TWEPP12_Underwood_V5 - Indico

Download Report

Transcript TWEPP12_Underwood_V5 - Indico

Modulator-Based, High Bandwidth
Optical Links
for HEP Experiments
G. Drake, W. S. Fernando , R. W. Stanek ,D. G. Underwood
High Energy Physics Division, Argonne National Lab, Argonne,
Il, United States
Log(BER)
Noise (mV)
Jitter (ps)
For a link at 10 Gb/s - -
Nice open eye
at BER=10-18
10-18 BER =1 error in ~1000 days !
10-12 BER = ~ 900 errors per day !
Electro-Optical Modulators
• Two methods for optical data transmission
– Direct modulation of light: common in short distance, short wave length
communication, all current LHC experiments use this technology
Elec. Tx
Current driver
Laser
(VCSEL)
Optical Tx
Elec. Rx
Receiver
PIN diodes
Optical Rx
– Indirect modulation of light: long distance, long wave length communication. ATLAS
TileCal will test this technology in 2013 (demonstrator) for use in Phase 2 upgrade
Laser (CW)
Elec. Tx
Voltage driver
Modulator
Receiver
PIN diodes
Elec. Rx
Optical Tx
Optical Rx
Monolithically integrated Silicon photonic device
2
Two main types of Modulators
– Mach–Zehnder interferometer based
ΔVoltage  Δrefractive index  phase amplitude
Pockels effect, Kerr effect, free carrier dispersion effect
Materials: LiNbO3, Si, InP
– Absorption based
ΔVoltage  Δoptical absorption
Output
Input
Franz-Keldysh (FK) effect in bulk semiconductors
and quantum-confined Stark effect (QCSE) in quantum-well (QW) structures.
Materials: InP, SiGe, Graphene
3
Modulating Materials for HEP
• LiNbO3 - based on the crystal property
– High bandwidth, tested rad-hard, very long (~5 cm), expensive, high
drive voltages
• InP - based on the crystal property
– Very High bandwidths, should be rad-hard, small (~2 mm), low drive
voltages, expensive at present, special-purpose technology
• Si - based on the free carrier dispersion effect
– High bandwidth, rad-hard (?), small (~1 mm), inexpensive, could
monolithically integrate, commercially available, use existing Si
Technology
4
Reliability
• Modulators are very simple and reliable. No known
failure mechanisms
– e.g. Luxtera transceiver MTBF > 2.3 x 109 hrs (300 million
device hours accumulated without a single intrinsic failure)
• E.g. 1 device failure in TileCal >34 years (9 months running, 1024
transceivers)
VCSEL
Photonic Si modulator
5
Other Considerations
• SM fiber is more rad-hard and cheaper than
most MM fiber. Ge doped MM fiber is $
• Lasers designed to run as CW can be more
reliable than switched VCSELs.
Also eliminates chirp.
• CW lasers can be at the Modulator or remote,
depending on Radiation level.
6
Modulator Selection for ATLAS TileCal
• Modulator selection based on several criteria:
– Availability: COTS devices 1st choice
– Reliability: Proven in the field
– Radiation tolerance: ~100 krad TID, ~1012 p/cm2 (and
–
–
–
–
rad-hard SM fibers are cheaper than doped MM)
Cost: Cost Savings over SNAP12 Baseline
Implementation: Ease over Baseline
Bandwidth: 56 Gb/s per readout board
BER: minimal correction needed
9.8 mm
We propose to implement optical links to be used in the TileCal
Phase 2 upgrade based on Luxtera’s silicon photonic transceiver. This
comes in a standard QSFP package which can be easily plugged into a
motherboard. We are doing a Demonstrator.
4 x 10Gb/s transceiver from Luxtera, 130nm Silicon on Insulator (SOI)
7
Commercial Integrated
Optics Chips are a
Promising Form of
Modulators.
1 cm
1 cm
laser
4 transmit and 4 receive fibers
on one integrated optics silicon
chip
10Gb/s each fiber
Use of modulators and CW
laser
Speed
10 + Gb/fiber commercial integrated optics
40 Gb/fiber with other commercial units
Laser reliability
Either CW laser onboard
Or displace laser outside detector.
