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K9 ____________________________________________________________________________________________________________________________ Electronics Laboratory: Optoelectronics and Optical Communication 17.05.2010 9-1 9 Optical point-t-point Communication Systems 21.05.2010 1.28 Tb/s (10 Gb/s x 64 x 2) over 70 km OTDM-Transmission (Transmitter-Fiber-Receiver) Tb/s Signal Processing by optical Nonlinear Material properties (eg. nonlinear optical fibers) Transmitter Receiver

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Page 1: K9 Optical point-t-point Communication Systemspeople.ee.ethz.ch/~fyuriy/oe/oe_optcom_chapters/...K9 _____ Electronics Laboratory: Optoelectronics and Optical Communication 17.05.2010

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9 Optical point-t-point Communication Systems 21.05.2010

1.28 Tb/s (10 Gb/s x 64 x 2) over 70 km OTDM-Transmission (Transmitter-Fiber-Receiver) Tb/s Signal Processing by optical Nonlinear Material properties (eg. nonlinear optical fibers)

Transmitter

Receiver

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Goals of the chapter:

• Analysis of signal distortion between transmitter and receiver in a simple fiber-optic point-to-point link with respect to attenuation and pulse dispersion

• Qualitative estimate of the maximum transmission distance L at a given signal data rate • Quantitative characterization of the signal detection process and definition of the minimal

detectable optical power for a particular type of signal distortion with respect to a detection error criterion

Methods for the Solution:

• Fiber attenuation α and addition losses k or fiber dispersion D define a maximum fiberlength Lmax for a given minimal received optical power Prec, min

• For digital signals and only simple on-off keying with threshold detection we calculate analytically the minimal received optical power Prec, min as a function of a tolerated Bit-Error Rate (BER) under the influence signal- and receiver noise, dispersion, timing-jitter etc.

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9 Electrical Time-Division Multiplex (ETDM): The following basic building blocks form the elements of complex fiber-optic networks:

• Optical fibers and waveguides to guide the optical waves from transmitter to receiver • Laser and LED for the generation (current modulation) of optical fields • Optical Amplifier for simultaneous amplification of several optical waves with THz-bandwidth • Modulators for modulating amplitude, phase and frequency of the optical carrier • Photodetectors for efficient conversion between optical signal into electrical signals

Connecting these components into systems rises questions like:

• Transmission concept, transmission format and network architecture • Transmission performance, bandwidth and transmission distance • Usage of available transmission medium • Modulation techniques and formats • Economic and technological boundary conditions, extendibility, transmission guaranty and efficiency of the system

This chapter addresses some basic transmission concepts and techniques less on a system level, but in the context of the elementary point-to-point-transmission with the following goals: Goals:

• Basic considerations of electrically multiplexed (time or frequency) optical point-point links with incoherent detection (intensity detection with PD)

• Quantitative limitations of transmission distance and data rates (Bit-Error Rates (BER) as a figure of merit) • Signal power budgets of fiber optic links

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Systems for transmission and distribution of information are optical carrier frequency system, where the base-band information is modulated incoherently or coherently onto an optical carrier. Optical waveguide obviously can not transmit baseband signals. RF and optical carrier frequency:

Optical communication networks are constructed similar to wired and RF-networks from elementary fiber-optic point-to-point links:

Communication networks

consist of sub-networks: 1) Point-to-point links, 2) Star-, 3) Bus- and 4) Ring-networks Signal multiplexing can be in the time domain (TDM) or in the wavelength domain (WDM)

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In analogy to RF-carrier-systems we classify optical carrier-frequency systems as:

- Analog or digital signal representation - Incoherent (Intensity-) or coherent AM-, FM- and PM-signal modulation, resp. demodulation - Digital (NRZ, RZ) coding - Single- or multiple wavelength optical systems In the following we consider only optical single frequency (wavelength)-systems, where the different signal-channels are multiplexed in the electrical time- or frequency domain.

Building-blocks of elementary

Point-to-Point-Link Detailed Point-to-Point Communication-System

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Schematic Representation of a 40 Gb/s-ETDM-Systems: (typical)

The whole MUX/DEMUX-Operation takes place in the electrical domain – the signal processing is carried out electronically and is limited by current IC-speed of about 40 Gb/s → 80 Gb/s (approaching 120 Gb/s in near future).

Point-to-point links based on the incoherent intensity modulation / detection comprise the following generic link-elements:

Current - or external modulated laser source (transmitter, regenerator)

Fiber-media (MM-, SM-fibers)

Optical amplifiers (optional)

Fiber- and waveguide components (isolators, splitters and combiners, fiber-splicing, connectors, couplers, filters, polarizers, etc.)

Photodetection (photoreceivers, regenerator)

Processing Electronics (amplifiers, clock-extraction, data-detection (thresholding), …)

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Electronic Bottle-Neck in MUX / DEMUX-functions:

It is obvious that the following electronic components in the ETDM configuration have to operate at the maximum data rate and are speed critical:

- Multiplexer (on the transmitter side) - Modulator driver / Laser driver - Preamplifier / Limiting-amplifier - Clock-Extraction Circuit - Threshold-Gate - Demultiplexer The fastest electronic ICs (only partially commercial) reach data rates of 40 Gb/s digital, resp. analog bandwidth ~30-40 GHz. These High Speed ICs are based on SiGe, InP or GaAs-transistors.

