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GLAST LAT Project March 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area GLAST Large Area Telescope: Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and Status Robert Johnson Santa Cruz Institute for Particle Physics University of California at Santa Cruz Tracker Subsystem Manager Gamma-ray Large Gamma-ray Large Area Space Area Space Telescope Telescope

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Page 1: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 1

GLAST Large Area Telescope:GLAST Large Area Telescope:

Tracker SubsystemWBS 4.1.4

2A: Electronics Design and Status

Robert JohnsonSanta Cruz Institute for Particle PhysicsUniversity of California at Santa CruzTracker Subsystem Manager

[email protected]

Gamma-ray Large Gamma-ray Large Area Space Area Space TelescopeTelescope

Page 2: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 2

TKR Electronics RequirementsTKR Electronics Requirements

• Details of the requirements are in released LAT documents:– LAT-SS-17 Level-3 Performance requirements– LAT-SS-134 Level-4 Mechanical & Thermal

requirements– LAT-SS-152 Level-4 Electronics requirements

• The major challenges are– Low power: <168 W of conditioned power

• Less than 0.29 W per MCM or 190 W/channel• The flight design achieves 0.25 W per MCM!

– Low noise occupancy: (noise trigger rate <500 Hz)• The trigger requires occupancy less than 5/100,000

ch/trigger• Readout and onboard processing requires <1/10,000

ch/trigger• The beam-test/balloon flight tracker achieved much better…

– Compact packaging: bring signals around the tray corner– Manufacturing and QC: 884,736 channels, >98% functional– Reliability: design, redundancy, testing

Page 3: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 3

Some Detailed RequirementsSome Detailed Requirements

• Internal charge injection for calibration and test, with pulse-height control and arbitrary selection of channels.

• Threshold uniformity: <15 mV rms across 64 channels.• Threshold control per GTFE chip by an internal DAC.• Dead time & Readout speed: less than 10% at 10 kHz

cosmic rate.• TOT: measure up to 4 MIPs. • Non-destructive readback of configuration registers.• Error checking: event alignment; command & data parity.• Layer-OR jitter <250 ns for a charge deposit > 0.5 MIP.• Reliability:

– Redundant readout paths.– Redundant power paths.– Protection against power shorts.

• Radiation hardness: 4 kRad TID; >37 MeV/mg/cm2 SEL thresh

• Passive cooling; temperature monitoring.

Page 4: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 4

Tracker Readout ArchitectureTracker Readout ArchitectureEmphasis on compactness, minimum of wiring, and redundancy:• Serial, LVDS readout and control lines on flat flex-circuit cables.• Either of the two communications cables can fail without affecting the other.• Two readout and control paths for every 64-channel front-end chip.• Any single chip can fail without preventing the readout of any other.

24 64-channel amplifier-discriminator chips for each detector layer

2 readoutcontroller chipsfor each layer

Con

trol

sig

nal f

low

Control signal flow

Data flow to FPGAon DAQ TEM board.

Data flow to FPGAon DAQ TEM board.

Control signal flow

Data flow

Nine detector layers are read out on each side of each tower.

GTRC

GTFEGTFE

GTRC

GTRC

GTRC

GTRC

GTRC

9-998509A22

• Trigger output = OR of all 1536 channels in a layer.

• Upon trigger (6-fold coincidence) data are latched into a 4-event-deep buffer in each front-end chip.

• Read command moves data into 1 of 2 GTRC buffers.

• Token moves data from GTRCs to TEM.

Page 5: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 5

Tracker Readout ArchitectureTracker Readout Architecture

• Block diagram of the ends of two readout layers and their connections to the TEM

– Clock, Command, Trigger, and Reset are bussed to the GTRC chips

– Token and Data daisy-chain up and down the 9 layers

– Each layers sends its Layer-OR directly to the TEM

– The TEM communicates only with the GTRC chips, always by serial LVDS.

– The GTRC communicates with 24 GTFE chips on the MCM.

