1. Introduction
DWDM optical coherent detection has been considered as the major technology for the next generation optical fiber communication system. In optical coherent systems, linear distortions, such as chromatic dispersion (CD), polarization mode dispersion (PMD) are compensated by electrical digital signal processing [
1]. The intra-channel nonlinear effects, such as self-phase modulation (SPM), may also be compensated by several post-compensation methods [
2
S. Oda, T. Tanimura, T. Hoshida, C. Ohshima, H. Nakashima, Z. Tao, and J. C. Rasmussen, “112 Gb/s DP-QPSK transmission using a novel nonlinear compensator in digital coherent receiver” in Tech. Digest of the Conference on Optical Fiber Communication , 2009, paper OThR6.
–
5
X. Li, X. Chen, G. Goldfarb, E. Mateo, I. Kim, F. Yaman, and G. Li, “Electronic post-compensation of WDM transmission impairments using coherent detection and digital signal processing,” Opt. Express
16(2), 880–888 (2008), http://www.opticsinfobase.org/oe/abstract.cfm?uri=oe-16-2-880. [CrossRef]
]. Nevertheless, DWDM system also induces the inter-channel nonlinear effects, for example, cross phase modulation (XPM). XPM cannot be compensated in a single channel receiver, because the single channel receiver does not have the information of the neighboring channels. As a result, XPM remains as one of the ultimate obstacles for coherent system. The XPM in optical transmission systems is rather complex. Previous researches [
6
T. K. Chiang, N. Kagi, M. E. Marhic, and L. G. Kazovsky, “Cross-phase modulation in fiber links with multiple optical amplifiers and dispersion compensators,” J. Lightwave Technol.
14(3), 249–260 (1996). [CrossRef]
–
13
O. Vassilieva, T. Hoshida, J. C. Rasmussen, and T. Naito, “Symbol rate dependency of XPM phase noise penalty on QPSK-based modulation formats” in Tech. Digest of the European Conference on Optical Communication
, 2008, paper We.1.E.4. [CrossRef]
] have clarified that the XPM is strongly dependent on system parameters such as data rate, fiber local dispersion, DWDM channel spacing and dispersion map. It is necessary to develop a simple method to analyze the XPM so that system designer is able to estimate XPM impact easily.
The frequency response of XPM was analyzed by the pump and continuous-wave (CW) probe model in [
6
T. K. Chiang, N. Kagi, M. E. Marhic, and L. G. Kazovsky, “Cross-phase modulation in fiber links with multiple optical amplifiers and dispersion compensators,” J. Lightwave Technol.
14(3), 249–260 (1996). [CrossRef]
]. Based on this pioneering work, a brief introduction of a simplified XPM model where the distributed XPM was reduced to a lumped phase modulation was reported in [
14
W. Yan, Z. Tao, L. Li, L. Liu, S. Oda, T. Hoshida, and J. C. Rasmussen, “A Linear Model for Nonlinear Phase Noise Induced by Cross-phase Modulation” in Tech. Digest of the Conference on Optical Fiber Communication
, 2009, paper OTuD5.
]. In this paper, in addition to that of [
14
W. Yan, Z. Tao, L. Li, L. Liu, S. Oda, T. Hoshida, and J. C. Rasmussen, “A Linear Model for Nonlinear Phase Noise Induced by Cross-phase Modulation” in Tech. Digest of the Conference on Optical Fiber Communication
, 2009, paper OTuD5.
], the fundamental model approximations and the model limitations are intensively discussed and verified. Additionally, simulation demonstrates that the normalized XPM phase noise auto-correlation, i.e. the spectrum shape equivalently, is not dependent on polarizations. Simulation also shows that the model agrees with it not only in terms of 2nd order statistical characteristics, but also the real time phase noise waveform, which implies higher order statistical agreements. With this model, impact of XPM in a phase shift keying (PSK) and on-off keying (OOK) hybrid optical coherent system and statistical characteristics of XPM phase noise are able to be estimated from system configurations. This function facilitates the system design significantly.
2. The simplified model
Fig. 1. Simplified model of XPM phase noise. (a) N-span M-channel DWDM system, (b) System with lumped XPM phase noise modulation, (c) Linear model of XPM phase noise
The principle, fundamental approximations and limitations of the model are explained in this section.