For data rates of 80-100 Gb/s there have been a only a few demonstrations-ICs realized in research labs. 80 Gb/s MUX with HEMT-Transistors: (hero-experiment: 150Gb/s divider circuit)

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Fiber optic systems evolved during the last 30 years through 5 system-generations characterized by different optical wave lengths, spectral source characteristics, fiber types and transmission formats:

Evolution of fiberoptic System-Generations: BL-product vers. year

9.1 Point-to-point links: general system considerations In the following we assume that the data format for modulation and detection is incoherent envelop (intensity)-modulation of the single- or multi-frequency optical carrier wave

→ Intensity-Modulation/Detection (ID) ; no information on optical phase used

( ) ( ) ( ) ( )Kurzzeit MiWe

ph opt opti t E t E t f ,ω φ−∗∝ ≠

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9.1.1 Point-to-point links (Prototype-structure, Intensity-modulation / detection)

Performance dominating are maximum the values, resp. the product of:

Data rate Bch and Fiber length L If the signal transmission or extraction is disturbed (noise, dispersion, attenuation, etc.) the received information will contain bit-errors (BE) at the receiver.

clock and data recovery (CDR)

characterized by BER and Prec,min

Source signal NRZ received optical signal with noise electrical receiver signal with noise Definition Bit Error Rate (BER):

The figure of merit for signal disturbance in a transmission is the so called Bit-Error-Rate (BER) defined as number of erroneous bits per unit time at a certain data rate B, or equivalently the probability that a bit is transmitted erroneously multiplied by the data rate B.

Main parameters influencing the BER:

Signal-Distortion in the source / modulator: (linear, nonlinear) - bandwidth, RIN and time-jitter of the diode laser / modulator / driver electronic Signal-attenuation: - Fiber attenuation α, fiber length L - coupling losses Laser-Fiber, Laser-Modulator-Fiber, Fiber-optical amplifier and fiber-photodetector

Prec(L) Ps,in(0)

L

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Signal-dispersion: - Fiber dispersion D, pulse broadening - (dispersion in frequency selective components) - (optical nonlinearity in fibers) - (polarization effects in fibers and components) Signal-Distortions in photoreceiver (mostly linear) - Responsivity R and frequency response of the photodetector, electronic pre- ,main- and limiting amplifier - Time-Jitter in the Clock- and Data-Extraction Circuit Signal degradation by noise: - Source noise: AM- and FM-noise from the SC-Laser (light intensity noise characterized by RIN) - Noise of optical in-line and pre-amplifiers (characterized by noise figure F) - Noise of the photodetector (shot-noise, APD-excess-noise) - Noise of the electronic amplifier chain (gain: 1000-10‘000) (opt. Pin ~nW/μW , elect. Pout: ~10mW) To guarantee a certain maximum BER in a digital transmission with a data rate Bch several limiting requirements of the following characteristics are necessary to be met:

Total analog System-Bandwidth B ~0.7-0.8xBch Maximum total attenuation of the transmission length (αeffL) and minimal source power (Popt,in) Total-Noise budget (source , receiver) Minimal received Signal Power Prec,min @BER at the receiver

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9.1.2 Power budget in a fiber-optic link (schematic)

Considering a simple point-to-point-link (without amplifier), we find the following component power losses k=Pout/Pin: - Attenuation losses of the fiber (proportional to the fiber length L, kfaser=e-αL) - Coupling losses (input) Laser-Fiber (kLF) - Insertion loss of an external modulator (kMOD) (optional) - Total Fiber-Splice losses (kSPLICE , mostly proportional to L) - Coupling losses (output) Fiber-Photodetector (kPD)

- Amplification in optical amplifiers (Gtot)

- Responsivity of the photodiode (R) Ps,in is the modulated optical power emitted by the source. We determine the power on the receiving photodiode as Pout:

( ) ( ) ( ) ( )

( ) ( )faser loss

out s ,in faser LF MOD SPLICE PD tot rec rec,min c

L Lout S ,in loss LF MOD SPLICE PD tot

h

with1P P e

P P 0 k L k k

e with ln k k k k G equivalent loss per unit length

k k G P L P B

L

ER, B

− −

= = >

= =α α α

αloss are local losses, represented formally as distributed losses over the distance L. Depending on

1) the requested BER 2) the necessary signal bandwidth Bch 3) and the noise properties of the receiver

the receiver is characterized by its sensitivity , resp. a minimal optical power Prec,min required at its input (Pout> Prec,min).

Pin Pout > Prec,min

k=Pout/Pin

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9.1.3 Attenuation Limit (loss limited BL-Product)

Transmission at low data rates Bch are usually not dispersion, but power limited. We get from the above relations the following value for a maximal fiber length Lmax, att:

( ) ( )

( ) ( )

faser max,attLs ,in LF MOD SPLICE PD rec,min ch

s ,inmax,att LF MOD SPLICE PD

faser rec,min ch

P e k k k k P B , BER

P1L ln k k k kP B , BER

α

α

− ≥

⎧ ⎫→ ≤ ⎨ ⎬

⎩ ⎭

Attenuation limited maximum fiber length Lmax,att

We will show in this chapter, that Prec,min for a required BER and for the situation, where the signal-to-noise ratio (SNR) is determined by the noise of the photoreceiver, is given by the following relation