TEM

NTREQ

NTACK

NSCMD

CLK

NRESET

TO

KE

N

NS

DA

TA

TACKB

SCMD_OUT

CLKB

CTRLREG

TREQ_IN

RD_IN

NT

OK

EN

_OU

T

NS

DA

TA

_IN

GTRC

GTFE

A3

A2

A1

A0

LEFT

RESETO

RESETB

RESETB

NTREQ

NTACK

NSCMD

CLK

NRESET

TO

KE

N

NS

DA

TA

TACKB

SCMD_OUT

CLKB

CTRLREG

TREQ_IN

RD_IN

NT

OK

EN

_OU

T

NS

DA

TA

_IN

GTRC

GTFE

A3

A2

A1

A0

LEFT

Page 6: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 6

MCM Readout Module ConfigurationMCM Readout Module Configuration

• 8-layer polyimide PWB• Top edge thickened and machined to a

0.64 mm radius• 1-layer flex circuit (“pitch adapter”)

bonded over the radius• Fully encapsulated wire bonds• Conformal coating• 2 Omnetics nano connectors• Steel mounting screws + adhesive

Readout IC

Machined corner radius with flex circuit bonded around the curve

TMCM, attached by screws

Detector

Tray Structure

Bias circuit

High-thermal conductivity transfer adhesive

Readout IC

Machined corner radius with flex circuit bonded around the curve

TMCM, attached by screws

Detector

Tray Structure

Bias circuit

High-thermal conductivity transfer adhesive

Machined corner radius with flex circuit bonded around the curve

TMCM, attached by screws

Detector

Tray Structure

Bias circuit

High-thermal conductivity transfer adhesive

24.58mm18.0mm

359.0mm

Grounding Screws3 Total

Mounting Screws, 1 of 8

Connector, 1 of 2

GTFE, 1 of 24GTRC, 1 of 2

Page 7: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 7

MCM PWB Layout ConceptMCM PWB Layout Concept

• Low-noise environment for the amplifier chips

• 8 layers are used for good analog/digital separation plus low-impedance ground and power planes.

• Analog and digital traces are well separated and never wrap around each other.

• Power planes and split analog/digital GND planes

• Complete planes are also used for the SSD bias and AVDD2low impedance path to the decoupling caps for the SSD signal return.

Analog Traces and Planes

Digital TracesDigital Pwr/Gnd

Analog PwrAnalog Gnd

ICR, C, etc.Stackup and

arrangement of conductors in the PWB

1. Digital traces; SMT parts; ASICs

2. Digital busses

3. Split digital/analog power

4. Split digital/analog ground

5. Analog ground

6. Analog traces from ASICs to the SMT parts

7. AVDD2 (analog 1.5V)

8. Detector bias

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2A Tracker Peer Review, WBS 4.1.4 8

Pitch AdapterPitch Adapter

• 1-layer Kapton flex circuit• Ni + Au plating for wire bonding• Precision tooling holes (not

shown)• Circuit & traces are trimmed to

length after bonding to the PWB (see Presentation 6E)

SS

D S

ide

(2

28

m

pitch)

AS

IC S

ide

“ground”

Bias HV

Page 9: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 9

F.E. Readout Chip (GTFE)F.E. Readout Chip (GTFE)

• Schematics-based design, using standard cells for logic.

• Standard-cell I/O pad ESD protection.

• Manual layout of the analog channel, I/O cells, memory, global routing.

• Automated place-and-route of the logic blocks.

• Design verification: Spice and gate level simulations; DRC; LVS; simulation of the final extracted netlist in Nanosim.

64 amplifier-discriminator channels.

4-deep event memory (addressed by TEM)Custom layout 2 custom DACs

Trigger and Data mask registersStandard-cell auto route

Control logic, command decodersStandard-cell auto route

Cap

Calibration mask and capacitors

I/O pads and protection structures

Page 10: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 10

GTFE Block DiagramGTFE Block Diagram

S

OUT

A

B

64

64

64

641

2D

C

Q

D

C

Q

LEFT/RIGHT

DEAFMODE

DATA OUT

64

67 X 4

EVENT BUFFER

2

2

W_ADDR

R_ADDR

WRITE STROBE

L1T

READ CMD

WRITE

CONTROL

READ

CONTROL

LOAD

DATAFROM

PREVIOUSGTFE

DATA READ SHIFT REGISTER

DATA MASK & READOUT REGISTER

TRIGGER MASK & READOUT REGISTER

DISCRIMINATORS

SHAPERS

PREAMPLIFIERS

CALIBRATE STROBE

LEFT COMMANDDECODER

RIGHT COMMANDDECODER

CMDL

CLKL

CMDR

CLKR

RESET

7 7

DAC REGISTER

CALIBDAC

THRESHDAC

64 ANALOG INPUTS

S

CTRLREG

FAST-OR

MODEREG

SEL ADDRESSED

(TRI STATE)

