advanced optical measurements in next generation networks october 2007 mike harrop...
TRANSCRIPT
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Agenda
Introduction Digital Transmission
Dispersion in optical Networks.
Dispersion challenges for 40G
OSA challenges for 40G/ROADM’s
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What is the fundamental of digital transmission…?
101010001001010101010101010000100101010011001010101001010
Tx Rx
The Rx circuit is clocking at the system line rate and ‘simply’ needs to discern between a 1 and a 0 to recover the original
signal.
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The need for speed…
SONET
SDH
Transmission Rate
Bit Period
OC-1 51.84 Mb 19.29 ns OC-3 STM-1 155.52 Mb 6.43 ns OC-12 STM-4 622.08 Mb 1.61 ns OC-24 1244.16 Mb (1.2 Gb) 803.76 ps OC-48 STM-16 2488.32 Mb (2.4 Gb) 401.88 ps OC-192 STM-64 9953.28 Mb (10 Gb) 100.47 ps OC-768 STM-256 39,813.12 Mb (40 Gb) 25.12 ps
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Eye diagram at Rx demonstrates signal quality
Low BERT
Intermediate BERT
Unacceptable BERT
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BERT causes a lot of pain to transmission groups
Typical values for acceptable BERT levels: >> 1 x10 -12
(or 1 bit error per 1,000,000,000,000 bits sent)
In terms of QoS measurements: single BIT error = 1 error second on the network
Conclusion of high BERT: Networks inability to operate at high speed Poor QoS figures
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What’s important in Optical Networks
Source : British Telecom Laboratories Technical Journal 2003 (authors Sikora, Zhou and Lord), Advanced network parameters which have to be properly evaluated
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What is Dispersion?
Dispersion is the time domain spreading or broadening of the transmission signal light pulses - as they travel through the fibre
OutOut
RXRX
In
TX
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Types of Dispersion
•Chromatic Dispersion:•Different wavelengths travel at different velocities
•Polarization mode dispersion:•Different polarization modes travel at different velocities
Pulse Pulse Spreading
PulsePulse Spreading
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Types of Dispersion
•Chromatic Dispersion:•Is deterministic
•Is linear
•Is not affected by environment
•Can be compensated•Polarization mode dispersion:
•Is stochastic
•Is not linear
•Is affected by the environment
•Cannot be easily compensated
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Source wavelengths = do not propagate at the same speed, thus arrive at different times
A pulse transmitted in such way suffers a spread, dispersion, limiting the transmission bandwidth.
Chromatic Dispersion Issue
1 2 3 1 23
13
PulsePulse Spreading
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Visualizing CD
Let’s visualize a light pulse travelling into a fiber and segment it into 9 quadrants (easier to visualize, and to draw!!!)
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Visualizing CD
Fiber length:
Light pulse:
Pulse width
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Effects of Dispersion
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Why is Measuring Dispersion so important?
As transmission speeds go up, the residual dispersion allowable at the receiver to give a fixed system penalty goes down.
Receiver Tolerance for a 1dB power penalty
2.5 Gb/s 16,000ps/nm
10 Gb/s 1,000ps/nm
40 Gb/s 60ps/nm
e.g. An 80km link at 1550nm will build up 17ps/(nm.km) x 80km = 1360ps/nm. Therefore at data rates at 10Gb/s and higher it is necessary to compensate for the chromatic dispersion.
To compensate effectively you need to measure the dispersion of the link.
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16 times less CD, cause 1
Time slot 125 us
Time slot 125 us
Faster means less time between pulses
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The chirp effect
Pulse before modulation
@ 2.5 Gb/s
@ 10 Gb/s
@ 40 Gb/s
P
P
P
P
modulation
16 times less CD, cause 2
Faster means broader pulses
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Dispersion Compensation
Good News : CD is stable, predictable, and controllable.