( )rec ,minP Q BER / Rσ=

From the desired BER-value we get the following so called Q-factor (eg. BER=10-9 → Q=6)

( ) rec,min1

1 1 rec,min

2ch

2RPIQ BER2 2

RMS value of the equivalent current noise at the amplifier input

I photocurrent of the 1-Bit, with: I =2RP

k B noise power is proportional to the signal bandwidthR responsivity of th

σ σσ

σ

= =

= −

=

= →

= [ ]

( )

( )

rec,min1

ch

chrec,min ch

without proof here

e photodetector A/WExpressing the receiver noise:

RPIQ2 k B

k BP Q BER k' B minimum required power at the receiver for a given BER

R

σ= = →

= ≈

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We see Prec,min increases only with chB , as a consequence ( )max,att chL ln 1 / B∼ decreases relatively moderate with increasing data rates Bch:

( ) ( ) ( )

{ }

s ,in o totmax,att LF MOD SPLICE PD

faser rec ,min ch faser rec ,min ch

s ,in tot s ,in totmax,att ch

faser faser faserch

P P k1 1L ln k k k k lnP B , BER P B , BER

P k P k1 1 1L ln ln ln Bk' 2k ' B

α α

α α α

⎧ ⎫ ⎧ ⎫≤ =⎨ ⎬ ⎨ ⎬

⎩ ⎭ ⎩ ⎭⎧ ⎫ ⎧ ⎫⎪ ⎪≤ = −⎨ ⎬ ⎨ ⎬

⎩ ⎭⎪ ⎪⎩ ⎭

Lmax,att(Bch)

Nonamplified Transmission distance L versus Bit-Rate B for different optical fibers:

-2DK/DK -1DK/DK

Attenuation limited

Dispersion limited

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9.1.4 Dispersion-Limitations (pulse broadening)

In chap.2 we considered the pulse broadening Δt caused by the material-dispersion Dmat. In fibers there is an additional dependence of the propagation vector β(ω) of the fiber mode on the fiber geometry leading to mode-dispersion Dmode (chap.3). The total dispersion is approximated by the sum of the dispersions:

emodmatfiber DDD +=

The maximal allowable pulse broadening ΔT for a data rate Bch is:

1 1 4 1puls ch max,dispT kT / B using T L D and k / ( typ.)λΔ ≤ = → Δ = Δ = − Δλ= spectral optical width of the signal , Lmax, disp=maximal, dispersion limited fiber length

with k=1 →≤Δ 1DLB fiberdispmax,ch λ

( )max, 1 / ~ 1/disp ch fiber chL B D B≅ Δλ Lmax,disp(Bch) Maximum dispersion limited (ISI) fiber length

(in a log L-log B-representation the curve Lmax,disp(Bch) decreases with –10dB/DK) Depending on the system generation the spectral width Δλ of the source is dominated a) by the large spectral width of the source (MM-FP-lasers) (older systems Δλ >>Bchλ2/c Fourier-limited spectrum of the optical pulse) b) or by the Fourier-limited pulse spectrum Δλ ≅ Bchλ2/c , resp. Δω=Bch (new systems with SM-DBR-lasers).

System of the 1. Generation: (0.8μm MM-FP-LD, Multimode-Fiber, ch2c Bν λ

λΔ = Δ >> )

The bandwidth Δλ of the laser source (multi-mode LD, opt. carrier) is much larger than the Fourier-transfom of the digital signal (envelop) Bch. The fibers have been multimode-fibers with very high mode dispersion.

System of the 2. Generation: (1.3μm MM-FP-LD, Singlemode-Fiber, Multimode Source Spectrum ch2c Bν λ

λΔ = Δ >> )

Use of standard single-mode fibers with a dispersions-minimum at 1.3μm and 1.3μm multi-longitudinal mode FP-diode lasers.

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Δλ ~2-3nm (Δv→ 200-400 GHz) , λ=1.35μm, D~ 0-10 ps/km/nm

( )max11 ~ /1 10

ch chBBL D L dB DK

B DΔ =< → = −

Δλ

λ

System of the 3. Generation: (1.3μm SM-DBR-LD, SM-fiber and singlemode source ch2c Bδν δλ

λ= <<

The bandwidth δλ of the unmodulated laser source (DBR-laser) is much smaller than the Fourier-transform of the digital signal Bch=Δν. Use of dynamically stable DFB-diode laser and standard fibers operated in the dispersion minimum at 1.3μm.

δλ ~ 0.01 nm (→ νopt ~1-2 GHz) , λ=1.35μm (operation close to the dispersion minimum), D~ 0 - 5-10 ps/km/nm

( )2

ch 2

22

ch max,disp ch max,disp max,disp 22

ch

2ch

2

c cB

1B L D B L D 1 L 20DK / DKc B D

~

c

1B

= → Δ = = − Δ

Δ ≅ =< → = −

πβ

ν ν λλ λ

λλλ

Systeme der 4. Generation: (1.55μm SM-DBR-LD, SM-fiber and narrow band sources ch2c Bδν δλ

λ= << )

The bandwidth δλ of the lasers source (DBR-laser) is much smaller than the Fourier-transform of the digital system Bch=Δνopt. Use of optical amplifiers, external modulators and WDM-concepts (optical multi-carrier systems).

