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ZTE Communications

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ECL 2<br />

…<br />

ECL 12<br />

ECL 1<br />

…<br />

ECL 11<br />

7 Gb/s<br />

PM-OC<br />

PM-OC<br />

DSB: frequency doubler<br />

EA: electrical amplifier<br />

ECL: external cavity laser<br />

EDFA: erbium-doped optical fiber amplifier<br />

S pecial Topic<br />

1 Tb/s Nyquist-WDM PM-RZ-QPSK Superchannel Transmission over 1000 km SMF-28 with MAP Equalization<br />

Ze Dong, Jianjun Yu, and Hung-Chang Chien<br />

Mux<br />

I/Q MOD<br />

7 Gb/s<br />

Mux<br />

I/Q MOD<br />

28 Gb/s<br />

PM<br />

EDFA<br />

28 Gb/s<br />

PM<br />

EDFA<br />

I/Q MOD: I/Q modulator<br />

IL: optical interleaver<br />

IM: intensity modulator<br />

OSC: real-time scope<br />

▲Figure 1. Testbed setup for 1Tb/s Nyquist-WDM superchannel transmission.<br />

the ISI. The aggregated terabit Nyquist-WDM superchannel<br />

is then launched into a recirculating loop comprising five 80<br />

km SMF-28 spans with an average loss of 16.7 dB and<br />

chromatic dispersion of 17 ps/km/nm at<br />

1550 nm. The loop has no optical dispersion compensation<br />

modules. For each span, an EDFA with midstage<br />

adjustable-tilt filter is used to provide flat gain. A tunable<br />

optical bandpass filter is also used to remove<br />

RZ<br />

IM<br />

IM<br />

RZ<br />

EA<br />

ATT<br />

DSB<br />

ATT<br />

EA<br />

amplified spontaneous emission (ASE) noise.<br />

The total launch power into the transmission fiber<br />

is 10.7 ± 4 dBm (-4 to approximately 4 dBm per<br />

subchannel) at 112 Gb/s. After that, a subcarrier<br />

is selected using a tunable optical filter (TOF) for<br />

coherent detection. At the receiver, an ECL with<br />

a linewidth less than 100 kHz is used as the fiber<br />

laser local oscillator (LO). A polarization-diverse<br />

90 degree hybrid is used for polarization and<br />

phase-diverse coherent detection of the LO and<br />

received optical signal before balance detection<br />

is performed. Analog to digital sampling and<br />

digitization occurs in the digital scope, which<br />

has a 40 GSa/s sample rate and 16 GHz<br />

electrical bandwidth. The captured data is<br />

processed through an offline DSP. First, the<br />

clock is extracted using a square and filter<br />

method, and the digital signal is resampled at<br />

twice the baud rate of the recovery clock.<br />

Second, a T/2-spaced time-domain finite<br />

impulse response (FIR) filter is used to<br />

compensate for chromatic dispersion. Third, two<br />

complex-valued, 13-tap, T/2-spaced adaptive<br />

PM<br />

PM<br />

25 GHz IL<br />

14 GHz<br />

RF<br />

25 GHz IL<br />

Signal<br />

LO<br />

Fiber<br />

25 GHz IL<br />

Optical Power (dBm)<br />

Optical Power (dBm)<br />

TOF<br />

90°<br />

Hybrid<br />

Offline DSP<br />

PD<br />

PD<br />

PD<br />

PD<br />

Coherent<br />

Detection<br />

Receiver<br />

O<br />

S<br />

C<br />

PM: polarization multiplexer<br />

PM-OC: polarization maintenance<br />

optical coupler<br />

TOF: tunable optical filter<br />

0<br />

-20<br />

-40<br />

-60<br />

-80<br />

1541<br />

0<br />

-20<br />

-40<br />

-60<br />

-80<br />

-100<br />

1541<br />

(a)<br />

(c)<br />

FIR filters, based on classic constant modulus<br />

algorithm (CMA), are used to retrieve the<br />

modulus of the QPSK signal.<br />

Carrier recovery is then performed. The<br />

feed-forward fourth power is used to<br />

estimate the frequency offset between the LO<br />

and received optical signal. Then, the<br />

Viterbi-Viterbi algorithm is used to estimate<br />

the carrier phase. To improve the<br />

transmission performance of a Nyquist-WDM<br />

PM-RZ-QPSK signal subject to tight optical<br />

filtering and crosstalk, we propose MAP<br />

equalization with high data-pattern<br />

dependence. First, a sequence of data<br />

symbols with BER less than 3 × 10 -4 is<br />

decided before averaging so that the<br />

symbols can be arranged into a data<br />

dependence pattern (64 kinds in the case of<br />

QPSK) to be a decision reference. Then, the<br />

data received after DSP is calculated by<br />

correlating with the decision reference to the<br />

maximum extent and mapping the QPSK data<br />

dependence decisions.<br />

3 Experiment Results<br />

The CW light waves (ECL1-12) range from 1541.5 nm to<br />

1543.7 nm with wavelength spacing of 25 GHz. An IM with<br />

appropriate DC bias and electrical amplifier power control are<br />

used to create an RZ pulse with 44% duty cycle. The Vpp of<br />

the 28 GHz RF signal is 17 V. Fig. 2(a) shows a single-carrier<br />

28 Gbaud QPSK signal before the RZ carver, and Fig. 2(b)<br />

shows a single-carrier 28 Gbaud QPSK signal after the RZ<br />

1542 1543 1544<br />

-100<br />

1541 1542 1543 1544<br />

Wavelength (nm) Wavelength (nm)<br />

0<br />

(d) 1 3 5 7 9 11<br />

1542 1543<br />

Wavelength (nm)<br />

18 dB<br />

1544<br />

▲Figure 2. Optical spectra (0.1 nm) (a) before RZ, (b) after RZ, (c) after two ILs for ECL7,<br />

and (d) after two ILs for ECL1-11.<br />

Optical Power (dBm)<br />

Optical Power (dBm)<br />

0<br />

-20<br />

-40<br />

-60<br />

-80<br />

-20<br />

-40<br />

-60<br />

-80<br />

-100<br />

(b)<br />

1541<br />

1542 1543<br />

Wavelength (nm)<br />

1544<br />

March 2012 Vol.10 No.1 <strong>ZTE</strong> COMMUNICATIONS 51

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