Figure 1(a) shows a schematic diagram of an
N-span,
M-channel, amplified and inline dispersion compensated DWDM system.
Figure 1(b) shows the proposed model corresponding to the system. Without losing the universality, the probe channel is assumed to be channel 1, and all the other channels are assumed as pump channels. In the model, the distributed inter-channel XPM of channel 1 is reduced to a lumped phase modulation at the end of fiber link.
Figure 1(c) illustrates how to build the modulating signal Φ
XPM applied to the phase modulator. In this paper, probe channel is assumed to be QPSK modulated because QPSK is one of the major modulation formats for coherent system. The pump channel is assumed to be OOK modulated, since such hybrid system induces the largest XPM impact. For simplicity, the polarization effect is ignored, which means that the PMD is zero and polarizations of probe and pump channels are aligned with each other. Waveform distortion on the pump channel is also ignored.
By assuming the CW probe channel 1 and the sinusoidally modulated pump channel 2, the XPM phase noise induced in one transmission span has the spectrum of:
where
γ is the fiber nonlinear coefficient,
α is the fiber loss coefficient,
L is the fiber length of each span,
d12
=
D(
λ1
-λ
2) is the inter-channel walk-off with
D as dispersion coefficient and
λ1
,
λ2
as the channel wavelengths [
6
T. K. Chiang, N. Kagi, M. E. Marhic, and L. G. Kazovsky, “Cross-phase modulation in fiber links with multiple optical amplifiers and dispersion compensators,” J. Lightwave Technol.
14(3), 249–260 (1996). [CrossRef]
]. The limitation of sinusoidally modulated pump channel may be removed by considering the fact that the XPM-induced phase shift may be represented as the sum of the phase shift induced by each pump frequency components [
6
T. K. Chiang, N. Kagi, M. E. Marhic, and L. G. Kazovsky, “Cross-phase modulation in fiber links with multiple optical amplifiers and dispersion compensators,” J. Lightwave Technol.
14(3), 249–260 (1996). [CrossRef]
,
7
K. P. Ho, Phase-Modulated Optical Communication Systems, (Springer, 2005), Chap. 8.3.
]. Based on those pioneering investigations, the details of the simplified model are shown in
Fig. 1(c). The inputs are undistorted pump channel intensity waveforms and the output Φ
XPM is the XPM phase noise on the probe channel.
H
12(
f) is described in
Eq. (1) which represents the transfer function corresponding to the phase noise induced by pump channel 2 in one fiber span. τ12 is the accumulated relative group delay between the probe and the pump in one span that is related to the dispersion map and expressed as:
where DDCF
and LDCF
are dispersion coefficient and length of dispersion compensation fiber (DCF) in each span. The phase noise associated with one of the pump channels (exp. Φxpm_2) is simply assumed to be the sum of all spans. Eventually, the total XPM induced phase noise ΦXPM is the sum of ΦXPM_i for all the pump channels.
In this model, there are two fundamental approximations. The first approximation is to model the distributed XPM as a lumped phase modulation. In reality, XPM occurs along the transmission link in a distributed manner, and XPM phase shift couples with probe channel transmission distortions, such as SPM, CD and PMD. This approximation requires the coupling between the XPM phase shift and the probe channel transmission distortion to be ignored. This leads to several model limitations as following: 1) The probe channel has to be PSK modulated, so that the phase distortion affects system performance directly. In the case of OOK probe, the XPM affects system performance through the phase-to-amplitude conversion which is a kind of XPM and probe coupling. The model leads to zero XPM penalty in OOK probe, which is not correct clearly. 2) The dominant nonlinear distortion of the probe channel has to be XPM, so that the coupling between XPM phase shift and the probe nonlinear distortion, such as SPM, would be ignored. In addition, other inter-channel nonlinear distortions, such as four wave mixing would be ignored also. Those requirements are usually satisfied in a typical QPSK and OOK hybrid system. 3) The de-coupling of the XPM phase shift and probe channel linear distortions, such as CD, PMD, is usually satisfied owning to the low-pass characteristic of XPM. As shown in
Eq. (1),
H
12(
f) may be approximately modeled as a RC low-pass filter with a cut-off frequency
f0
=
α/(
2πd
12). The cut-off frequency
f0
is typically less than GHz: for example, with a typical single mode fiber system (0.2 dB/km fiber loss, 16 ps/nm/km dispersion and 100 GHz channel spacing), the cut-off frequency is 0.6 GHz. Considering that the probe channel symbol rate is typically beyond 10 Gbaud, the coupling between the high speed probe and low speed XPM would be ignored under the linear CD and PMD distortions.