δλ ~ 0.01 nm (→ νopt ~1-2 GHz) , λ=1.55μm, D~ 5 ps/km/nm (Increasing use of dispersion-shifted fibers at 1.55μm)

Δλ=λ2/c0Bch (Signal, Fourier transform limit )

δλ (source)<<Δλ

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Dispersion at the „Dispersions-minimum λZD“:

Because of the finite spectral width Δλ≥Bchλ2/c of any optical signal and because of the frequency dependence of the dispersion D(λ) the dispersion only becomes zero for one precise wavelength λ0=λZD: Therefore the signal dispersion can be minimized, but does not vanish completely:

Average dispersion D =2ΔD for a signal spectrum Δλ:

( ) ( )

( )

ZDZD

ZD

22

ZD 2

~0

2

ch ch

D DD D ....... D S 2D

DWe define S

cwith B v , B fourier-limitedv c

λλ

λ

λ λ λ λ λλ λ

λ

λλ λ

⎧ ⎫∂ ∂⎪ ⎪= + Δ + Δ + = Δ = Δ =⎨ ⎬∂ ∂⎪ ⎪⎩ ⎭

∂=

= Δ = → Δ = −

222 3

max, max, max,

22

max, 3 3

1

1 1~

ZDch disp ch disp ch disp

ZDdisp

c ch hB

B L D B L S B L Sc

LcB S

⎛ ⎞Δ ≅ Δ = ≤⎜ ⎟

⎝ ⎠

⎛ ⎞→ = ⎜ ⎟

⎝ ⎠

λλ λ

λ

Dispersion at the Dispersion minimum λZD

System of the 5. Generation: (1.55μm SM-DBR-LD, SM-Fiber, single mode source ch2c Bδν δλ

λ= << , and optical

amplification)

Similar to the 4. Generation but including WDM and optical amplifiers.

Δλ

λZD

ΔD

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9.2 Noise properties of optical receivers

9.2.1 3-R-receiver concept

Optical signals are corrupted during generation, transmission, detection and signal processing by attenuation of the amplitude, pulse-broadening and addition of noise (source-, amplification-, detection-noise and noise from the electronic processing). To restore the signal amplitude the attenuation must be compensated by electronic gain. This „reamplification“ (R) restores the signal amplitude, but not the pulse form (eg. pulse width T) and does not eliminate noise. Before the pulse broadening becomes to excessive leading to symbol-interference, or the pulse amplitude comparable to the system noise the pulses have to be electronically regenerated in so called repeater circuits (3R-regeneration)

- reamplification (R1)

- regeneration of pulse form (R2) and

- resynchronisiert (R3) of the pulses to the bit-clock of the system Schematic electronic 3R-Regenerator circuit:

Bild 3-R-Regeneration und Funktionsblöcke, selbst

CL = Clock-signal Today the functions R2 and R3 are still realized electronically, which limits data rates to the speed of digital high speed ICs

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9.2.2 Concept of Detections (Digital RZ or NRZ-transmission)

If we could consider the whole transmission chain “driver current-source-laser-fiber-detector-amplifier-detection filter” as a linear system with the input-output-frequency response HT(ω) and the total impulse response hT(t), then the general signal response is the convolution-operation between iLD(t) and hT(t):

source noise detector noise electronic circuit noise

Signal Eye-diagram of vout(t):

For digital signal transmission of random bit-sequences the so called eye-diagram as the superposition of all possible vout(t) in a particular bit-time slot T for all possible bit-pattern of iLD(t) characterizes the transmission with respect to pattern-distortion and noise:

( ) ( ) ( )

( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )

Fourier transformout LD T

out LD T LD Laser Fiber Photo Amplifier Filter( Modulator ) Detector

out

LD

T

v t i t' h t t' dt'

V I H I H H H H H

with :v amplifier output voltagei laser currenth total impulse respon

ω ω ω ω ω ω ω ω ω

+∞

−∞

= − ⎯⎯⎯⎯⎯⎯→

= =

===

i i i i i i

se

CDR (clock and data recovery) Threshold VD Sampling time tD

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Schematic NRZ-eye-diagram: NRZ-eye-diagram 1) ideal and 2) with attenuation and dispersion:

Bit-time-slot T

Bild, selbst

Reduction of the eye-opening in amplitude and pulse width and on-set of symbol-interference from neighboring bit-slots. NRZ-eye-diagram with attenuation, dispersion, time-jitter and noise:

Jitter results in a stochastic time shift (δt) of the bits, resp. level-transitions. Noise leads to a stochastic variation of the actual signal value. Both effects reduce the „eye-opening with high error-free detection probability“.

In the ideal case one would chose the signal sampling time tD for detection of vout(t) at tD=(m+1/2)T, m=0,1,2, … (activation of the threshold switch) and the decision-level VD at (v1-Bit+v0-Bit)/2.

Ideal (α=0, D=0, component bandwidth B=∞) With attenuation (reduced amplitude) and pulse broadening (symbol-interference) but not BER

Threshold VD

tD = Sampling time

1-level, vout,1

0-level, vout,0

mT (m+1)T

Threshold VD

Threshold VD

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For ideal eye-diagrams the sampling time and the decision level are in the centre of the maximal eye-opening.

The presence of attenuation, dispersion, jitter and noise reduces the „eye-opening“ and the position of the sampling time and decision level has to be optimized (eg. dynamically, if the noise sources change) for minimum BER. In a statistical sense the eye-opening represents the „sampling area with low bit-errors“ and should be as large as possible.