(DFL has Different junction structure than VCSELs)
Low Bit Error Rate
10-18 vs typical 10-12 for current systems
Simplified error correction schemes
Low power
One CW laser - split many ways
Modulators are very efficient
Short electrical paths – no cable drivers
Low voltage drivers – not current
Rad hard optical parts
We have tested silicon integrated
optics for >64
krad application
Modulator parts should work at much higher levels
Optical part expected to work at multi-Mrad
Low power, small size
8
ANL Bench Tests of Quality and BER of the Complete Link
(Modulator & Receiver with 200m SM fiber)
FPGA board generate
PRBS7 bit stream
@10.3125 Gb/s
Use FPGA to generate
random bit stream
4 input ports, 4 output
ports.
DSA8200
Communication
Analyzer
4 SMA cables to Tx
4 SMA cables from Rx
SMA
QSFP Interface
board
Luxtera Tx
Mod
Rx
8 SM fiber bundle
100 m
Scope to monitor Quality (eye
diagram) and calculate Bit Error
Rate (BER)
Feedback
9 9
Eye diagram of Complete Link
Mask 140% of 10GBASE-R
The quality of the link is measured and compared with IEEE 802.3ae
and the performance exceeds the requirements by 40% more
10
Verified* Luxtera 10-18 BER Spec
Per link @ 10 Gb/s
10-18 BER =1 error in ~1000 days !
10-12 BER = ~ 900 errors per day
ANL
test
Log(BER)
Noise (mV)
Jitter (ps)
Luxtera / Molex
Test
Nice open eye at
BER=10-18
Why is Low BER important ?
• High BER requires Forward Error Correction (FEC) which consumes 30% of the
bandwidth and requires error correction which consumes power and introduce
susceptibility to radiation
• BER < 10-18 ~ ~ no need for FEC -> save money and bandwidth and more rad-hard!
Achieved:
• Per Link 10Gb/s (faster by x2 the upgrade target)
• BER < 10-18 (better by x106 over upgrade performance)
• Lower power consumption (factor of x6 the upgrade target)
11
Summary of Comparison
Versatile Links (target)
Technology
Bandwidth (Gb/s)
Bit Error Rate (BER)
Luxtera
40 G
Directly modulated laser
based ( eg. VCSEL)
Per
fiber
InP
Modulators
LiNbO3
Modulator
Modulator based
5
14
(10-12)
10-18
80
40
Fiber Type
Multi Mode
Reach (m)
100
4000
10000
10000
Power (mW/Gb/s)
100
8
<50*
<50*
Reliability
VCSELS have many failure
mechanisms, complex
Single Mode
No known failure mechanisms, very simple
* Estimate
12
Overall Plan for Demo of Luxtera / Molex QSFP Modulator based Devices
On-Detector
Counting House
200 M
13
A Proposed Interface to the TileCal Main Board
6
ADC hi gain
12 bit ADCs
12 tubes
PM
T
ADC low gain
shaper
Integrator
charge
injection
ADC low gain
Luxter
a
TO USA15
QSFP connector
6 differential
serial links
(4 Tx, 2 Rx)
Serializer & Control
PM
T
shaper
Integrator
charge
injection
FPGA (Kintex-7)
Note Extra I2C and monitor links
through QSFP connector to emulate
non-rad-hard PIC uC
ADC hi gain
Integrator
multiplexer
Stockholm and Valencia are
now designing the
mainboard and ROD to
accommodate the Luxtera
QSFP package.
Includes duplicate
backup links
Integrator
ADC
Luxtera QSFP has 4 x 14 Gb/s transceivers
QSFP: Quad Small Form Factor Pluggable
Inside ATLAS Tilecal Iron Girder
14
First Steps of ANL Radiation Test Program
Links run continuously at 10 Gb/s during irradiation
3 technologies
Integrated Silicon – CMOS (4-channel)
InP single channel
LiNO3 single channel
Proton Beam
Electron Beam
NO SEE @ 1012 protons/cm2 & 64 krad TID
OK after ~100 krad TID
and 3.5 x min ionizing
15
Levels of Radiation Sensitivity
in Modulator-based COTS devices
•
•
•
•
•
•
•
Modulator
Logic and RF circuitry in Modulator chip
Attached CW Laser
Voltage regulators
Glue, Capacitors, etc
Only issue so far
Control Unit ( PIC uC or..)