Dispersion compensating fiber (“DC fiber”) has large negative dispersion -85ps/(nm.km)
DC fiber modules correct for chromatic dispersion in the link
delay [ps]
0d
Tx Rx
DC modulesfiber span
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Dispersion Compensation for DWDM
Consider 3 channel SMF system
Dis
per
sion
(ps
/(nm
.km
))
Wavelength (nm)1300 1550 15701530
18.5
17.0
16.2
0
-85
SMF-28
DCFSlope = 0ps/nm^2/km
Dis
per
sion
-D
+D
Distance
SMF after 80km1296ps/nm @ 1530nm1360ps/nm @ 1550nm1480ps/nm @ 1570nm
Using 16km of DCF @ 85 ps/(nm.km).
Gives a residual dispersion of -64ps/nm @ 1530nm 0ps/nm @ 1550nm120ps/nm @ 1570nm
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Dispersion Compensation for DWDM
Dispersion compensation modules can only compensate exactly for
one wavelength
DWDM system design requires knowledge of end-to-end CD as a
function of wavelength… especially for long-haul
Dis
pers
ion
Transmission path
10 Gb/sTolerance
-D+D
-D
+D +D
40 Gb/sTolerance
For 40Gb/s transmission slope compensators will be required.
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CD: Bad compensation
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Dispersion Compensation for DWDM
Note. In practise system vendors don’t compensate perfectly for CD at each stage. Usually a system will be pre-compensated and then not brought back to zero during transmission. This is to avoid additional non-linear penalties such as Four Wave Mixing and Cross Phase Modulation.
Dis
pers
ion
Z
D Accumulated
-D
+D
DRes
+D +D
-D
Transmission path
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Types of Dispersion
•Chromatic Dispersion:•Different wavelengths travel at different velocities
Pulse Pulse Spreading
•Chromatic Dispersion:•Is deterministic
•Is linear
•Is not affected by environment
•Can be compensated
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Chromatic Dispersion - Conclusion
For 10Gbits/s and higher DWDM systems we need to measure both the dispersion and the slope accurately.
Many ways to measure CD in fibre but with the tolerances required for accurate compensation – the only accepted method for making this measurement with this sort of accuracy is the Phase shift method
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Patented FTB-5800 method:
Source
Oscillator DUT or FUT
Optical filteringPhasemeter
Chromatic dispersionMeasurement Method- Phase Shift FOTP-169
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Chromatic dispersionMeasurement Method- Phase Shift FOTP-169
Ref
Test 1
Few kms of fiber
RGD 1
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Chromatic dispersionMeasurement Method- Phase Shift FOTP-169
Test 2Few kms of fiber
Ref
RGD 2
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Chromatic dispersionMeasurement Method- Phase Shift FOTP-169
Test 3
RGD 3
Few kms of fiber
ADVANTAGES: - More points: more resolution- Ideal for compensation- Ideal for complex networks
Ref
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C Band Source Spectral Distribution
-50
-45
-40
-35
-30
-25
-20
1530 1535 1540 1545 1550 1555 1560 1565
nm
dB
m
Reference Filter 1562.25 nm
Grating Monochromator = 1 nm Pass Band Variable Filter
Scans All C and L Bands
A B
Reference and Measured Spectral Regions
The system compares spectral regions about 1 nm width (A,B,…) with a reference to find the relative group delay and compute CD
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Measuring CD
Delay points are acquired
Lamdba
Delay
(ps)
Lamdba
Points are fitted according to modelsDelay
(ps)
Slope of Delay gives CD
Lamdba
0
10
20
30
40
50
60
CD (ps/nm)
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The by-default or user selected mathematical model is The by-default or user selected mathematical model is fitted to the RGD point using the generalized least fitted to the RGD point using the generalized least square method.square method.