9.2.3 Detector- and Receiver Noise

The above eye-diagram of vout(t) shows that at the sampling time tD the amplitudes of the 1- and 0-level fluctuate due to the noise processes around an average value:

1-Level: ( ) ( )1 1 1out , D out out Dv t v v t= + Δ

0-Level: ( ) ( )0 0 0out , D out out Dv t v v t= + Δ

For simplicity reasons we consider in the following the input signal currents I(t) at the transimpedance amplifier input (because vout(t)=RtrI(t)). All noise currents are referenced to this input:

( ) ( )( ) ( )

1 D 1 n,1 D

0 D 0 n,0 D

I t I i t 1 Bit

I t I i t 0 Bitinstantaneous value=average value+noise

= + −

= + −

Assuming that the variables in(t) of the current noise processes are ergodic = sample average = time average:

( ) ( ) ( )T B

2 2 2 2n n n n n

definition T 0 0

1lim i t dt i p i di i f dfT

σ+∞

→∞ −∞

= = =∫ ∫ ∫ σ=variance, in2(f) = noise power spectral density, B= detection bandwidth

σ2=average power in bandwidth B p(in(t)) = probability density of finding in(t) in the interval 2/dii nn ±

σ=variance, in2(f) = noise power spectral density, B= detection bandwidth

σ2=average power in bandwidth B

p(in(t)) = probability density of finding in(t) in the interval 2/dii nn ±

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We assume a Gaussian noise process, which a Gaussian amplitude-distributions for in ( )2

21 exp

22n

nip iσπ σ

⎛ ⎞= −⎜ ⎟

⎝ ⎠

Noise sources of the receiver: A) Photodetection – Noise (Shot-noise):

As discussed in chap.7 the photodetection is a statistical process of quantized events leading to shot-noise and a shot-noise current iph,n in the photocurrent ( ) ( )ph ph ph ,ni t i i t= + . For photon fluxes which are not extremely small the detection noise process can be approximated by a Gaussian random process. Spectral noise power density of the photocurrent: (no noise of the optical source RIN=0)

( )

( ) ( )

2ph,n ph

2ph

T B2 2 2

ph ph,n ph,n phT 0 0

related to the noisepower in a bandwidth B by:

i f 2ei

1lim i t dt i f df 2ei BT

σ

σ→∞

=

= =∫ ∫

relation between noise variance and spectral density

iph,n2(f)= noise power density spectrum of iph,n(t)

B=receiver bandwidth (resp. effective noise bandwidth) B) Amplifier – Noise (thermal noise and shot-noise):

Transistors in circuits produce thermal and shot-noise, similar ohmic resistors produce thermal noise.

Globally the effect of all internal noise sources in the amplifier circuit after the PD can be reproduced by two equivalent input noise sources ir(t), ur(t) and a noise-free circuit. The two correlated input noise-sources are the equivalent current- and voltage-noise sources ir(t) and ur(t), described by their variances:

( ) ( ) ( ) ( )B B

2 2 2 2 2 2i r r u r r

T T0 0

1 1lim i t dt i f df ; lim u t dt u f dfT T

σ σ→∞ →∞

= = = =∫ ∫ ∫ ∫

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( )tr

2n,R

Thermal noise of feedback R=R :

i f 4kT / R=

The values of these equivalent noise sources are a figure of merit of the noise properties of a circuit and are usually independent from the input signal. (for details see: course of Ellinger and Jäckel: Integrated Circuits for High Speed Communications) Example: simple transimpedance circuit with OP-Amps: (see exercise)

Transimpedance Transimpedance-circuit with noise-free circuit with external equivalent noise sources: Amplifier vout= - R iph: Internal noise sources:

R = feedback resistor

( ) ( )

( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )

out ph

out ,n eq,n n ,R r r eq,n R r r

eq

Signal amplification: v t R i t

Equivalent input noise current (noise current density):from : v Ri t i t R i t R u t i t i t i t u t / R

autocorrelation / Fourier transform

noise power spectrum: i

= −

= = + + → = + +

→ −

( ) ( ) ( ) ( )( ) ( )2 2 2 2 *,n r r r r n

correlation neglected

f 4kT / R i f u f / R 2 Re i u / R S fω= + + + =

Concept:

ieq,n(t) should produce the same output noise v2

out,n as ur(t), ir(t) and in,R(t). Rin 0

noise free

ieq,n(t)

in,R(t)

ir(t)

ur(t)

iph(t)=photo-current ieq,n

2(ω) ?

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9.2.4 Receiver Sensitivity and Bit-Errors Signal/Noise-Ratio (SNR) and Bit-Error Probability:

For analog signal processing the previous noise analysis provided the spectral noise power density Sn(f)=ieq,n2(f), resp.

the signal/noise-ratio SNR=iph2/ (ieq,n

2(f)B)= iph2/ σn

2 of a circuit block. Practically we are interested in the following question with regard to analog signals:

If we tolerate a signal error in a measurement, then what is the probability to exceed the tolerated error (Δ%) ? For digital signals with only 2 discrete signal-levels 0 or 1, the question is modified to:

What is the probability, that a certain bit current superposed by noise is detected erroneously by a sampled (tD) threshold ID detection, eg. a 0-level I0(tD) is detected as a 1-level, or vice-versa?

