

19

Nominal target position

Fe

Pb Ta

empty

Data

Mean scattering angles in x y z = 2mm 2mm 20mm voxels (x-y slices taken at z = 0mm)

Monte Carlo (~ 20 times data)

empty Fe

Pb Ta

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Comparison Data vs. MC cont’d

Pb

Empty

Ta

Fe

Only data for which the POCA isreconstructed within the MTS volume are used for comparison.

For measurements at small angles ( < 1o), MC and data do not agree that well, yet.

This is presumably due to:

• the fact that the GEM detectors in the MTS have not yet been aligned with tracks. For now, we are solely relying on mechanical alignment.

Any misalignment increases the angle measurement because the scattering angle is by definition positive.

• the fact that the GEANT4 description of the materials used in the station itself is not yet perfect

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Next steps…

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30cm30cm30cm Prototype

31.1cm

31.7cm

All designs by Lenny Grasso; under construction at Fl. Tech

Target plate

GEM su

pport

(with

cut-o

ut)

Front-e

nd card

s

GEM detectoractive area

HV board

Maximizes geometric acceptance

?

? Planned Geometry & Mechanical Design:

“Cubic-foot” prototype

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• originally developed for CMS Si-strip detector by ICL

• production in 2003/04• yield of 120,000 good chip dies• 128 channels/chip• preamplifier/shaper with50ns peaking time

• 192-slot buffer memoryfor each channel

• multiplexed analog output• integrated test pulse system• runs at 40 MHz • used e.g. by CMS, COMPASS,ZEUS, STAR, Belle experiments

MOST IMPORTANT:• Chip is still available • “Cheap” ! (CHF28/chip)

We have procured 160 chips for our ten 30cm × 30cm detectors(min. 120 needed)

HEP group, Imperial College, London

APV25 readout chipAPV25 readout chip

30cm30cm30cm Prototype

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Front-end hybrid cardFront-end hybrid card

APV25

Diodeprotection

for chip

Connectorto chamber

• 128 channels/hybrid• Integrated diode protection against sparks in GEM detector

• Estimated cost: EUR55/card• Plan to get 160 cards for MT• 8 Prototype boards made at CERN

• First on-detector tests performed with MT-GEMs at CERN by Sorin, Hans, Kondo (→ Sorin’s next talk):

HM

HM

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30cm30cm30cm Prototype

Electronics & DAQ under development

Est. cost per electronics channel: $1-2

Prototypes of basically all components exist by now and are under test at CERN by RD51 electronics group

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Plans for 2Plans for 2ndnd half of 2010 half of 20101. Analyze data for minimal station

• Measure performance: resolution, efficiency, muon tomography• Test other reconstruction methods (EM, Clustering) besides POCA on real data• Publish results

2. Build & operate 30cm 30cm 30cm MT prototype with SRS• Help develop DAQ for SRS (→ software!)• Commission all GEM detectors with final SRS electronics & DAQ at CERN• Develop offline reconstruction• Get experimental performance results on muon tracking• Take and analyze lots of Muon Tomography data at CERN• Test performance with shielded targets in various configurations• Ship prototype to Florida and install in our lab; continue MT tests there

3. Development of final 1m 1m 1m MT station• Prepare for using large-area GEM foils (~100cm 50cm):

Adapt thermal stretching technique to large foils• Try to simplify construction technique:

Build small Triple-GEM detectors without stretching GEM foils (using our standard CERN 10cm 10cm detectors, going on now)

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Towards 1m 1m 1m MT station

New infrastructure for stretching GEM foils:• Thermal stretching method (plexiglas frame)• Heating with infrared lamps (40-80oC)• On flat metallic optical bench ( = heat bath) • Everything inside large mobile clean room• Potentially scalable to 1-2 m for large GEMs

New grad students: Mike & Bryant

2m optical bench

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Funding situation

• Good news:– Substantial progress with hardware in 2009/10

and strong support from RD51 have convinced Dept. of Homeland Security to continue project for one more year

– Funding action for June ’10 – May ’11 in progress– Funds for full SRS readout system (15k ch.) for

“cubic-foot” station expected to be available in ‘10– Continuing to fund post-doc (Kondo) and one

grad student (Mike) to work on project

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Acknowledgments

A big to RD51:

– Rui, Miranda for support w/ building the detectors– Esther, Fabien, Maxim, (Saclay) for lending us

the GASSIPLEX cards – twice…– Theodoros (Demokritos) & MAMMA for getting us

started on the LabView DAQ system– Leszek, Serge, Marco & Matteo (GDD) for all the

help with setting up various tests in the GDD lab– Hans & Sorin for all the design, development,

and testing work on the SRS

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Backup Slides

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Triple-GEM design} Top honeycomb plate

} Bottom honeycomb base plate

} Drift cathode and spacer

}}}

} 2D Readout Foilwith ~1,500 strips

Follows originaldevelopment forCOMPASS exp.& further develop-ment for TERA

3 GEM foils stretched & gluedonto frames/spacers

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Minimal MT stationMinimal MT station

32

Setup at GDD in April 2010

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Beyond FY10… Beyond FY10…

4/16/2010 M. Hohlmann, Fl. Inst. of Technology - DNDO review #7, Washington, D.C. 33

(, X-ray, charged particles)

Large photosensitive GEM Detector (100-200 keV ’s) ?

Fl. Tech – U. Texas, Arlington planned joint effort (Physics & Material Science Departments)

Muon Tomography with

integrated -detection ?