Another approximation is to ignore the pump channel intensity waveform distortion. The approximation of undistorted pumps is usually valid when the transmission length is shorter than the dispersion length or the nonlinear length. However, the dispersion length of a 10 Gbaud signal in a single mode fiber is about 100 km, which is much shorter than the typical several hundred kilometer transmission length. The typical nonlinear length is also usually shorter than the transmission length. As a result, the mechanism of this approximation in this model would be different. It is attributed to the low-pass characteristic of XPM and the white characteristic of the low frequency spectrum of OOK waveforms. It is clear that the spectrum of undistorted OOK waveform is white in the low frequency part. In other words, the low frequency components may be regarded as a random noise. Pump channel transmission distortions, such as SPM, CD and PMD, introduce the inter-symbol-interference (ISI). The ISI makes the determined bit pattern, or intensity waveform, more random. However, it does not affect the white low frequency components of the pump channel. The essential fact is that a distorted random noise would be still a random noise. Owning to the low-pass filtering of H
12(f), the XPM phase noise spectrum is determined by the shape of H
12(f) in either case with or without transmission distortion. Eventually, the pump channel intensity waveform distortion may be ignored. Nevertheless, this approximation is no longer valid when the pump channel is in PSK, such as RZ-QPSK. Without transmission distortion, the intensity waveform of RZ-QPSK is periodic, and the low frequency spectrum components should be near zero. With distortion, the ISI makes the spectrum whiter and the low frequency spectrum components turns higher. The essential requirement of this approximation is that the low frequency spectrum of undistorted pump channel intensity waveform is white. More complicated model would be required with PSK pump channel, which is out of the scope of this paper.
In short, the lumped phase modulation and undistorted pumps approximations lead to the model limitations as following: 1) The probe channel has to be PSK modulated. 2) The XPM has to be the dominant source of distortions to the probe channel. 3) The pump channel have OOK or other non-constant-envelop modulation format, such as quadrature amplitude modulation and amplitude-phase shift keying modulation. 4) The dispersion map seems not to be a major limitation. A typical terrestrial QPSK and OOK hybrid system usually satisfies above requests.
The proposed model would be verified in following section 3 and 4. Generally, the XPM phase noise Φ
XPM is determined by the bit patterns of the pump channels. It looks like a random noise, whose probability density function is assumed to Gaussian distribution [
15
K. P. Ho, “Error Probability of DPSK Signals With Cross-Phase Modulation Induced Nonlinear Phase Noise,” IEEE J. Sel. Top. Quantum Electron.
10(2), 421–427 (2004).
]. For simplicity, the discussion in following mainly focuses on the standard deviation and auto-correlation of XPM phase noise.
3. Simulation
Fig. 2. System setup of hybrid transmission NZ-DSF: non-zero dispersion shifted fiber, DCF: dispersion compensation fiber, PC: polarization controller, MUX: optical multiplexer
In order to verify the proposed model, a 9-channel, 50 GHz spacing DWDM transmission system as shown in
Fig. 2 was investigated by numerical simulation. The channel number was limited to 9 for the reason of nonlinear simulation speed, whereas 80-channel experiment will be demonstrated in section 4. The CW probe channel lay in the middle, and the pump channels were 11 Gb/s NRZ modulated. The 900 km fiber link consisted of 12 spans. Each span had 75 km non-zero dispersion shifted fiber with a local CD coefficient of 4ps/nm/km. Eighty percent of the span CD was post-compensated by a DCF for each span. The span launch power was -4 dBm/ch. For simplicity, ASE noise was ignored in simulation. The polarization of each channel was aligned by polarization controllers and the polarization mode dispersion (PMD) of fiber link was assumed to be zero, so that the scalar nonlinear Schrödinger equation could be used. The coherent receiver, including the carrier phase recovery, was assumed to be ideal. The residual dispersion of the whole transmission link was also compensated completely at the receiver.
