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

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Presentation transcript:

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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 2 Muon Tomography Principle 56 Fe Θ Θ Incoming muons (μ ± ) μ Θ Θ μ Note: angles are exaggerated ! (from natural cosmic rays) Cargo container hidden & shielded high-Z nuclear material μ tracks Regular material: small scattering angles HEU: Big scattering angles! μ Q=+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 235 U Approx. Gaussian distribution of scattering angles θ with width θ 0 : Tracking Detector

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 3 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) Θ Θ ~ 1.5 cm e-e- μ Readout electronics Cargo container hidden & shielded high-Z nuclear material μ tracks MPGD, e.g. GEM Detector F. Sauli MPGD Tracking Detector (GEMs) GEM Detector Small triple-GEM under assembly Gas Electron Multiplier Detector

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 44 General 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 1m  1m  1m GEM-based Muon Tomography prototype station Measure performance on shielded targets and “vertical clutter” with both prototypes

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany /10 Strategy Two-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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 66 Hardware 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 – 55 Fe 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 77 Triple-GEM Detector 768 y-strips 768 x-strips High voltage board (voltage divider) HV input (4kV) Gas inlet Gas outlet HV sections On X-ray bench at GDD Triple-GEM pulses under 8 keV X-rays Gate pulse for ADC Argon escape Photo peak terminators Single channel meas. with ORTEC pre-amp

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 88 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 2  10 4 At this high voltage, the transfer gap becomes efficient for X-ray detection adding some pulses from the “double-GEM” structure. (Not discharges !) equal sharing Detector efficient Anode current – horizontal strips [nA] Anode current vertical strips [nA] Applied Chamber HV [V] Pulse height spectra Argon escape peak 8 keV X-rays Mips (cosmic ray muons)

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 99 Pulse height distribution Distribution of total strip cluster charge follows Landau distribution as expected Minimum Ionizing Particles (Cosmic Ray Muons) Landau Fit [ADC counts]

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 10 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 11 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 fit to 855 measured individual strip clusters => On the average, strip cluster is 3.2 strips wide (  1  )

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 12 MT Targets triggered

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 13 Minimal MTS with Pb target Event recorded with Pb target present in center of minimal MTS:

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 14 Hits & Tracking Empty Station Station with Pb target X-Z projection Y-Z projection X-Z projection Y-Z proj. Real Data

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 15 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) a bb a MT station Scattering Object μ track direction Scattering angle

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 16 Muon Tomography with GEMs ! 16 Muons reconstructed: Empty 558 Fe 809 Pb1091 Ta1617 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 !!!

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 17 MT Front View (x-z) Empty FePbTa [deg] Imaging in the vertical not as good as imaging in x-y because triggered muons are close to vertical

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 18 3D Target Imaging Empty FePbTa  [deg] Scattering points (POCA) colored according to measured scattering angle (Points with  < 1 o are suppressed for clarity)

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 19 Comparison 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 20 Comparison Data vs. MC cont’d Pb Empty Ta Fe Only data for which the POCA is reconstructed within the MTS volume are used for comparison. For measurements at small angles (  < 1 o ), 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 21 Next steps…

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 22 30cm  30cm  30cm Prototype 31.1cm 31.7cm All designs by Lenny Grasso; under construction at Fl. Tech Target plate GEM support (with cut-out) Front-end cards GEM detector active area HV board Maximizes geometric acceptance ? ? Planned Geometry & Mechanical Design: “Cubic-foot” prototype

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 23 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 with 50ns peaking time 192-slot buffer memory for 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 chip 30cm  30cm  30cm Prototype

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 24 Front-end hybrid card APV 25 Diode protection for chip Connector to 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 25 30cm  30cm  30cm 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 26 Plans for 2 nd half of 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)

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 27 Towards 1m  1m  1m MT station New infrastructure for stretching GEM foils: Thermal stretching method (plexiglas frame) Heating with infrared lamps (40-80 o C) 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 28 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 29 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

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 30 4/16/2010 M. Hohlmann, Fl. Inst. of Technology - DNDO review #7, Washington, D.C. 30 Backup Slides

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 31 Triple-GEM design } Top honeycomb plate } Bottom honeycomb base plate } Drift cathode and spacer } } } } 2D Readout Foil with ~1,500 strips Follows original development for COMPASS exp. & further develop- ment for TERA 3 GEM foils stretched & glued onto frames/spacers

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 32 Minimal MT station 32 Setup at GDD in April 2010

5/25/2010 M. Hohlmann, Florida Institute of Technology - RD51 Coll. Meeting, Freiburg, Germany 33 Beyond FY10… 4/16/2010 M. Hohlmann, Fl. Inst. of Technology - DNDO review #7, Washington, D.C. 33 Large photosensitive GEM Detector ( keV  ’ s) ? Fl. Tech – U. Texas, Arlington planned joint effort (Physics & Material Science Departments) Muon Tomography with integrated  -detection ?