It is plausible that in the presence of noise a bit-error probability appears, resp. a bit-error-rate (BER=bit error rate). Intuitively we expect that the BER increases with decreasing SNR, because the signal is masked by more noise. We are looking for the functional relationship between BER and SNR.

It should not be overlooked that there are signal-dependent (source noise RIN, shotnoise of PD) or signal-independent (eg. amplifier noise) parts in the noise spectrum. Digital Signal Processing: (schematic):

td = sampling time , ID = threshold current

I1

Io

Photodetector: Signal amplifier: Decision circuit (sampling and level detection):

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Assumptions:

We are considering two discrete 1 and 0 signal levels 1 0I , I with noise in,1(t), in,0(t) with the correspondence I1(t) ≡ „1“ and I0(t) ≡ „0“, which are sampled at the time tD within the bit-time slot T and compared with a noise-free threshold value ID :

( ) ( ) DD1n1D1 ItiItI >+= → Detection „1“ right decision

( ) ( ) DD1n1D1 ItiItI <+= → Detection „0“ wrong decision (bit error) due to in,1(t)

( ) ( ) DD0n0D0 ItiItI >+= → Detection „1“ wrong decision (bit error) due to in,0(t)

( ) ( ) DD0n0D0 ItiItI <+= → Detection „0“ right decision

( ) ( )ti,ti 0n1n are the momentary noise signals of level 1 and 0. The noise amplitudes are assumed to show a Gaussian amplitude statistic ( )niP , characterized by:

( )( ) ( ) ( )

( ) ( )

( )( )2

n2n

n

2n eq

2 2n1 n n n

i2

nn

noise average : i t 0

noise power spectral density : S f i f 0 known

noise square average, variance : i t S f df S B

1Gaussian probability distribution : p i e2

σ

σ

σ π

+∞

−∞

=

= ≥

= = ≈

=

tD

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Graphical Representation of the Amplitude Statistics:

Probability P(1/0) of a bit-error at 1-bit: (detecting 0 instead of 1)

( ) ( ) ( )1

n1 1 1

221 11 1

1 12 21 11 1 1

using i =I -I

1 1 11/ 0 exp exp22 22 2 2

D DI I In D

nn nn n n

I Ii I IP di dI erfcσ σσ π σ π σ

−∞ −∞

⎛ ⎞⎛ ⎞ − ⎛ ⎞−⎜ ⎟= − = − =⎜ ⎟ ⎜ ⎟⎜ ⎟ ⎜ ⎟⎜ ⎟ ⎝ ⎠⎝ ⎠ ⎝ ⎠∫ ∫

erfc = complementary errorfunction Probability P(0/1) of a bit-error at 0-bit: (detecting 1 instead of 0)

( ) ( ) ( )0

220 00 0

0 02 20 00 0 0

1 1 10 /1 exp exp22 22 2 2D D

n Dn

I I In nn n n

I Ii I IP di dI erfcσ σσ π σ π σ

∞ ∞

⎛ ⎞⎛ ⎞ − ⎛ ⎞−⎜ ⎟= − = − =⎜ ⎟ ⎜ ⎟⎜ ⎟ ⎜ ⎟⎜ ⎟ ⎝ ⎠⎝ ⎠ ⎝ ⎠∫ ∫

If in a bit-sequence the 1-bit appears with a probability p(1) and the 0-bit with p(0) then their bit-error probability BEP is:

( ) ( ) ( ) ( ) ( ) ( )BEP p 0 P 0 / 1 p 1 P 1 / 0 with p 1 p 0 1= + + =

P(in) 0-level error 1-level error

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If 0- and 1-bits have equal probabilities:

( ) ( )

( ) ( ) ( )011 0 1 0

1 0

1 0 1/ 2

1 10 /1 1/ 0 , , , ,2 4 2 2

DDD n n

n n

p p

I II IBER P P erfc erfc f I I Iσ σσ σ

= =

⎡ ⎤⎛ ⎞ ⎛ ⎞−−= + = + =⎡ ⎤ ⎢ ⎥⎜ ⎟ ⎜ ⎟⎣ ⎦

⎢ ⎥⎝ ⎠ ⎝ ⎠⎣ ⎦

Because the optimal detection threshold ID is not yet determined, we choose ID in such a way, that BEP becomes minimal:

1n0n

01n10nD

0n

0D

1n

D1

D

III.respQIIII0I

BERσσσσ

σσ ++

==−

=−

→=∂

This requirements results in the optimal BER of:

( )2 1 0D

n0 n1

I I1 Q 1BER erfc exp Q / 2 with the definition of I : Q2 2 Q 2 σ σπ

−⎡ ⎤⎛ ⎞= ≅ − =⎜ ⎟⎢ ⎥ +⎝ ⎠⎣ ⎦ (with optimal threshold)

Graphical Representation of BER(Q):

6Q10BER

7Q10BER9

12

=→=

=→=−

Noise σ ↑ Q ↓ BER ↑ Amplifier- ,source, jitter

I1 ↑ Q ↑ BER ↓ Source power, attenuation, losses, dispersion

I0 ↑ Q ↓ BER ↓ On-off ratio, dispersion

Solution Procedure:

0 1 1 0n n D rec,min;given : BER Q I , I , I Pσ σ→ ⎯⎯⎯⎯→ →

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The Q-value only depends on the noise variance and signal n and Iσ , resp. of the 2 2SNR I / σ= of the two signal levels. We only get a simple relation for the ideal case, when the 0-level is ideal 0 and the noise is independent of the signal level:

1n0 n1 n 0 1 n

n

I 1, I 0 Q SNR I 2Q2 2

σ σ σ σσ

= = = → = = → =

The non-ideal cases, where eg. the noise level of the detection system is signal dependent, has to be discussed for the particular case. Practically the BER is given and the SNR, resp. the required minimal signal power Prec,min is the quantity we are looking for.