Working Group Wednesday 16:00
16
In this Luxtera / Molex device
uC is used for startup
reads and sets parameters for operation
also allows readout of temperature, current, etc
After startup, the device will continue to operate
until power down
(or perhaps some large change in device)
We can use external I2C, etc through spare pins on
QSFP connector to eliminate uC
17
USB
FPGA
board
8 SMA
PC
8 SMA
QSFP
QSFP
board
Shielded from radiation
~100 m
CW Lasers
USB
I2C Main
+ Power
Receivers
12 V
I2C
2 x Differential I2C
I2C
PM Fiber
QSFP
QSFP
connect
SMA
8 Fiber
Fiber SM
Fiber SM
2 Fibers SM
LiNbO3
InP
QSFP
Radiation Exposure Region
Electrical feedback
Monitoring
optical power,
Voltages,
currents
4 x 10Gb/s
BER testing
18
Summary: Modulators
• Modulators are a robust replacement for VCSEL-based optical readout:
– High Speed: >10 Gb/s. No speed limits
– Reliable: Rad hard, BER ~10-18. MTBF ~2.3 x 109 hrs
• We have proposed an optical link be used in TileCal and have built a prototype
link based on Luxtera transceiver
– Characterized it for use @ 10 Gb/s with < 10-18 BER
– Tested radiation hardness up to 8 x 1011 p/cm2
• No SEU at this level
• Need some changes to the controller ----
• Investigating other COTS modulator devices made of other materials.
• Investigating options to use modulators in very high radiation environments
such as tracker upgrades
19
Development of Free-Space (fiberless) Links
Utilizing Modulators
• Advantages:
– Low latency (no velocity factor)
– Work over distances from few mm (internal triggers)
to ~Km (counting house) or far ( to satellite orbit)
– Low mass
– No fiber routing
– Communicate between ID layers for trigger
decisions.
20
A trigger concept using modulators and prisms
Data path for on-board tracking trigger which could couple 2
planes of 3D doublets.
21
MEMS Mirrors
for steering over ~ order 1 M distance
A commercially available MEMS mirror
(Developed at ARI, Berkeley)
Argonne Center for Nan-scale Materials (CNM)
developed novel MEMS mirrors that should solve
the problems of commercial mirrors. The mirror
is supported laterally and it can be actuated using
4 torsional actuators.
April 8, 2016
22
22
A nice demonstration
1 Gb/s to a target moving ~1 cm at > 100 Hz
Reflective lens
Reflection
850 nm LASER
For alignment
This Assembly moves
X
ADC
optical  electric
TIA
Y
Si Detectors
SPI
Lookup
Small
Prism
Digital
filter
table
Rigid Coupling
GRIN lens to wires
Capture
FPGA
Bit Error Tester
1550 LASER Beam
FPGA
SPI
DAC
X
Amp
Y
SFP
wires
Asphere Lens
MEMS Mirror
to launch
to steer
Modulator
No Bit errors overnight
CW LASER
1550 nm
23
23
ANL Long Range Free-Space
Communication Telescope Demo
1 Gb/s over 80 Meters
24
24
Modulator Plans
• Radiation Test Luxtera Molex without the
microcontroller
Protons 3.5 x min ioni.
Gammas total dose up to 3 MR
Neutrons
• Radiation test components of Luxtera/Molex
Voltage Regulator
Laser
ATLAS Tilecal Demonstrator Tests
Kintex 7 FPGA
Radiation test Other Devices and other materials
For higher radiation environments
Develop other Optical Communication capabilities
25
Summary
• Modulators are simple, reliable, fast
• Silicon Integrated Technology exists for some HEP
applications
• For ATLAS Tilecal demonstrator we expect:
factor 106 lower BER,
factor ~ 3 cost savings
factor ~ 6 power savings
simplification
• We are continuing to test commercial and other
modulators
• Have demonstrated precise beam steering with
MEMS mirrors
26
Backup
27
References
[1] KK. Gan, F. Vasay, T Weidberg, “Lessons Learned and to be Learned from LHC”, Joint ATLAS-CMS Working Group on OptoElectronics for SLHC, ATL-COM-ELEC-2007-001 CMS-IN-2007/066
[2] Philippe Farthouat’s 2011 ATLAS upgrade talk
[3] T. Weidberg “VCSEL Reliability Studies and Development of Robust VCSEL Arrays” TWIPP 2011
[4] W. Fernando, “Overview and status of ATLAS pixel detector”, Nucl.Instrum.Meth., A596, 58-62 (2008)
[5] D. Giugni, S. Michal, R. Boyd, ATLAS PIXEL nSQP Project, ATL-IP-ES-0150
[6] Papotti et. al ,“An Error-Correcting Line Code for a HEP Rad-Hard Multi-GigaBit Optical Link”, 12th Workshop on
Electronics For LHC and Future Experiments, Valencia, Spain, 25 - 29, pp.258-262 (2006)
[7] Molex specifications
(http://www.molex.com/molex/products/family?key=fourteen_data_rate_fdr__active_optical_cable_aoc&channel=products&chanName=fa
mily&pageTitle=Introduction&parentKey=fiber_optic_product_families)
[8] J. Gilmore, TMB Mezzanine SEU Testing - Preliminary Results (www.physics.ohiostate.edu%2F~gilmore%2Fcms%2Fregulators%2Fcyclotron_report_v2.ppt)
[9] W. Pascher et al., “Modelling and design of a travelling-wave electro-optic modulator on InP”, Opt. Quant. Electron., vol.