LEFT COMMAND SELECT

DATA HIT

DATA HIT

LOAD/READ TRIGGER MASK

LOAD/READ CALIBRATE MASKLOAD/READ MODE REGISTERLOAD/READ DAC REGISTERCALIBRATE STROBE

MUX

641TRIGGER FROM PREVIOUS GTFE

FROM SILICON STRIPS

CALIB. MASK & READOUT REGISTER

EVENT_TRIG

EVENT_DATAEVENT_OR

• 64 amplifier-discriminator channels

• 7-bit threshold DAC

• Calibration mask register

• 7-bit calibration DAC

• Trigger mask register and trigger layer-OR

• Data mask register

• 4-deep event buffer

• Pair of redundant command decoders

• Pair of redundant trigger receivers

• Leftward readout register

• Rightward readout register

• LVDS I/O cells

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2A Tracker Peer Review, WBS 4.1.4 11

Readout Controller Chip (GTRC)Readout Controller Chip (GTRC)• All digital• Tanner standard-cells, except for

• LVDS I/O cells.• SEU hardened configuration

register.• RAM (64 hits, 2 buffers)

• Design in VHDL; synthesis, auto place and route.

• Verification: VHDL sim; DRC; LVS; Nanosim of extracted netlist.

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Readout CablesReadout Cables

• Standard-technology 4-layer Kapton flex circuits

• 8 unique layouts (with identical schematics)

• Require 36-inch panels for manufacture• Power traces/planes, LVDS signals, and

thermistor loops• Procurement specification: LAT-PS-01132

Thru-holes for Micro-D connector

EM cable manufactured by Parlex

Thermistor Location

Solder pads for nano-connector

4 Termination resistors

Page 13: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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Electronics CoolingElectronics Cooling

• Low IC power density (20 MHz clock): – GTFE chip: 7.8 mW for 0.33 cm2 0.024 W/ cm2

– GTRC chip: 32 mW for 0.12 cm2 0.26 W/cm2

• Total MCM power of 0.25 W is spread by the PWB over about 100 cm2 along the tray edge 2.4 mW/cm2. The 8-layer board has several full copper planes to spread the heat.

• A 5-mil 3M high-thermal-conductivity transfer adhesive lies between the MCM and carbon-carbon tray closeout.

• The carbon-carbon carries the heat to the sidewall through a 20 cm long boss and 10 fasteners into the tower sidewalls.

• The 1.5 mm thick K13D/YS90 sidewalls carry the heat to the bottom of the tower.

• Copper straps carry heat from the sidewalls into the Grid.• SSDs stay below 30°C operational. The ICs will be only a few

degrees warmer.

Page 14: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 14

Example EM TrayExample EM Tray

Connector Saver

Handle for assembly fixtures

Thermal Boss

Bias Circuit

MCM

Encapsulated ASICs

• The bias circuit is a 2-layer Kapton flex circuit.

• Top layer: 16 wire-bond pads (Ni-Au plating) + HV bias traces and bulls-eye pads for conductive adhesive.

• Bottom layer: hatched “ground” plane.

Page 15: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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2A Tracker Peer Review, WBS 4.1.4 15

Grounding & ShieldingGrounding & Shielding

FILTER FILTER

TKR/CAL_FE

ACD_FEFILTER

ACD ASSY

FILTER

TEM ASSY.

EPU

FILTER

FILTER

FILTER

POWER ASSY.