Receiver-sensitivity, minimal detectable power:

With a given BER we get Q(BER) and the minimal detectable average power min,recP gives 1,min r ec ,min 1,minP R 2 P R I= = . R is the responsivity of the photodetector and Bch is the bandwidth of the receiver (assuming a 50% ratio between 1’s and 0’s):

( )

( ) ( )2

1,min ,min

,min

2 2

n n ch

n rec

nrec n ch

S B

Q BER RP RP

Q BER Q BERP S B

R Rσ

σ

σ

=

= = →

= =

Minimal received power for n0 n1 n 0, I 0σ σ σ= = = and frequency and signal independent Sn

The minimal received power increases with noise and for lower BER

For systems limited by receiver noise: Prec,min ~ chB

For the attenuation limit Lmax ~ 1/Prec,min

For dispersion limited systems Prec,min is modified by the details of the pulse distortion mechanisms (jitter, etc.)

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9.2.5 Additional Mechanisms for BER-Degradation Additional noise processes increase the minimal detectable power Prec,min and are characterized by the ration of the min. detect. powers with and without the particular noise effect (power penalty, increased Prec,min)

( )( )

1rec ,min

rec ,min Q

with noise effectwithout noise effect

PP

> assuming that in both cases the BER, resp. the Q-factor must be the same.

9.2.5.1 Intrinsic Noise-Limit by Quantum-Noise - Detection Limit

In the most ideal case of a noise-free preamplifier there is only inherent shotnoise of the detection process itself (+ source noise): (here the detection noise is signal dependent !)

Np = number of photons per bit, 1-level: Np photons with shot noise, 0-level: Np=0 photons with no shot noise,

η = quantum efficiency of the photodetector (electrons per photon)

T= 1/B = bit time-slot

,1 1 0; / ; 0 detector efficiencypopt p

NP I eN T I

Tω η η= → = = =

( ) 21 1

21 1// 2 2

22 2

1 1 quantum-noise for intensity detection (not heterdyne)2 2 42

p

p pp

n p

p

f T B

Ne N NI I TQ SNR B N Q

TNeI f e fT

NQBER erfc erfc

ηη η η

ση

η

Δ = == = = = = = → =

Δ Δ

⎛ ⎞⎛ ⎞= = ⎜ ⎟⎜ ⎟ ⎜ ⎟⎝ ⎠ ⎝ ⎠

Example: eg. BER=10-9 → Q=6 → η Np>72 photons !

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9.2.5.2 BER-Reduction due to the finite Extinction Ratio (qualitative)

If the intensity of the 0-level is not ideally zero, that is 0I0 > , this results in a reduction of the eye-opening and an increase of the BER due to the reduced on-off-ratio 1 0 on off exI / I = P / P = 1 / r . To keep the BER identical the power of the 1-level has to be increase accordingly (without proof):

The increase of the extinction ratio rex would lead to a reduction of the factor Q, resp. to the increase in the BER.

The increased Prec,min(rex>0), resp. the increase in the of the average signal power r ecP , compared to the ideal situation Prec,min(rex=0), defines the power penalty, compensating the decrease of Q.

( ) ( ) ( ) ( )ex

exex

ex 0 1

1 ex 1 ex 0 ex rec ex1 1 0 ex

n1 n0 n1 n0 n1 n0 n1 n0 ex n1 n0r =0

=

from eg.p.9 26

r P / P extinction ratio

R P r 0 RP r 0 -RP r 0 2RP r 0I I -I 1 r= =1 r

non ideal , r >0ìdeal , r 0

σ σ σ σ σ σ σ σ σ σ−

=

= > > >−= = =

+ + + + + +

Q 1 0rec

P Pwith P2+

=

1dB penalty → ~0.1 extiction ratio

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( ) ( ) ( ) ( )

( )( )

ex

ex 0 1

1 ex 1 ex 0 ex rec ex1 1 0 ex 1 0rec

n1 n0 n1 n0 n1 n0 n1 n0 ex n1 n0r =0

rec exex

rec ex

r P / P extinction ratio

R P r 0 RP r 0 -RP r 0 2RP r 0I I -I 1 r P P= =Q with P1 r 2

P r 010 log 1

P r 0

σ σ σ σ σ σ σ σ σ σ

δ

δ

=

= > > >− += = = =

+ + + + + +

⎛ ⎞>= =⎜ ⎟=⎝ ⎠

exDefinition : Power penalty :

[ ] ( )exr ec r ec ex

ex

1 r0 log dB ; P 0 P for r 01 r

⎛ ⎞+= =⎜ ⎟−⎝ ⎠

(without

proof: see Agrawal) Using current-modulated diode lasers one is often forced to keep the 0-level I0, resp. the corresponding laser current above threshold ITH, ILD > ITH, in order to reduce turn-on-delays and relaxation oscillations. This leads to a reduction of the on-off ratio, rex. Similar external modulators with finite on-off-transmission ratios lead to a reduction of the on-off ratio.