With such ideal coherent receiver, the output of digital storage oscilloscope was the XPM phase noise directly, and the auto-correlation could be calculated accordingly. The results of the simplified model were calculated according to
Fig. 1(c). The undistorted pump channel intensity waveforms were obtained by simulation.
H
12(f),
τ12
and other parameters could be calculated from system configurations according to
Eqs. (1) and
(2).
Figure 3(a) shows the auto-correlation of the XPM phase noise. It is clear that the proposed model agrees with the numerical simulation in terms of 2nd order statistical characteristics.
Figure 3(b) shows the waveform comparison. It demonstrates that the agreement of the model and the simulation is not only in 2nd order statistical characteristics, but also in the real time waveform, which would lead to higher order statistical agreements.
Fig. 3. (a) auto-correlation and (b) waveform of the XPM phase noise. simulation: results obtained by solving the nonlinear Schrödinger Equation, model: results by the proposed model.
The discussion in section 2 shows the limitations of the model. The PSK probe and XPM dominant distortion limitations seem to be straightforward. In order to verify the other two limitations, systems of zero in-line dispersion compensation with 11 Gbit/s OOK and 11 Gbaud RZ-QPSK pumps were simulated, whereas the other system parameters kept same.
Figure 4(a) shows the XPM phase noise auto-correlation of OOK pump system. The result of the model agrees with simulation well, which demonstrates the model functions under various dispersion maps.
Figure 4(b) shows the auto-correlation when the 11 Gb/s OOK pump channel is replaced by the 11 Gbaud RZ-QPSK pump. There is significant difference between the simulation result and the model result. It provides a clear evidence of the limitation, which is only valid with OOK pump channels.
Fig. 4. XPM phase noise auto-correlation of zero in-line dispersion compensation system with (a) 11 Gb/s NRZ pump and (b) 11 Gbaud RZ-QPSK pump, simulation: results obtained by solving the nonlinear Schrödinger Equation, model: results by the proposed model
Next, in order to investigate the impact of polarization, the scalar Schrödinger equation was replaced by the vector equation in following. All the pump channels had aligned 0 degree linear polarization, whereas the polarization of probe channel was linear with various azimuths
θ of 0, 15, 30, 60, and 90 degree. All the other parameters were kept the same as the previous simulation, including the zero PMD.
Figure 5(a) shows the standard deviation of XPM phase noise as a function of polarization factor that is defined as cos
2(
θ)+sin
2(
θ)/3. It is proved that the amplitude of XPM phase noise depends on polarization, and is proportional to the polarization factor, which is consistent with the results in [
6
T. K. Chiang, N. Kagi, M. E. Marhic, and L. G. Kazovsky, “Cross-phase modulation in fiber links with multiple optical amplifiers and dispersion compensators,” J. Lightwave Technol.
14(3), 249–260 (1996). [CrossRef]
].
Fig. 5. Impact of polarization: (a) reduction of XPM phase noise, (b) independence of normalized auto-correlation
The result of
Fig. 5(a) is consistent with the common understanding that XPM depends on polarizations. However, the answer of which kind of XPM characteristic does not depend on polarizations has been still unclear.
Figure 5(b) shows that the normalized auto-correlation of XPM phase noise, or phase noise spectrum shape equivalently, is not dependent on polarizations. The diamonds and circles corresponds to the cases
θ=0 and 60 degree, when PMD was 0. There is no difference between them. In order to reproduce more complicated and realistic scenarios, the ideal zero PMD was replaced by a realistic value of 0.1 ps/sqrt(km) and two cases were investigated: the case with aligned polarization at the transmitter (shown by triangles in
Fig. 5(b)) and the case with randomized polarization at the transmitter (shown in squares). There is no difference between those four polarization settings, and all of them agree with the proposed model well.