DIST-GLT ASSY. SPACECRAFT

T

28 VOLTS

MIL-1553

SSR

HSKP

GRID COMMON

SPACECRAFT

SUBSYSTEM

GROUND

COMMON

SIU

FILTER

BONDINGSTRAP

( ONE PLACE )

FILTERFILTER

OUTER SHIELDGRID CABLE

LAT RF SHIELD

BOX ENCLOSURE

LAT Overview

Page 16: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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Tracker Grounding & ShieldingTracker Grounding & Shielding

Aluminum covering on all 6 sides

Conductive tape on joints

Cu thermal straps provide the conduction path to the Grid

8 cables ground the 19 trays & electronics to the TEM

Zillion screws tie the sidewalls into the trays

Page 17: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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Tray Grounding & ShieldingTray Grounding & Shielding

• The bias circuit includes a hatched “gnd” plane (actually 1.5 V) that corresponds to the amplifier voltage reference. It separates the SSDs from the structure and couples closely to the 120 V bias on the backs of the SSDs.

• The MCMs have separate analog and digital ground planes with separate returns to the TEM, but they are coupled together on each MCM by an SMT jumper.

• 3 long screws tie each MCM ground into the aluminum core

Aluminum HexCell

C.F. Laminate Bias Plane

Silicon Strip Detectors

C.C.F. Close-Out

Mounting Screws

Multi-Chip Module (MCM)

Wire bonds & Right Angle Interconnect

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2A Tracker Peer Review, WBS 4.1.4 18

Tray Grounding & ShieldingTray Grounding & Shielding

• The 1.5 V analog supply (AVDDA) feeds the source of the input FET and is thus the small-signal reference of the detector system.

• It couples to the SSD bias via HV capacitors on the MCM and through the capacitance of the bias circuit.

• This provides the small-signal current return path of the detector system.

• All voltage supplies occupy planes on the MCM and are coupled to ground via numerous ceramic and tantalum capacitors on the MCM.

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EMI/EMCEMI/EMC

• The Tracker will be well shielded:– All transmitted signals are LVDS and digital (very low radiation and

excellent noise rejection). In addition, power and ground reference planes are always directly under or over the signal pairs.

– Aluminum foil (over carbon-fiber) covering all 6 tower module sides.

– Conductive tape around the corners to connect the sides.

• SSD strips are the sensitive nodes, but– They are well shielded from any radiation.

– Only a very local reference is needed (the amplifiers are millimeters from the strips with well identified, short current return paths).

– The local grounding around the SSDs is critical for noise performance.

• EM emissions will be tested from the qual unit, but we expect it to satisfy requirements easily (433-RQMT-0005). Preliminary measurements on the BTEM showed no measurable emission, even with the aluminum shielding walls removed.

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2A Tracker Peer Review, WBS 4.1.4 20

EMI/EMCEMI/EMC

• Primary document 433-RQMT-005• Radiated Emissions (RE101, RE102)

– 20% of total emissions are allocated to subsystems outside LAT RF shield• ACD, Tracker, Heaters

– 60% of total emissions are allocated to subsystems inside LAT shield

• Radiated Susceptibility (RS101,RS103)– All subsystems must meet Section 5.3 of 433-RQMT-005

• Conducted Emissions (CE101, CECM)– Only the T&DF subsystem is affected and must meet

requirements• Conducted Susceptibility (CS101, CS116)

– Only the T&DF subsystem is affected and must meet requirements

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2A Tracker Peer Review, WBS 4.1.4 21

BTEM EMI TestBTEM EMI Test

Spectrum Analyzer

BTEM with Shield

removed

Electric field antenna

Magnetic field antenna

No measurable EMI detected, clock on or off, even with the tower shield removed.

Page 22: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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Prototype Electronics PerformancePrototype Electronics Performance

• See LAT-TD-1090. Reviewed at TKR ASIC review Dec 6, 2002.• Analog tests with “mini-MCM” plus full-length ladder (384 channels)

– Gain and noise from charge-inject/threshold scans– Noise measurements from trigger-rate threshold scans– Noise occupancy from random triggers– Noise injection from digital readout– Gain versus number of channels pulsed– Pulse shapes and Time-Over-Threshold

• Functional tests with full MCMs (no SSDs attached)– All digital functionality– Power consumption– Voltage and timing margins– DAC calibrations– Thermal cycling

• Radiation Testing

See Presentation 3B for more recent results on Engineering-Model trays.

