A Readout System Utilizing the APV25 ASIC for the Forward GEM Tracker in STAR

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A Readout System Utilizing the APV25 ASIC for the Forward GEM Tracker in STAR G. J. Visser 1 , J. T. Anderson 2 , B. Buck 3 , A. S. Kreps 2 , T. Ljubicic 4 1 Indiana University Center for Exploration of Energy and Matter, USA 2 Argonne National Laboratory, USA 3 Massachusetts Instituteof Technology, USA 4 Brookhaven National Laboratory, USA Introduction The Forward GEM Tracker (partially installed and commissioning now in STAR Run 12) will extend STAR’s tracking reach to η=2 (covering the Endcap EMC), enabling charge sign discrimination for e + /e from W +/− decay. When studied with longitudinally polarized proton beams, W production parity violating asymmetries are an ideal tool to study the spin-flavor structure of the proton and hence an important part of the spin physics program at STAR. The FGT, located inside the inner field cage of the STAR Time Projection Chamber (TPC), is a set of six independent triple-GEM detector disks, consisting of four independent quadrants pinned to a common support. For each quadrant, contained in its own working gas pressure volume with independent bias voltage divider board, a planar strip / pad (two dimensional readout) padplane fabricated on kapton film with two copper layers is used, in conjunction with the triple GEM structure, to detect the ionization signal of charged particle tracks and provide high spatial resolution (<100 µm) readout. The outer (inner) radius of the active area of an FGT quadrant is 381 (115) mm, while the perimeter frame is only 13 mm wide. The “Phi- projection” of charge is sensed with 720 strips on the padplane, while the “R-projection” of charge is sensed with 560 “lines” of pads interconnected with lines on the routing layer of the padplane, for a total of 1280 channels per quadrant. The front-end electronics assemblies, described in detail in section II, Fig. 2. The FGT front-end board. The layout of the readout interface signals is symmetric to the two ends of the board, since it is used in both orientations on the FGT detector. The 640 input signal route to 640 card-edge connector pads along the bottom edge. Ground is connected from the detector to the two pressfit nuts soldered to pads on either side of the middle APV chip. effectively “straddle” the gap between quadrants, with four front-end assemblies per disk, and a common ground for the whole disk. This ground is locally isolated from the other disks and the support structures; each of the disks is grounded through its front-end cables to the substantial clean gr This work was supported in part by the Offices of NP and HEP within the U.S. DOE Office of Science and by the U.S. NSF. Design choices Some compromises are necessary for maximum channel density. The analog signal path must be kept relatively simple. In particular: •A passive shaper uses no power, little board area •An ADC driver stage is not necessary if we can keep the drive impedance reasonably low without it •Differential drive is not necessary if the ADC uses a (relatively) high VDD and if we can tolerate a little nonlinearity However we do not compromise on the line receiver, this is the most crucial element. It is important to: •Receive differential signal accurately •Not inject common-mode ground noise back to cable & front end electronics •Equalize cable frequency response Receiver / freq eq. Shaper ADC σ = 5.62 (12-bit: 1.40) 11.5 ENOB Open input: Typical cluster in R projection (timebin on X axis) 15 MHz* sine input, single event 100 pt readout 21 hostile (red) and 1 hostile (blue & brown) Indicates ~2% crosstalk in neighbor channels, acceptable but will try to reduce with layout improvements DAC per channel σ = 0.43 σ = 0.52 Noise and linearity are evaluated with open input and with 14.9 MHz sine input. Nonlinearity ≈ 0.05 % ADC FE FIFO ADC FE FIFO … (36 ch total) ADC FE FIFO ADC FE FIFO ADC FE FIFO ADC FE FIFO ADC FE FIFO … (36 ch total) ADC FE FIFO ADC FE FIFO ADC FE FIFO Mezzanine board Main board Processor FPGA Output FIFO VME slave 2eSST etc. Each 160 MB/s i.e. 400 words/evt @ 200 kHz 160 MB/s 1 MB 320 MB/s FE (Front-end processing): This includes acquisition buffer writing, point extraction, lookahead zero suppression, channel number & header insertion Channel data FIFO: 1024 words (16 bits + 2 flags, internal use only) XC3SD3400A-4 Frontend FPGA XC3S500E-4 12 total, 6 ch each The bottom line… Noise and nonlinearity opto- isolated I 2 C master (2×) cable to FEE Complete integrated readout and power system for FGT Current status • 3 modules assembled & tested • Interim firmware (FE deadtime, no block transfers) • Deployed in support of CDC and FDC development Next steps: • Full deadtimeless readout, 2eSST transfers • Minor changed to layout (obsolence, crosstalk) • Develop production test • Pre-production run (20 modules) in early 2011 • 188 modules (+spares) in 2012 ADC (quad) frontend FPGA Crosstalk Single event 1000 pt readout *Corresponds to peaking time ≈33 ns for combined system (preamp, cable, ADC) Readout module for 2×12 APV (3072 det. channels) The PCB is 10 layers w/ 6 planes (3 GND), 0.003” buried capacitance. GAS II: A Versatile Wire Chamber Readout ASIC. N. Dressnandt, N. Doshi, M. Newcomer., IEEE NSS 2009. http:// www.star.bnl.gov/ System response Preamp + 18 m cable + ADC main FPGA analog line receiver / filter to readout / control backplane (CPCI style) FEE Power Supply ±1.8V 2.5A remote reg. 0 – 360° clock phase shifter (4×) for APV & ADC cable to FEE

