Harness QA and Assembly to Barrels - PowerPoint PPT Presentation

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Harness QA and Assembly to Barrels

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DORIC and VDC. opto package (2 VCSELs, 1 p-i-n) power tapes, redundancy system ... VDC/DORIC 50 Mrad, 2.5 1014cm-2 n ... DORIC threshold varies. 12. single ... – PowerPoint PPT presentation

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Title: Harness QA and Assembly to Barrels


1
Status report of the ATLAS SCT optical links
John Matheson (RAL) for the ATLAS opto-links team
  • links architecture
  • total dose radiation hardness
  • investigation of SEU
  • cooling issues
  • mechanical issues
  • system tests
  • pre-production harness
  • conclusions

1
2
silicon barrel module
  • silicon microstrip detector
  • readout chips
  • need timing, trigger, control in
  • need data out
  • optical links for low mass, crosstalk

2
3
links architecture
  • 40 MHz clock and control on single fibre
  • by biphase mark encoding
  • 2 data fibres/module, 40 MHz NRZ

radiation hardness (10yr) 10 Mrad, 2?1014
1 MeV neutrons cm-2
3
4
power budget
4
5
barrel harness
  • DORIC and VDC
  • opto package (2 VCSELs, 1 p-i-n)
  • power tapes, redundancy system
  • furcation tube (now black !)
  • each harness serves 6 modules

5
6
VCSEL irradiation 1
  • 20 VCSELs irradiated at INER, Taiwan
  • 30 MeV protons, 2?1014 cm-2
  • 168 hr at 10 mA, 168 hr at 20 mA

6
7
VCSEL irradiation 2
  • VCSELs degrade i.t.o. threshold, efficiency
  • injection annealing foreseen in ATLAS
  • 60 Mrad gamma - little change

7
8
VCSEL ageing
  • 20 VCSELs aged at 100C for 2534 hr
  • no failures

R (1/N?t) ln(1/(1-C))
AF (I2/I1)2 expEA/KB (1/T1 - 1/T2)
duty cycle during data transfer 50 fraction of
time sending data 50 fraction of time LHC
operates 33
8
9
Irradiation of other components
  • VDC/DORIC 50 Mrad, 2.51014cm-2 n
  • 1 week at 100C no failures? ? 0.3 max chip
    failure in SCT (redundancy makes OK)
  • wafers being qualified for production
  • p-i-n diode 11015cm-2 n, 0.5 ?0.35 A/W
  • aged 60C ? ? 5 failures in SCT
  • passives 31014cm-2 24 GeV p, no change
  • opto-flex assembly 31014cm-2 24 GeV p,
    behaviour as expected from component-level
    irradiations

9
10
single event upset
energy deposition in p-i-n diode may cause SEU
window A gt command bit error
window B gt BC clock error clock arrives up to
6.25ns early ABCD may lose synchronisation
10
11
single event upset in command signals
  • Links measured in loop-back mode
  • measure errors in command bits

loop-back link
DORIC
VDC
  • SEU irradiations at PSI
  • pions, protons 300-500 MeV/c
  • vary light power
  • DORIC threshold varies

11
11
11
11
12
single event upset in bunch crossing clock
BC clock SEU measured in 24 GeV PS beam
  • forward module in beam - optical link
  • barrel module in counting room - Cu link

L1 trigger beam spill L1 triggers
  • BC counter of ABCD is read out after each L1
    trigger
  • difference between the modules gt SEU

?SEU ? error rate (s-1) / flux
12
13
single event upset summary
  • minimum Ip-i-n 75?A
  • max SCT flux 2?106cm-2s-1
  • fraction of module data lost

9 ? 10-4 command bit (worst case) 7.8 ? 10-5 BC
clock error
13
14
cooling measurement 1
  • heat load from chips 0.4W
  • defines T at opto-package
  • component lifetime is T dependent
  • need to get the heat to the cooling block

14
15
cooling measurement 2
  • dT1 through flex
  • T drop dT1 dT2 dT3
  • minimise dT1 using vias below chips
  • AlN backing, BN-loaded epoxy

15
16
cooling measurement 3
  • total dT 18C at -7C ambient
  • expect opto-package T 0C
  • up to 10C tolerable for lifetime
  • FEA predicts total dT 25C with no heat
    transfer to environment, shows importance of vias

16
17
mechanical issues design clearance
clearance between top of opto-package/chip cover
and lower side of module is most critical point
compliance of flex must compensate variations in
  • barrel eccentricity
  • tape stack height

17
18
mechanical issues clearance measurement
clearance measured using jig (Geneva) and
envelope module
worst case uses max. barrel eccentricity, 6 tapes
to push opto-package upwards
1.4mm clearance measured using slip gauges in
agreement with the design value
18
19
CERN system test a surprise
send 2 closely spaced L1 triggers module being
read out when second trigger arrives
excess noise correlated with position
19
20
CERN system test - light leaks
excess noise is due to light leaking from optical
fibres different colour furcation tubes measured
at RAL - black is opaque
20
21
first pre-production harness
  • harnesses to be made by Radiantech Inc, Taiwan
  • before full-scale production, 8 pre-series
    harnesses will be made
  • pre-series harnesses to be used in system test
    at RAL with at least 6 modules at low T on B3
    sector
  • first harness received August 02
  • some minor issues to be resolved
  • optical links are fully functional

21
22
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23
pre-production harness bit error rate
measurements
ttc link operating point
data link operating point
both links have been operated for 12 hr with no
errors
23
24
pre-production harness towards a system test at
RAL
  • barrel module on pre-series harness
  • fully functional, 1600 e- noise
  • pre-series tests completion will define start of
    production in industry

24
25
conclusions
  • SCT harnesses must be rad-hard to 10Mrad, 1?1014
    n/cm2
  • fibre, ASICs, VCSELs, p-i-n diodes, optical
    interconnects qualified
  • harnesses are not immune to SEU but the level is
    tolerable
  • mechanical tolerances must be respected to
    preserve clearances
  • cooling must be adequate to preserve device
    longevity
  • on-sector tests at RAL will be completed before
    production begins

industrial production of 352 barrel
harnesses scheduled to begin late 2002
25
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