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Threshold DispersionThreshold Dispersion

The RMS dispersion, with or without SSDs connected, is below 8 mV, better than the requirements.

The dispersion is independent of the number of channels simultaneously pulsed.

0 10 20 30 40 50 60

Threshold DAC Setting

0

20

40

60

80

100H

it E

ffic

ien

cy

G Chip, with 32 Channels Pulsed Simultaneously

No load on inputs.

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Trigger RatesTrigger Rates

0 1 2 3

Threshold/Gain (fC)

100

101

102

103

104

105

106

Ra

te (

Hz)

G0G1G2F3F21F22

Trigger Rate per Chip (64 Channels)

1.3 fC=1/4 MIP

Long TOT pulses; look like cosmic rays

Three ladders connected to mini-MCMs were tested. These are the results for Ladder-0

Page 25: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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Noise OccupancyNoise Occupancy

0 100 200 300

Channel Number

0

2

4

6

No

ise

Hits

Ladder 0, 80V bias, 1.3 fC threshold, 1.5 million triggers.

Our first direct measurement of noise occupancy with the new electronics system.

Page 26: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

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MCM Power ConsumptionMCM Power Consumption

AVDDA

1.5 V

AVDDB

2.5 V

DVDD

2.5 V address 5

DVDD

2.5 V address 0

No Clock 77.4 mW 39.3 mW 82.8 mW

20 MHz 77.4 mW 39.3 mW 134.3 mW 138.5 mW

MCM Power (W) Allocation

MCM Address > 0 0.251

MCM Address = 0 0.255

Tower 9.05 10.5 W

16 Towers 145 168 W

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ASIC Review Action ItemsASIC Review Action Items

• Test full trays• Test noise 1 channel at a time• Noise occupancy vs threshold (deviation from gaussian noise)• Noise versus threshold• Efficiency vs threshold• Test FIB ICs with ladder• Test at high rates• Wafer probing system (see Presentation 5D)• Approved parts (see Presentation 5B)• Procurements (see Presentation 5A)

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Actions from ASIC ReviewActions from ASIC Review

• Measurements with complete trays (EM mini-tower)– Four trays, with a total of 6 SSD planes have been tested.

– Initially there were noise problems that were solved by fixing the grounding

• Grounding of the Al core via long screws in the MCM (always has been a Level-IV specification).

• Grounding of the metallic tray service/storage box.

– Now the noise and gain are consistent with what has been seen on the mini-MCMs connected to single ladders.

Long grounding screw in plated-through hole. (Conformal coat had to be scraped off.)

Aluminum handle (part of service box), also grounded to the core.

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Actions from the ASIC ReviewActions from the ASIC Review

• Example Layer-OR counting rate from 1 GTFE chip on a mini-tower tray (OR of 64 channels).

Threshold scan FE 21

0,01

0,1

1

10

100

1000

10000

100000

0 10 20 30 40 50 60

Threshold DAC

Co

un

tin

g r

ate

(H

z)

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Actions from ASIC ReviewActions from ASIC Review

• Make threshold scans on G and F version chips pulsing only one channel per chip at a time.– Pulsing only one channel, the noise sigma was about the same

for G and F versions.– This confirmed the suspicion that the higher noise sigma seen in

the F chip was related to crosstalk effects when multiple channels were pulsed.

• Measure noise occupancy versus threshold and determine at which threshold the occupancy deviates from gaussian noise. – The resulting plots give noise sigmas consistent with

expectations.– Deviations from the exponential curve at low threshold are due to

saturation from the time-over-threshold. We cannot see any evidence of spurious pickup.

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Example Noise Rate PlotExample Noise Rate Plot

OR of 64 Channels. With a gain of 75 mV/fC the fitted ENC is 1710 electrons.

GTFE3

-2

0

2

4

6

8

10

12

14

16

18

0 1 2 3 4 5

Thr**2 (fC**2)

ln(r

ate) ln(rate)

Fit

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Single-Channel Noise RatesSingle-Channel Noise Rates

• Only one channel at a time is enabled in the trigger mask, and the Layer-OR rate is measured by a frequency counter at each threshold setting.