9.2.5.3 BER-Reduction due to intensity noise of the source (qualitative)

Laser sources also exhibit intrinsic noise in the emitted power, which is described as Relative Intensity Noise (RIN)

defined as ( ) ( ) ( ) ( )2 2 Bopt opt 2 2

RIN opt2 20opt opt

i P 1RIN , resp. I RIN d2I P

ω ωω σ ω ω

π= = = ∫ .

For the detection process the RIN-noise is treated as part of the optical modulation signal. As the 1- and 0-level have different RIN-values, RIN(Pon) and RIN(Poff), this results in an increase of the total variances

n1 n0andσ σ of the 1- and 0-level. This causes an increase in the BER, resp. the minimal received power for keeping BER constant and a loss in maximal transmission distance Lmax. This degradation can be described by a power penalty:

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( )

( )

2 2 2 2 2 21,tot 1,RIN 1 1 1 1

2 2 2 2 2 20,tot 0 ,RIN 0 0 0 0

1R P RIN d with detector-shotnoise and thermal noise of the receiver for the 1-level2

1R P RIN d with detector-shotnoise and therm2

σ σ σ ω ω σ σπ

σ σ σ ω ω σ σπ

⎧ ⎫= + = + =⎨ ⎬⎩ ⎭

⎧ ⎫= + = + =⎨ ⎬⎩ ⎭

( ) ( )

( )( )

( )

0

rec rec

1,tot 0 1 0

rec

RINrec

al noise of the receiver for the 0-level

Simplifying , if P 02RP RIN 0 2RP RIN 0

Q with some simple algebra

Intensity noise power penalty :

1P RIN d2Q 10 logP RIN 0

σ σ σ σ

ω ωπδ

= →

> == ≡ →

+ +

⎛ ⎞⎛ ⎞⎜ ⎟⎜ ⎟⎝ ⎠⎜ ⎟=

=⎜⎜⎝ ⎠

∫( )2 110 log 1 Q RIN d

2ω ω

π⎛ ⎞= − −⎜ ⎟⎝ ⎠⎟

⎟∫

(without proof, see Agrawal)

Observe that for ( ) 21 RIN d 1/ Q2

ω ωπ

=∫ δRIN becomes infinite, meaning that even infinite signal power does not decrease the

BER anymore which results in a so called “noise-floor”.

9.2.5.4 BER-Reduction due to time-jitter (qualitative)

Dynamic processes in the modulated source, the driver- and detection electronic, as well as in the fiber result in time fluctuations δt of the arrival time of the pulses in their associated time slots.

Assuming that the fluctuations δt are represented by a Gaussian process with known 0,0t t >= δσδ , then, as the following figure shows qualitatively, this jitter leads to a reduction of the of the “vertical” eye-opening at a fixed detection time td.

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The effective reduction of the eye-opening and the resulting effective increase of the level-noise, increases the BER described by a power penalty δjitter.

δjitter causes an increase of the minimal received power or a loss in maximal transmission distance Lmax. Assuming a particular signal shape, then δIon(δt) can be determined, with the Bit-time T=1/B

( ) ( ) ( )( )

( )( ) ( )

( ) 2

2 2 2

recjitter 2 2 2

rec

2 2jitter jitter

2

for cos Pulse : h t cos B t / 2 cos t / 2T

follows for the jitter Power Penalty:

P b 1 b / 210 log 10 logP 0 1 b / 2 b Q / 2

t with rms-value of the timing-jitter

4b 6 B3

π π

δ

δ τ τ

π τ

− = =

− −

⎛ ⎞⎛ ⎞ −= = ⎜ ⎟⎜ ⎟ ⎜ ⎟− −⎝ ⎠ ⎝ ⎠

= = →

= − 2jitter

(without proof)

Jitter of more than 13% of the Bit-timeslot T lead to a power penalty larger than 1dB !

B τjitter

BER=10-9, Q=6

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We omitted the coherent optical modulation techniques, which realize in comparison to the considered intensity modulation format slightly better SNR, but are not frequently use to-day because of their considerable requirements (frequency stability of laser sources) on the optical components (see Kap.11 Appendix).

Optical single wavelength systems are mostly limited by the bandwidth (< 40-100 GHz) of electronics, laser modulators and photodetectors. The usage of the available fiber bandwidth of ~10 THz is very modest. Transmitting several different carrier wavelength through the same fiber (OWDM=optical wavelength multiplexing) will improve the total data rate and bandwidth usage considerably.

• Depending on data rate, spectral width of the source Δλ, dispersion D, attenuation α and fiber length L optical links are attenuation or dispersion limited

• At low data rates B the attenuation and the noise properties of the receiver dominate the maximum transmission distance Lmax

• At high data rates B fiber dispersion and receiver noise become dominant • As a practical figure of merit for the whole link or for the receiver alone the bit-error-rate BER is used, which

defines for a given bit rate B the necessary optical power at receiver Prec,min • Additional effects such as timing-jitter, finite on-off ratio etc reduce the BER and are commonly characterized

by the power penalty δ for the Prec,min.

Conclusion / Summary: