Florida Institute of Technology, Melbourne, FL

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Presentation transcript:

Florida Institute of Technology, Melbourne, FL Status of the Medium-Sized SRS Readout Electronics for Muon Tomography using GEMs Kondo GNANVO Florida Institute of Technology, Melbourne, FL

K. Gnanvo - RD51 Coll. Meeting -CERN April 2011 OUTLINE Cosmic Ray Muon Tomography (MT) using GEMs MT station prototype with the medium-size SRS Electronics DATE with UDP for the data acquisition AMORE for monitoring and data analysis Preliminary results of Cosmic ray Muons Data with GEM/SRS Conclusion & Perspectives 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Cosmic Ray Muon Tomography (MT) using GEMs Application To detect high-Z material smuggled Measurement of the deflection of cosmic muon by the material through Multiple Coulomb scattering Need large area detectors with excellent position to track the cosmic muons => GEMs Proof of the concept with minimal MT station prototype (2009) K. Gnanvo & al .“Imaging of high-Z material with a minimal prototype of a Muon Tomography station based on GEM detectors for nuclear contraband detection.”, Nucl. Instr. and Meth. A (2011), doi:10.1016/j.nima.2011.01.163 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

MT Station with the Medium-Sized SRS Electronics Full Cubic foot size MT Station 30 x 30 cm2 GEM detectors 10 chambers: top, bottom & side station SRS + APV chips: read out ~16K channels Scintillator / PMT for external trigger DATE + AMORE for daq & analysis GEM chamber 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Medium-size SRS Electronics for Muon Tomography Trigger PMT Power supply Network switch GEM test setup Back side of SRS FEC interface Front side of SRS: C-Cards interface HV supply for the GEMs DATE and AMORE PC 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

K. Gnanvo - RD51 Coll. Meeting -CERN April 2011 DATE Framework with UDP equipment for the SRS Data Acquisition (Filippo Costa, ALICE DAQ) DATE: ALICE DAQ software Data Acquisition & Test Environment on Linux SLC5 Many features available , user friendly GUI for run control environment, basic online monitoring of the raw data, electronic logbook. Data transfer to the DATE PC through Gigabit Ethernet via UDP: One Ethernet port on the FE card connected to another port on the DATE PC via a copper cable or optical fiber cable data, (1Gb/s to 10 Gb/s throughput) Network switch to handles as many as the 8 UDP ports for MT application 4 tested so far successfully Some configuration issues with the Ethernet switch to be addressed for data transfer with more than 5 cards “Slow Control” for the system configuration C script for Initialization of the FEC, ADC boards, APV hybrids and the network configuration … DATE execute the C-code at Start of Run to configure the system 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

AMORE for monitoring and data analysis AMORE is ALICE Data Quality Monitoring Software framework Automatic MonitoRing Environment founded on ROOT & DATE Monitoring Library Communication between publisher and clients through DIM a publish/subscribe system developed at CERN Flexibility to do offline data analysis (pedestal subtraction, zero suppression …) Simple POCA reconstruction algorithm will be integrated for real time imaging of the Muon Tomography scenario 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Preliminary results: Pedestal run Baseline correction, pedestal subtraction, zero suppression First step: computation of raw pedestal data Pedestal offset needed to correctly calculate the baseline correction data Second step: common mode offset calculated for each time frame for each event Accurate common mode offset requires the raw pedestal offset data as input Third step: Computation of fine pedestal data Meeds the common mode offset data of step#2 correction, pedestal offset subtraction Pedestal data are stored in root files and uploaded by AMORE before the start of run Pedestal offset for APV no2 Pedestal noise for APV no2 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Preliminary results: Zero suppression The zero suppression is performed at 3 sigma of the pedestal noise for each channel Accurate zero suppression required common mode correction for each time frame for each event Raw data After pedestal subtraction After zero suppression Time resolution Strip Number 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Preliminary results: Test of GEM1 2D hit distribution 2D charge distribution X/Y charge sharing MIP spectrum Cluster size distribution Cluster multiplicity Mean cluster size = 5 25% multi hit events 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Preliminary results: APV channel crosstalk Double muon hits APV channel crosstalk 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Preliminary results: APV channels cross talk Double hits position correlation crosstalk position correlation crosstalk at stripNo ± 32, 96 Double hits charge correlation crosstalk charge correlation Ratio = hit /crosstalk Ratio = 40 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Preliminary results: Missing Hits 50% of the events record hit on only one axis of the detector Happens equally on X or Y plane and also equally for all 12 hybrids. Not a hit lost during zero suppression Not software related No packet lost during data transfer to DATE or bug in AMORE analysis code We suspect a problem external trigger input signal to the 4 FEC boards Maybe trigger signal jitter in the NIM fan out module or inside the FEC board Data lost due to the delay causes by the jitter We are investigating the issue. X-plane Y-plane 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011

Conclusion & Perspective Where we are now We have successfully tested the medium size SRS electronic system with a commercial network switch supporting 9KB jumbo frames We took up to 600 Gb data with the 4 FEC/ADC cards and 16 APVs DATE and AMORE used with the UDP equipment implemented by ALICE DAQ team A very advanced data analysis tool based on AMORE is tested and available for SRS users We still have some few issues to address i.e. the data transfer via e network switch with more than 4 FEC/C-card Some tuning of the trigger delay in each card to avoid the missing hits Where we want to be in the next few weeks The production APV25 hybrids is on going at Hybrid SA company and a first batch is going to be tested on site on Monday 04/18 We will hopefully get 300 hybrids by early May (160 for MTS Florida Tech) We plan to equip our 10 detector with this system to mount a cubic foot size MTS for the next round of cosmic ray muons data taking 14/04/2011 K. Gnanvo - RD51 Coll. Meeting -CERN April 2011