Optical Measurements in 100 and 400 Gb/s Networks:

Optical Measurements in 100 and 400
Gb/s Networks:
Will Coherent Receivers Take Over?
Fred Heismann
Chief Scientist
Fiberoptic Test & Measurement
Key Trends in DWDM and Impact on Test & Measurement
Complex Modulation Formats
with
Polarization Multiplexing
Coherent Receivers
with Phase- and PolarizationDiversity + DSP
Flexible Grid, Superchannels
and
Nyquist WDM
More sensitive to ASE noise
How do I measure in-band
OSNR?
Large tolerance to CD & PMD
Do I still need to measure
fiber dispersion?
Optical Constellation Analyzer
Do I ever need another optical
test instrument?
High-Resolution OSA
Where are my standards for
center frequencies?
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Coherent Receiver with High-Speed Digital Signal Processing
LO
Laser
PBS
0º /
90º
Mixer
ADC
ADC
Data
PD
Signal Decoding
ADC
Phase Recovery
PBS
ADC
0º /
90º
Mixer
CD Compensation
100 Gb/s
PM-QPSK
PMD Compensation
Digital Signal Processor
 Unprecedented tolerance to fiber dispersion
•
More than 30,000 ps/nm GVD and at least 25 ps mean DGD
• Do I still need to measure fiber CD and/or PMD?
 Additional measurement capabilities
•
CD, PMD, PDL and even OSNR
•
Do I still need to measure in-band OSNR?
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Do I Still Need to Measure CD, PMD and / or OSNR?
Do I still need to measure fiber link CD and PMD?
 NO – if I want to upgrade my system from 10 Gb/s to 100 Gb/s
• Dispersion tolerance of coherent receiver is large enough
 YES – if I am going to use “new” fiber
• PMD tolerance of coherent receivers is limited
Do I still need independent OSNR measurements?
 YES – if my coherent receiver does not measure OSNR
• Not all coherent receivers have this capability
 YES – for performance verification of newly installed systems
• Need to establish accurate baseline
 YES – for trouble-shooting of failing systems
• If receiver does not work  no OSNR measurement
How else can I measure in-band OSNR of polarizationmultiplexed signals?
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Coherent Optical Constellation / Modulation Analyzer
ADC
PD
LO
Laser
PBS
0º /
90º
Mixer
ADC
SoftwareBased
Digital
Signal
Processor
Results
PBS
ADC
0º /
90º
Mixer
Digital Storage
Optical
Signal
ADC
 Unprecedented capabilities to analyze optical signals
•
•
•
•
•
Constellation analysis: EVM, amplitude & phase distortions / offsets, …
Eye analysis: shape, noise, jitter, Q-factor, crosstalk, OSNR, …
Polarization analysis: SOP, PMD, PDL, DOP, skew , …
Bit-pattern analysis: BER, Q-factor, …
Frequency analysis: Optical spectrum
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Commercial Optical Constellation / Modulation Analyzers
High-quality coherent receiver + real-time digitizing oscilloscope
+ software-based digital signal processing = bulky instrument
Not quite field deployable
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Will Measurement Capabilities Migrate to Transponders?
Software-based DSP
• More versatile
• More capabilities
• Relatively slow
• Relatively bulky
ASIC-based DSP
• Less versatile
• Fewer capabilities
• Real time processing
• Small footprint
Coherent Transponder
?
DSP with increased
measurement capabilities
In-situ analysis of signal quality and fiber properties
Why would I ever need another optical test instrument?
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Why Would I Need Other Optical Test Instruments?
 Fiber loss is still very important
• Propagation and splice losses, reflections, …
• Especially important for systems with distributed Raman amplification
• Still need optical power and OTDR measurements
 Trouble-shooting of failing systems
• Constellation analyzer requires decoding of received signal
• If signal cannot be decoded  no measurements
• Need independent instruments for OSNR, PMD, spectrum, …
 Installation and verification of new systems
• Full fiber link characterization: loss, CD, PMD, OTDR measurements
• Initial performance evaluation: power levels, center frequencies, OSNR
