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Sensor and Readout Status of the PIXEL Detector. Talk Structure. Sensors Readout Development and Prototyping with test results. IPHC Functional Sensor Development. All sensor families:. 30 x 30 µm pixels CMOS technology Full Reticule = 640 x 640 pixel array.
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Sensor and Readout Status of the PIXEL Detector Leo Greiner 2007-09-11 TC_Int
Talk Structure • Sensors • Readout • Development and Prototyping with test results Leo Greiner 2007-09-11 TC_Int
IPHC Functional Sensor Development All sensor families: • 30 x 30 µm pixels • CMOS technology • Full Reticule = 640 x 640 pixel array Mimostar 2 => full functionality 1/25 reticule, 1.7 µs integration time (1 frame@50 MHz clk), analog output. (in hand and tested) Phase-1 and Ultimate sensors => digital output (in development) Data Processing in RDO and on chip by generation of sensor. The RDO system design evolves with the sensor generation. Leo Greiner 2007-09-11 TC_Int
HFT PIXEL Readout Functional Goals • Triggered detector system fitting into existing STAR infrastructure (Trigger, DAQ, etc.) • Deliver full frame events to STAR DAQ for event building at approximately the same rate as the TPC (1 KHz for DAQ1000). • Reduce the total data rate of the detector to a manageable level (< TPC rate). • Reliable, robust, cost effective, etc. Leo Greiner 2007-09-11 TC_Int
Mimostar Data Flow System Goal: 10 Sensors / Ladder 33 Ladders 135M Pixel Leo Greiner 2007-09-11 TC_Int
Raster scan Data examined Per clock cycle Implemented in FPGA on daughter card Leo Greiner 2007-09-11 TC_Int
Cluster Finder Efficiency Real Data taken with MIMOSTAR2 detectors by IPHC Traditional ADC Sum Method 2 Threshold FPGA method Cut on the central pixel goes from 14 to 8 ADC counts (left to right) every 1 ADC. 1 ADC = 7.1 e-. Leo Greiner 2007-09-11 TC_Int
PIXEL Data Rates (1 KHz) • Rate @ R1 (2.5cm) = 52.9 / cm2 • Rate @ R2 (6.5cm) = 10.75 / cm2 • Rate @ R3 (7.5cm) = 8.76 / cm2 (at L = 1027) • Average event size = 114 KB • Data Rate = 114 MB/sec at 1KHz • 33 fibers • 33 RORC (6 readout PCs) Leo Greiner 2007-09-11 TC_Int
Prototype 3 Sensor Telescope We tested the functionality of a prototype MIMOSTAR2 detector at the LBNL ALS and then in the environment at STAR during the last three weeks of the 2006-2007 run at RHIC. Our goal was to gather information on: • Charged particle environment near the interaction region in STAR. • Performance of our cluster finding algorithm. • Performance of the MIMOSTAR2 sensors. • Functionality of our interfaces to the other STAR subsystems. • Performance of our hardware / firmware as a system. • The noise environment in the area in which we expect to put the final PIXEL detector. Leo Greiner 2007-09-11 TC_Int
Telescope Electronics / RDO MimoStar2 chips on kapton cables MOTHER BOARD DAUGHTER CARD Control PC (Win) STRATIX Acquisition Server (Linux) Leo Greiner 2007-09-11 TC_Int RORC SIU
Telescope Sensors and Mechanical Housing 3 MIMOSTAR2 chips mounted as close together as reasonably possible on low mass kapton cables in a telescope configuration. Leo Greiner 2007-09-11 TC_Int
Mimostar2 Telescope test at the ALS 1.2 GeV electrons at the ALS Booster Test Facility Important Due to un-terminated DAC pads on the sensor, our noise level was double the value achieved under ideal conditions at IPHC in France. IPHC =>11-15 electrons at 30º C LBL => 30-35 electrons at 28º C MPV = 49 (Standard) and 43 (Radtol) ADC counts at ~230 electrons Leo Greiner 2007-09-11 TC_Int
Efficiency and Accidental rates for ALS test Merged cluster data – typically 2-3 hits per cluster. Increased noise in sensors results in reduced performance. Leo Greiner 2007-09-11 TC_Int
Telescope Installed at STAR Magnet Pole Tip Beam Pipe Electronics Box Telescope head – 1.45 m from interaction point just below beam pipe. Leo Greiner 2007-09-11 TC_Int
STAR Prototype Run Results Typical CDS full frame event in one sensor. Clusters are clearly visible above the noise level. • Measured charged particle flux was ~ 3.9 merged clusters per sensor (1.7 µs integration time, L=81026 cm-2s-1). • Noise level of system in the STAR environment was 7.48 ADC counts, comparable to laboratory and ALS measurements. • Prototype system integrated with STAR Trigger, slow control and run control sub-systems. Events delivered to DAQ standard RDO PC. • TLD measured dose at head position, 325 rad over running time. This scales to an integrated dose of several hundred Krad / run. Leo Greiner 2007-09-11 TC_Int
Distribution of track angles in Mimostar2 telescope Leo Greiner 2007-09-11 TC_Int
Summary for beam runs • RDO system with data sparsification implemented and functional for Mimostar2 sensors. • Prototype system characterized, but with increased noise. • Fully functioning interfaces between our prototype detector and STAR detector infrastructure. • Completed measurements of detector environment at STAR including induced electronic noise. Leo Greiner 2007-09-11 TC_Int
Some tasks and milestones for the next year • August 2008 – delivery of Phase-1 sensors from the foundry. • Develop new generation RDO system based on Virtex-5 FPGA. • Testing of Mimostar2, Mimostar3 and Mimosa22e sensors. • Prototype low radiation length cable. Leo Greiner 2007-09-11 TC_Int
fin Leo Greiner 2007-09-11 TC_Int