In short, simulation results demonstrate the capabilities and limitations of the proposed model. Simulation results also show that polarization does not affect the shape of auto-correlation, or the spectrum, of XPM phase noise. It only affects the amplitude, or power. As a result, the proposed model may be applied to non-ideal polarization scenarios, even though the model ignores the polarization effects.
4. Experiment
In order to verify the proposed model, 80 channels, PSK-OOK hybrid DWDM transmission experiment was done. The experimental setup was the same as simulation setup in
Fig. 2 except that the probe channel was 43 Gb/s QPSK modulated and the number of DWDM channels was 80. The processing algorithm in the coherent detection digital receiver was based on the Viterbi-Viterbi carrier phase recovery [
8
T. Tanimura, S. Oda, M. Yuki, H. Zhang, L. Li, Z. Tao, H. Nakashima, T. Hoshida, K. Nakamura, and J. C. Rasmussen, “Non-linearity tolerance of direct detection and coherent receivers for 43 Gb/s RZ-DQPSK signals with co-propagating 11.1 Gb/s NRZ signals over NZ-DSF” in Tech. Digest of the Conference on Optical Fiber Communication , 2008, paper OTuM4.
].
Figure 6 shows the Q values measured as a function of phase recovery average length after 450km (
Fig. 6(a)) and 900km (
Fig. 6(b)) transmission at the launch power of -4dBm/ch. The OSNR was 12.3dB for the both cases. The simplified model results were obtained by single channel experiment with lumped phase noise modulation calculated by the proposed model. In order to reduce the experimental difficulties, the phase modulation was emulated in electrical digital domain after coherent detection and analog to digital convertors with a speed of 2 samplers per symbol. Since the coherent detection linearly converted an optical domain signal into the electrical domain, the emulated phase modulation was equivalent to a real phase modulation as shown in
Fig. 1(b). The results of proposed model were confirmed to agree with real experiment in its tendency and the maximum deviation between the two as 0.5 dB.
Fig. 6. System performance of simplified model and real experiment (a) 450km (b) 900km
In addition to the Q value, the XPM phase noise auto-correlations obtained by the experiment and the proposed model were compared. By using the method in [
14
W. Yan, Z. Tao, L. Li, L. Liu, S. Oda, T. Hoshida, and J. C. Rasmussen, “A Linear Model for Nonlinear Phase Noise Induced by Cross-phase Modulation” in Tech. Digest of the Conference on Optical Fiber Communication
, 2009, paper OTuD5.
], the normalized auto-correlation of XPM phase noise was measured in the experiment. The results of simplified model were calculated according to
Fig. 1(c),
Eq. (1) and
Eq. (2).
Figure 7 shows the normalized auto-correlation after 450km (
Fig. 7(a)) and 900km (
Fig. 7(b)) transmission at a launch power of -4dBm/ch. The experiment and proposed model results agreed well.
Fig. 7. Normalized auto-correlations of XPM phase noise after transmission over (a) 450km and (b) 900km.
In short, the Q value under XPM distortion and auto-correlation of XPM phase noise were measured in the experiment. The results of experiment and proposed model agree well with each other in both cases of 450 km and 900 km transmission, which demonstrates that the proposed model functions under various system conditions.
5. Statistical characteristics of XPM phase noise
The proposed model is verified by simulation and experiment in sections 3 and 4. By employing this model, the characteristics of XPM phase noise may easily be estimated, although XPM phenomenon is rather complex and strongly dependent on system parameters. In the proposed model, the XPM looks like a low-pass filter
H
12(
f). According to
Eq. (1), the cut-off frequency is inversely proportional to the walk-off
d
12, whereas the fiber loss
α is usually a constant value. As a result, the walk-off
d
12 is the most important parameter in XPM analysis. Obviously, a large walk-off is helpful to reduce the XPM phase noise and increase the auto-correlation length. Another key parameter is the accumulated group delay
τ
12 in one span, which is related to the dispersion map. Obviously, a large
τ
12 is helpful to de-correlate the XPM phase noises induced in different spans. Such de-correlation may reduce the total XPM phase noise, since the XPM phase noises of different spans are added incoherently or partially coherently. The proposed model could explain various XPM phenomena reported in previous publications, just as shown in following.