35(4), 453-464 (2003)
[10] R. A. Soref and B.R. Bennett , “Electrooptical Effects In Silicon”, J. Quantum Electron., 23, 123 (1987)
[11] M. Bruzzi, "Radiation damage in silicon detectors for high-energy physics experiments," Nuclear Science, IEEE
Transactions on , vol.48, no.4, pp.960-971, Aug 2001
[12] S.T. Liu et al., "Total dose radiation hard 0.35 μm SOI CMOS technology," Nuclear Science, IEEE Transactions on , 45(6),
2442-2449 (1998)
[13] F Vasey et al, “The Versatile Link common project: feasibility report”, JINST 7 C01075 (2012) doi:10.1088/17480221/7/01/C01075
[14] HHI specifications (http://www.hhi.fraunhofer.de/en/departments/photonic-components/inp-modulators/)
[15] T. Pinguet et al. , "Monolithically integrated high-speed CMOS photonic transceivers," Group IV Photonics, 2008 5th
IEEE International Conference on , vol., no., pp.362-364, 17-19 Sept. 2008
[16] C. Gunn, et al., “A 40Gbps CMOS Photonics Transceiver”, Proceedings of SPIE 6477, 64770N (2007).
[17] BT Huffman et al.The Radiation Hardness of Certain Optical Fibres for the LHC Upgrades at -25C. JINST 2010 5 C11023.
28
References
RD23 Collaboration, “Optoelectronic Analog Signal Transfer for LHC Detectors”.
CERN/DRDC/91-41/DRDC/P31. CERN, Geneva 1991.
[PIXEL]W. Fernando, “Overview and status of ATLAS pixel detector”,. Nucl.
Instrum.Meth 2008; 58-62: A596.
[KK] K.K.Gan, W. Fernando, H. Kagan, R. Kass, A. Law et al, “Radiation-Hard
Optical Link for SLHC”. Nucl.Instrum.Meth,2008:88, 2008:88-92:A596.
L.S. Yan, Q.Yu, A.E.Willner (UCLA), "Simple Measurement of the Chirp Parameter
of Optical Modulators Using Partial Optical Filtering", Optoelectronics and
semiconductor integrated Devices, P2.28, IEEE.
[CHIRP] "Simple Measurement of the Chirp Parameter of Optical Modulators Using
Partial Optical Filtering", L.S. Yan, Q.Yu,
A.E.Willner (UCLA) Optoelectronics and semiconductor integrated Devices
P2.28 IEEE.
[LITHIUM] E.L. Wooton, et. al. (JDS Uniphase), ‘ “« A Review of Lithium Niobate
Modulators for Fiber-Optic Communications Systems”, » ) IEEE Journal of
Selected Topics in Quantum Electronics, Vol.6 No1,(, (2000) S 1077-260X(260X
(00)01136-9.
[TIPP2011] W. Fernando, D. Underwood, R. Stanek, “Optical Data Links –
Technology for Reliability and Free Space Links”, Physics Procedia, TIPP11-D11-00045, (2012) to be published.
29
[DPF] W. Fernando, D. Underwood, R. Stanek “New Optical Link Technologies for
HEP Experiments”, Meeting of the Division of Particles and Fields of the American
Physical Society, Brown University, August, 2011 arXiv:1109.6842v1.
[IEEE] D. Underwood, P. DeLurgio, G. Drake, W. Fernando, D. Lopez, G. Drake, B.
Salvachua-Ferrando, R. Stanek, “Development of Low Mass Optical Readout for High
Data Bandwidth Systems” IEEE Nuclear Science Symposium Conference Record
(NSS/MIC), 624-629, 2010.
[IBM]W. Green, M. Rooks, L. Sekaric, and Y. Vlasov “Ultra-compact, low RF power, 10
Gb/s silicon Mach-Zehnder modulator”, Opt. Express 2007; 17106-17113:15.
[JINST] D. Underwood, B. Salvachua-Ferrando, R. Stanek, D. Lopez, J. Liu, J. Michel,
L. C. Kimerling, “New Optical Technology for low mass intelligent trigger and readout”,.
JINST 5:C07011,2010.
[InP] 40Gb/s InP Modulator ………………………………………
http://www.hhi.fraunhofer.de/fileadmin/hhi/downloads/PC/flyer/40_Gbits_InP_Web.pdf.
[PIC] I.Galysh, K.Doherty, J. McGuire, H.Heidt, D.Niemi,G.Dutchover, (The StenSat
Group) "CubeSat: Developing a Standard Bus for Picosatellites"
http://www.stensat.org/Publications/SPIE.PDF.
[FPGA] Z.K.Baker, M.E.Dunham, K.Morgan, M.Pigue, M.Stettler, P.Graham,
E.N.Schmierer, J.Power (Los Alamos) “Space Based FPGA Radio receiver Design,
Debug, and Development of a Radiation Tolerant Computing System”.International
Journal of reconfigurable Computing, Volume 2010,Article ID 546217,
doi:10.1155/2010/546217.
30
The Future of Optical Links - Light Modulators
Commercial integrated optics chips are a promising form of modulators
Features Speed- 10 Gb/fiber commercial integrated optics
40 Gb/fiber with some commercial units
Laser reliabilityEither CW laser onboard (different junction structure than VCSELs)
Or displace laser outside detector.
Low Error Rate
10-18 vs typical 10-12 for current systems
Simplified error correction schemes
Low power
One CW laser - split many ways
Modulators are very efficient
Short electrical paths – no cable drivers
Low voltage drivers – not current drivers
Rad hard optical parts
We have thoroughly tested silicon integrated optics for 64 K rad application
Modulator parts should work at much higher levels
Optical part expected to work at multi-Mrad
levels
31
Studies of Direct Feedback Concept
 The commercial MEMS mirrors have ~40 dB resonance peaks at 1 and 3 KHz.
 To use the direct feedback, developed an inverse Chebyshev filter which has a notch at
1 kHz, and appropriate phase characteristics (Left Figure)
 With the filter we were able to make the beam follow a reflecting lens target within
about 10 μm when the target moved about 1 mm (Right Figure).
 Still has some fundamental issues at large excursion (~1 cm)
 A separate feedback link solves this issue
A test setup used to demonstrate MEMS
mirror steering with an analog control loop
which compensates for the mirror resonances
at 1 and 3 KHz.
The amplitude-frequency map of our analog
feedback loop, demonstrating phase stability at
100 Hz.
April 8, 2016
32
32
Beams in Air: Size vs Distance
Due to diffraction, there is an optimum diameter for a beam for a given
distance in order to reduce 1/r2 losses
 The Rayleigh distance acts much like Beta-Star in accelerators
– Relates waist size and divergence
– Depends on wavelength
 If we start with a diameter too small for the distance of interest, the
beam will diverge, and will become 1/r2 at the receiver, and we will
have large losses (We can still focus what we get to a small device
like an APD or PIN diode ). This is typical of space, Satellite, etc.
applications.
 If we start with an optimum diameter, the waist can be near the
receiver, and we can capture almost all the light and focus it to a
small spot
 Examples, ~ 1 mm for 1 m, ~ 50 mm for 1 Km
April 8, 2016
33
33
BER Tested by Luxtera
 A system has been developed to test in a
Voltaire switch (model 4036) with
continuous data flow
 Switch is fully populated (36 ports) and data
 Proven with a long term BER test on a
is injected in each port at 40Gbps.
random cable samples
 Infiniband port counters are used to
monitor the actual data flow and presence  Tests proved that there is no noise floor
of errors
 Test is run at room temperature.
34