3-term Sellmeier (Standard fiber)3-term Sellmeier (Standard fiber)
5-term Sellmeier5-term Sellmeier
Lambda Log LambdaLambda Log Lambda
Cubic (Unknown fiber, flattened fiber and amplified links)Cubic (Unknown fiber, flattened fiber and amplified links)
Quadratic (Compensating, DSF and NZDSF fibers)Quadratic (Compensating, DSF and NZDSF fibers)
LinearLinear
RGD Fitting
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Wavelength (nm)1530 1535 1540 1545 1550 1555 1560
14.5
15
15.5
16
16.5
17
17.5
18
18.5
0
5000
10000
15000
20000
25000
Standard Fiber
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Extrapolated 0 = 1320.14 nm
CD at 1550nm = 16.641 ps/nm.km
Wavelength (nm)1250 1300 1350 1400 1450 1500 1550
-5
0
5
10
15
-80000
-70000
-60000
-50000
-40000
-30000
-20000
-10000
0
10000
20000
Standard Fiber
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0 = 1547.754 nm
DSF Fiber
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Example of NZDSF Analyzed with the help of the FTB-5800
NZDSF fiber (True Wave®)
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Specifications
Good repeatability Good accuracy
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EXFO FTB-5800
Industry leading accuracy on CD and Slope Ideal for 10G-40G compensation Source Shape insensitivity EDFA testing
time saving Component characterisation Fast measurement Powerful but simple software
Measuring Chromatic Dispersion
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Reminder
•Polarization mode dispersion:•Different polarization modes travel at different velocities
PulsePulse Spreading
•Polarization mode dispersion:•Is stochastic
•Is not linear
•Is affected by the environment
•Cannot be easily compensated
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Visualizing PMD
Let’s visualize a light pulse travelling into a fiber and segment it into 9 quadrants (easier to visualize, and to draw!!!)
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Visualizing PMD
Fiber section:
Light pulse:
Pulse width
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PMD Impact
If we transmit 1-0-1:
1 0 1
With PMD, this becomes:
1 0 1
The « 1 » is dimmer, the « 0 » can have light: BER
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Asymmetries in fiber during fiber manufacturing and/or stress distribution during cabling, installation and/or servicing create fiber local birefringence.
A "real" long fiber is a randomly distributed addition of these local birefringent portions.
What causes PMD
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What causes PMD?
Fiber defects
Environmental constraints
Geometric Internal Stress
Lateral Pressure
Bend
Heat
Wind (aerial fibers)
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Small Birefringence
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Small Birefringence
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Small Birefringence
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Small Birefringence
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Small Birefringence
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Small Birefringence
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Small Birefringence
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Small Birefringence
Fast Fast
Slow Slow
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Large Birefringence
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Large Birefringence
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Large Birefringence
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Large Birefringence
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Large Birefringence
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Large Birefringence
Fast Fast
Slow Slow
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
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Birefringence and mode coupling
Fast Fast
Slow Slow
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Causes of PMD
Birefringence (Bad) Introduced during manufacture non uniform intrinsic fibre stresses ie core
concentricity non uniform extrinsic stresses ie pressure
Mode coupling (Good) fibre bend and twist in-built stress in “spun” fibre splices
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PMD - Lower Bit Rate
fast axis
z, t
slow axis
t
T0 T
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PMD - Higher Bit Rate
fast axis
z, t
slow axis
t
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PMD vs Wavelength and Time
Pradeep Kumar Kondamuri and Christopher AllenInformation and Telecommunications Technology Center, The University of Kansas, Lawrence, Kansas, 66045 Douglas L. RichardsSprint Corporation, Overland Park, Kansas
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1dB Penalty probability: Very low
Average PMD
System Tolerance
Low PMD average
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1dB Penalty probability: low
Average PMD
System Tolerance
Limit PMD average
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1dB Penalty probability: very high
Average PMD
System Tolerance
Too high PMD average
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A PMD outage is when the instantaneous DGD exceeds a given threshold (Max DGD)
A factor 3 between Max DGD and Average PMD is taken from a number of ITU‑T Recommendations (including G.959-1 OPTICAL TRANSPORT NETWORK PHYSICAL LAYER
INTERFACES) for 99.9954% of no PMD problems
Once you know the system tolerance (Max DGD), aim at PMD < 1/3 of this value if you transmt Sonet/SDH
PMD Power Penalty
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PMD Pass-Fail criteria
ITU-T G.959.1, version 7.6 defines Max DGD as 3*<DGD>
It also defines Max DGD as 30ps for OC-192
ITU-T G.650 places it at 25ps Max DGD, but this is based of FIBER, with no allowance to components. Good for Fiber Manufacturer, too tight for NSP
IEEE-802.3ae has Max DGD at 19ps (10 GigE), and with a tolerance of 99.999987% (Corporation, Banks, etc need higher security) Max DGD is divided by 3.73 for this level
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PMD vs Outage probability
System vendors give Max DGD. You choose Outage probabliity, then calculate PMD to achieve
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Maximum PMD value to ensure 99.9954% probability that the tolerable broadening will correspond to a mean power penalty of
1 dB.