• Two channels from the first chip are shown below.• Fitted noise ENC: 1580 electrons and 1542 electrons respectively.• No evidence of excess noise down to as low as 0.5 fC threshold.

Channel 0, Chip 0, Ladder 11

-2

0

2

4

6

8

10

12

14

0 0.5 1 1.5 2 2.5 3

Thr**2 (fC**2)

ln(r

ate)

Channel 31, Chip 0, Ladder 11

-2

0

2

4

6

8

10

12

14

0 0.5 1 1.5 2 2.5 3

Thr**2 (fC**2)

ln(r

ate)

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GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 33

Actions from ASIC ReviewActions from ASIC Review

10 14 18 22 26 30Threshold

500

1000

1500

2000

Averaged Chip Noise vs Threshold Setting

Error bars shown for Chip 0 are the RMS spreads of the 64 channels

Chip 0Chip 1Chip 2Chip 3 Chips 0, 2, and 3 are FIB’ed ICs

Page 34: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 34

Actions from ASIC ReviewActions from ASIC Review

• Study the how the efficiency varies with threshold.– This was studied by the Bari group by Monte Carlo.– See LAT-TD-1128. The simulation is for single muons.

Threshold (MIP) 0 degrees 40 degrees

0.25 99.9 99.9

0.30 98.5 96.0

0.35 98.2 94.0

0.40 97.7 92.4

0.45 96.3 90.8

0.50 92.0 89.5

Page 35: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 35

Actions from the ASIC ReviewActions from the ASIC Review

0

0.5

1

1.5

2

2.5

3

3.5

4

64 128

Strip number

Co

un

tin

g r

ate

(H

z)

Source(100 Hz) + noise (1 kHz)Source (100 Hz)

• Test the system at high rates– This was done with a ladder, mini-MCM, and SLAC EGSE.– Self trigger, using the Layer-OR, and lower the thresholds on a

subset of channels to achieve high trigger rates.– No new problems were found.– Below is a source profile at low and high trigger rates.

Page 36: GLAST LAT ProjectMarch 24, 2003 2A Tracker Peer Review, WBS 4.1.4 1 GLAST Large Area Telescope: Tracker Subsystem WBS 4.1.4 2A: Electronics Design and

GLAST LAT Project March 24, 2003

2A Tracker Peer Review, WBS 4.1.4 36

Prelim. Results on the Flight ASICsPrelim. Results on the Flight ASICs

• GTFE V-G3: 1 wafer was diced without prior probe testing:

– 14 ICs were mounted on mini-MCMs and 4 on a full-size MCM (also populated with 20 older-version GTFE chips).

– All 18 randomly selected chips worked 100%.

– No evidence of the comparator instability that plagued the previous version (all 18 chips show identical behavior, with stable Layer-OR outputs even at the minimum threshold setting).

– The timing margin on the register read-back was corrected:• All 4 chips on the full-size MCM load and read correctly at VDD=2.5V up to

28 MHz (old versions fail at 23 MHz).• All 4 chips also load and read correctly at VDD=2.25V and 20 MHz.

– One mini-MCM was connected to a full-size ladder. Noise performance is similar to the previous versions.

• GTRC V-6: 1 wafer was diced without prior probe testing

– Tested with probe card & test suite, as well as on mini-MCM and full MCM

– All functionality is correct.

– Timing margin improved: data readout works up to 30 MHz at 2.5V

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2A Tracker Peer Review, WBS 4.1.4 37

GTFE Version-G3 Noise FitsGTFE Version-G3 Noise Fits

• Example noise rate vs. threshold for a channel connected to an SSD strip.

• Distribution of fitted noise values, for a fitted average gain of 74 mV/fC.

GTFE G3

0

5

10

15

20

25

015

030

045

060

075

090

010

5012

0013

5015

0016

5018

0019

50

Noise

Fre

qu

en

cy Avg.=1634 e

Channel 12

-2

0

2

4

6

8

10

12

14

0 0.5 1 1.5 2 2.5 3

Thr**2 (fC**2)

ln(r

ate)

1638 electrons