description

A Readout System Utilizing the APV25 ASIC for the Forward GEM Tracker in STAR. G. J. Visser 1 , J. T. Anderson 2 , B. Buck 3 , A. S. Kreps 2 , T. Ljubicic 4 1 Indiana University Center for Exploration of Energy and Matter, USA 2 Argonne National Laboratory, USA - PowerPoint PPT Presentation

Transcript of A Readout System Utilizing the APV25 ASIC for the Forward GEM Tracker in STAR

Page 1: A Readout System Utilizing the APV25 ASIC for the Forward GEM Tracker in STAR

A Readout System Utilizing the APV25 ASIC for the Forward GEM Tracker in STAR

G. J. Visser1, J. T. Anderson2, B. Buck3, A. S. Kreps2, T. Ljubicic4

1Indiana University Center for Exploration of Energy and Matter, USA2Argonne National Laboratory, USA

3Massachusetts Instituteof Technology, USA4Brookhaven National Laboratory, USA

IntroductionThe Forward GEM Tracker (partially installed and

commissioning now in STAR Run 12) will extend STAR’s tracking reach to η=2 (covering the Endcap EMC), enabling charge sign discrimination for e+/e− from W+/− decay. When studied with longitudinally polarized proton beams, W production parity violating asymmetries are an ideal tool to study the spin-flavor structure of the proton and hence an important part of the spin physics program at STAR.

The FGT, located inside the inner field cage of the STAR Time Projection Chamber (TPC), is a set of six independent triple-GEM detector disks, consisting of four independent quadrants pinned to a common support. For each quadrant, contained in its own working gas pressure volume with independent bias voltage divider board, a planar strip / pad (two dimensional readout) padplane fabricated on kapton film with two copper layers is used, in conjunction with the triple GEM structure, to detect the ionization signal of charged particle tracks and provide high spatial resolution (<100 µm) readout. The outer (inner) radius of the active area of an FGT quadrant is 381 (115) mm, while the perimeter frame is only 13 mm wide. The “Phi-projection” of charge is sensed with 720 strips on the padplane, while the “R-projection” of charge is sensed with 560 “lines” of pads interconnected with lines on the routing layer of the padplane, for a total of 1280 channels per quadrant. The front-end electronics assemblies, described in detail in section II,