SONET-SDHBit rate
(Gbit/s)
2.5
10
40
Average PMD*(ps)
40
10
2.5
Digital TransmissionsPMD Specifications
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Maximum PMD value to ensure 99.999987% probability that the tolerable broadening will correspond to a mean power penalty of
1 dB
10 GigEBit rate
(Gbit/s)
10
Average PMD*(ps)
5
Digital TransmissionsPMD Specifications
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Total PMD vs PMD Coefficient
Total link PMD (ps)
10ps over 400km
5ps over 50km
Which is better?
PMD Coefficient (ps/√km) used by fibre & cable manufacturers, based on ITU recommendations that a network will be 400km.
For 10G Total limit is 10ps, using our network length of 400km gives:
10ps
√400km= 0.5ps/ √km
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Typical values for new fibre.
G.652 Standard Single Mode
<0.1ps/km
G.655 NZDSF
<0.04ps/km
e.g. For a 80km SMF link you would expect to see 0.1 x sqrt(80km) = 1ps Delay
For a 80km NZDSF link you would expect to see 0.04 x sqrt(80km) = 0.36ps Delay
Installed base?
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Installed Base
Source: John Peters, Ariel Dori, and Felix Kapron, Bellcore
10G
40G
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Reminder
•Polarization mode dispersion:•Different polarization modes travel at different velocities
PulsePulse Spreading
•Polarization mode dispersion:•Is stochastic
•Is not linear
•Is affected by the environment
•Cannot be easily compensated
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Pitfalls
•Chromatic Dispersion:•Should be specified at the cable specs (install or rental of dark fiber)•Should be tested/compensated on installation or ahead of system turn up•Should be considered very deeply for DWDM systems
•Polarization mode dispersion:•Should be specified at the cable spec level (install or rental of dark fiber)•Fibers should be tested and classified for suitability of different lines speeds•High levels could mean very costly re-engineering
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Conclusions
Uncontrolled fiber dispersion leads to increased BERT and lower QoS metrics
Dispersion should be considered mission critical to any operator considering high speed digital transmission
Accurate measurement and interpretation of those data are critical…
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TIA/EIA FOTP 124 : Polarisation Mode Dispersion for Single-mode fibres by Interferometry.
Traditional Interferometric Method (TINTY)
LimitationsGaussian Interferogram Smooth ripple free, Gaussian like sourceIdeal random coupling DUT
AutocorrelationPeak
Cross correlation
Half width
Gaussian fit
BroadbandSource
Polarizer
FUT
Interferometer
Mirror
Analyzer
Detector
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FOTP-124: Are these Gaussian???
Saudi Arabia:
South Africa:Delay (ps)
-2 -1.5 -1 -0.5 0 0.5 1 1.5 2
10
20
30
40
Delay (ps)-20 -10 0 10 20
0
5
10
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FOTP-124: Are these Gaussian???
USA:
UK:Delay (ps)
-3 -2 -1 0 1 2 3
0
5
10
15
Delay (ps)-1.5 -1 -0.5 0 0.5 1 1.5
0
5
10
15
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FOTP-124: Are these Gaussian???
Delay (ps)-2 -1.5 -1 -0.5 0 0.5 1 1.5 2
0
5
10
15
Delay (ps)-1.5 -1 -0.5 0 0.5 1 1.5
0
5
10
15
20
UK:
UK:
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?