 Introduction of optical superchannels and Nyquist WDM
• Spectral analysis of entire superchannel (>100 GHz BW)
• High-resolution OSA with wider wavelength range than OMA
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Other Optical Instruments Employing Coherent Detection
 Coherent optical sampling scope
• Modulation analyzer with short-pulse LO laser
• Waveform analysis with much higher bandwidth
 Coherent OTDR
• Higher sensitivity  longer distances
- Submarine cables > 10 000 km
• Higher resolution (< 10 m)
 Coherent OFDR
• Very high-resolution (component testing)
 High-resolution coherent OSA
• High spectral resolution ( 5 … 300 MHz)
• Leveraging telecommunication components
 Coherent PMD analyzer
• In-service PMD measurement (single-polarized signals only)
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Coherent High-Resolution Optical Spectrum Analyzer
WDM
Input
Signals
Coherent Receiver with
Polarization Diversity
LPF
PBS
Scanning
Local
Oscillator
Laser
Pp(ν)
3 dB
Coherent
Mixers
with Balanced
Detection
3 dB
RF
Power
Detectors
Laboratory instrument
Ps(ν)
3 dB
LPF
 5 MHz … 300 MHz spectral resolution
• Determined by electrical bandwidth of receiver
 >70 dB dynamic range
 > 1000 GHz/s tuning speed
 Sub-GHz accuracy over entire C-band
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Field instrument
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High-Resolution Spectra of Modulated Optical Signals
-10
Optical Power [dB]
-20
Measured with Coherent
OSA (300 MHz Resolution)
-30
-40
-50
-60
-70
195.17
10 Gb/s
NRZ-OOK
2.5 Gb/s
NRZ-OOK
43 Gb/s
PM-QPSK
195.22
195.27
Optical Frequency [THz]
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195.32
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Output Spectrum of Faulty 128 Gb/s PM-QPSK Transmitter
-20
Optical Power [dB]
128 Gb/s PM-QPSK
-30
-40
Gratingbased
OSA
-50
High-Resolution OSA
-60
-80
-40
0
40
Relative Frequency [GHz]
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Ultra-Densely-Spaced “Nyquist WDM” Signals for 400 Gb/s
 25 … 33% higher spectral efficiency than conventional signals
 Signals are no longer centered on 12.5 GHz ITU grid
5
Relative Optical Power [dB]
150 GHz
4 x 100 Gb/s
or
4 x 200 Gb/s
0
-5
-10
-15
200 GHz
-20
-25
-150
-100
-50
0
50
100
150
Relative Optical Frequency [GHz]
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High-Resolution Spectral Analysis of Nyquist WDM Signals
Densely Spaced Nyquist Signals
Signals shall
not overlap
Precise
adjustment
of center
frequencies
is critical
50-GHz Spaced Nyquist Signals

How accurately can I measure the center frequencies?
•

What reference frequencies shall I use?
•

Determine from 3 or 10 dB bandwidth?
Optical subcarriers may not be centered on 12.5 GHz ITU grid
Are absolute center frequencies the right metric?
•
Or should it be the relative spacing of center frequencies?
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What Comes Next?
 In-service OSNR measurements on 100 / 400 Gb/s signals
• How can we measure in-band noise of polarization-multiplexed signals?
- All physical parameters of light are used for data encoding
- Polarization extinction method doesn’t work
• Can coherent receivers help us to distinguish signal from noise?
- Without decoding of the digital information
- When signals are distorted by large CD / PMD and optical filters
 Compact coherent wavemeters?
• Hand-held devices for CWDM and DWDM systems
• When will the technology become cheap enough?
 Measurement of non-linear noise and crosstalk?
• Is it possible to distinguish nonlinear effects from ASE noise?
- SPM, XPM, XPolM, FWM
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Will Coherent Receivers Take Over?
I certainly believe so!
 Enhanced measurement capabilities in coherent transponders
• In-situ analysis of signal quality and fiber link properties
 More T&M instruments using coherent detectors
• Fault location
• Trouble shooting
• Installation and verification tests
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Thank You!