Fig. 2. The FGT front-end board. The layout of the readout interface signals is symmetric to the two ends of the board, since it is used in both orientations on the FGT detector. The 640 input signal route to 640 card-edge connector pads along the bottom edge. Ground is connected from the detector to the two pressfit nuts soldered to pads on either side of the middle APV chip.

 effectively “straddle” the gap between quadrants, with

four front-end assemblies per disk, and a common ground for the whole disk. This ground is locally isolated from the other disks and the support structures; each of the disks is grounded through its front-end cables to the substantial clean gr

This work was supported in part by the Offices of NP and HEP within the U.S. DOE Office of Science and by the U.S. NSF.

Design choicesSome compromises are necessary for

maximum channel density. The analog signal path must be kept relatively simple.

In particular:

•A passive shaper uses no power, little board area

•An ADC driver stage is not necessary if we can keep the drive impedance reasonably low without it

•Differential drive is not necessary if the ADC uses a (relatively) high VDD and if we can tolerate a little nonlinearity

However we do not compromise on the line receiver, this is the most crucial element. It is important to:

•Receive differential signal accurately•Not inject common-mode ground noise back

to cable & front end electronics•Equalize cable frequency response

Receiver / freq eq.Shaper

ADC

σ = 5.62 (12-bit: 1.40)11.5 ENOB

Open input:

Typical cluster in R projection (timebin on X axis)

15 MHz* sine input, single event 100 pt readout

21 hostile (red) and 1 hostile (blue & brown)

Indicates ~2% crosstalk in neighbor channels, acceptable but will try to reduce with layout improvements

DAC per channel

σ = 0.43 σ = 0.52

Noise and linearity are evaluated with open input and with 14.9 MHz sine input.

Nonlinearity ≈ 0.05 %

ADC FE FIFO

ADC FE FIFO

… (36 ch total) …

ADC FE FIFO

ADC FE FIFO

ADC FE FIFO

ADC FE FIFO

ADC FE FIFO

… (36 ch total) …

ADC FE FIFO

ADC FE FIFO

ADC FE FIFO

Mezzanine board

Main board

Processor FPGA

Output FIFO

VME slave

2eSST etc.

Each 160 MB/s i.e. 400 words/evt @ 200 kHz

160 MB/s

1 MB

320 MB/s

FE (Front-end processing):This includes acquisition buffer writing, point extraction, lookahead zero suppression, channel number & header insertion

Channel data FIFO:1024 words (16 bits + 2 flags, internal use only)

XC3SD3400A-4

Frontend FPGA

XC3S500E-4

12 total, 6 ch each

The bottom line…

Noise and nonlinearity

opto-isolated I2C master (2×)

cable to FEE

Complete integrated readout and power system for FGT

Current status• 3 modules assembled & tested• Interim firmware (FE deadtime, no block transfers)• Deployed in support of CDC and FDC development• Next steps:

• Full deadtimeless readout, 2eSST transfers• Minor changed to layout (obsolence, crosstalk)

• Develop production test• Pre-production run (20 modules) in early 2011

• 188 modules (+spares) in 2012

ADC (quad)

frontend FPGA

Crosstalk

Single event 1000 pt readout

*Corresponds to peaking time ≈33 ns for combined system (preamp, cable, ADC)

Readout module for 2×12 APV (3072 det. channels) The PCB is 10 layers w/ 6 planes (3 GND), 0.003” buried capacitance.

†GAS II: A Versatile Wire Chamber Readout ASIC. N. Dressnandt, N. Doshi, M. Newcomer., IEEE NSS 2009.

http://www.star.bnl.gov/

System responsePreamp + 18 m cable + ADC

main FPGA

analog line receiver / filter

to readout / control backplane(CPCI style)

FEE Power Supply ±1.8V 2.5A remote reg.

0 – 360° clock phase shifter (4×) for APV & ADC

cable to FEE