Source Shape Auto-correlation
Infinitely broad source Infinitely thin line
Broad uniform Very thin peak
Odd-looking spectrum Broad peak, humps, ripple, etc…
Add Autocorrelation to Crosscorrelation
Autocorrelation: source shape
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TIA/EIA FOTP 124a : Polarisation Mode Dispersion for Single-mode fibres by Interferometry.
Generalised Interferometic Method (GINTY)
No LimitationsNo reliance on Gaussian InterferogramAny fibre or component can be measuredAny source shape acceptable
BroadbandSource
Polarizer
Interferometer
Mirror
Analyzer
PBS
Detectors
FUT
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FOTP-124
6.1.2 PMD Calculation for Fibers with Strong Mode Coupling
The PMD delay, <>, is determined from the half width parameter, , of the Gaussian curve fitting applied to the interferogram according to:
Where is the RMS width of the Gaussian calculated from the interferogram…
6.2 AccuracyAccuracy is related to the capability to precisly fit the
interferogram with the Gaussian function…
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What do the standards say?
Ref. IEC 61282 Fibre Optic communication system design guides – Part 9: Guidance on PMD measurements and theory
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Measuring PMD
FTB-5500B:
Highest accuracy and resolution Ideal for 10G-40G compliance & certification
Source Shape insensitivity Test the whole link EDFA, OADM testing
Fast measurement time Powerful but simple software Same source as FTB-5800 CD Analyzer
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What to do with a link with high PMD?
Frequent PMD problems (not measured when built)
Need a way to find high PMD sections:
PMDTOT =N(PMDN)2
Example: 15ps, 2ps, 1ps, 6ps
225ps2 + 4ps2 + 1ps2 + 36ps2 = 266ps2
2661/2 = 16.31ps
Find the 15ps section, replace it, problem solved…
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hL
LPMD
Birefringence & Mode Coupling
fast
slow
h
fastslow
fast
slow
fast
slow
Fibres with short (h) where Fast & Slow axis change frequently, tend to have low PMD
Fibres with long (h) where Fast & Slow axisChange infrequently, tend to have high PMD
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DOP Polarization-OTDR
Quantitative =not measured PMD value not measured
DOPSOP1, DOPSOP2, h and L = all measured Tendency for High PMD
fiber under testPulsed DFB
Laser
Detector
Polarimeter
hL
LPMD
/4
Polarizer /4
SOP1/SOP2
4x2 OTDR acquisitions for characterizing SOP(z)
0
23
22
21
S
SSSDOP
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Example of Measurement and Validation (1)
Link Length ~ 41 kmPMD = 9.8 psPMDcoefficient ~ 3 ps/km
Cable opened and PMD measured with EXFO FTB-5500B PMD test set:
29 km, PMD = 4.3 ps
5 km, PMD = 17.4 ps
7 km, PMD = 6.9 ps
29 km 5 km 7 km
High Contrast
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Example of Measurement and Validation (2)
Link Length ~ 41 kmPMD = 9.8 psPMDcoefficient ~ 1.53 ps/km
Cable opened and PMD measured with EXFO FTB-5500B PMD test set:
6 km, PMD = 9.25 ps
35 km 6 km
High Contrast
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Bi-directional Measurements
Quite similar results
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Fiber Mapping in a Cablekm 0 3 6 9 12 15 18 21 24 27 30 33 36 39 42 45 48 51 54 57 60 63 Fiber
#PMD (ps)
1 1 7.6
2 2 19.4
3 3 12.4
4 4 3.7
5 5 8.4
6 6 8.8
7 7 8.2
8 8 15.7
9 9 2.5
10 10 28.1
11 11 9.5
Open and test
Source: Connibear, A.B. and Leitch, A.W.R., Uni. Port Elizabeth, “Locating High PMD Sections of an Overhead Cable Unsing Polarization OTDR”
Fiber # PMD (ps)
PMD (ps) 40.6-49.6km
Replace and retest
fiber#
1 7.6 1.7
2 19.4 18.5 2.9
3 12.4 7.2
4 3.7 2.7
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Questions?