Fig. 8. Dependences of XPM phase noise on (a) fiber launch power, (b) dispersion compensation (DC) ratio, (c) DWDM channel spacing, (d) guard spacing, (e) total channel number, (f) pump OOK channel bit rate. HWHM: the half-width half-magnitude of auto-correlation. std. the standard deviation of phase noise
Figure 8 presents the standard deviation and auto-correlation length as a function of various system parameters, when a system configuration similar to
Fig. 2 is assumed.
Figure 8(a) shows the impact of fiber launch power. The phase noise increases in proportion to the launch power in linear unit (mW), and the auto-correlation length does not depend on it. The fact that the transfer function in
Fig. 1(c) is independent on the launch power explains this nature.
Figure 8(b) shows the impact of inline dispersion compensation ratio. It has been reported that low dispersion compensation ratio improves transmission performance with regards to XPM [
9
X. Liu and S. Chandrasekhar, “Suppression of XPM penalty on 40-Gb/s DQPSK resulting from 10-Gb/s OOK channels by dispersion management” in Tech. Digest of the Conference on Optical Fiber Communication , 2008, paper OMQ6.
,
10
S. Chandrasekhar and X. Liu, “Impact of channel plan and dispersion map on hybrid DWDM transmission of 42.7-Gb/s DQPSK and 10.7-Gb/s OOK on 50-GHz grid,” IEEE Photon. Technol. Lett.
19(22), 1801–1803 (2007). [CrossRef]
]. The proposed model supports such a conclusion that may be explained by the impact of accumulated group delay
τ
12. With the reduction of dispersion compensation ratio, the accumulated group delay becomes larger, so that XPM phase noise is reduced.
Figures 8(c) and
8(d) show the impacts of channel spacing and guard spacing, which is defined as the frequency spacing between the interested channel and the nearest pump channel. XPM phase noise is reduced with large channel spacing and guard spacing. This is consistent with the results reported previously [
9
X. Liu and S. Chandrasekhar, “Suppression of XPM penalty on 40-Gb/s DQPSK resulting from 10-Gb/s OOK channels by dispersion management” in Tech. Digest of the Conference on Optical Fiber Communication , 2008, paper OMQ6.
,
11
A. S. Lenihan, G. E. Tudury, W. Astar, and G. M. Carter, “XPM-induced impairments in RZ-DPSK transmission in a multi-modulation format WDM system” in Tech. Digest of Conference on the Lasers and Electro-Optics , (CLEO) 2005. paper CWO5.
]. By enlarging channel spacing or guard spacing, the walk-off parameter is increased. As a result, smaller phase noise and longer auto-correlation are achieved.
Figure 8(e) shows that the standard deviation and auto-correlation length saturate with increasing number of channels, just as reported in [
12
X. Huang, L. Zhang, M. Zhang, and P. Ye, “Impact of nonlinear phase noise on direct-detection DQPSK WDM systems,” IEEE Photon. Technol. Lett.
17(7), 1423–1425(2005). [CrossRef]
]. In DWDM system, the channels far-away from the wavelength of interest tend to have larger walk-off, which leads to much smaller XPM phase noise contribution. Consequently, the near channels dominate the XPM phase noise, and far-away channels may be ignored.
Figure 8(f) shows the impact of pump channel bit rate. It shows that the phase noise decreases with pump channel bit rate. Similar conclusion was also reported in [
13
O. Vassilieva, T. Hoshida, J. C. Rasmussen, and T. Naito, “Symbol rate dependency of XPM phase noise penalty on QPSK-based modulation formats” in Tech. Digest of the European Conference on Optical Communication
, 2008, paper We.1.E.4. [CrossRef]
]. It may also be explained by the proposed model. Given the launch power, the pump channel spectrum density reduces with the bit rate. Owning to low-pass filtering characteristic of XPM, only the low frequency component contributes to the phase noise. As a result, the standard deviation reduces with the pump channel bit rate.
In short, the proposed single model explains various XPM phenomena in
Fig. 8, although each of them has been investigated and reported [
9
X. Liu and S. Chandrasekhar, “Suppression of XPM penalty on 40-Gb/s DQPSK resulting from 10-Gb/s OOK channels by dispersion management” in Tech. Digest of the Conference on Optical Fiber Communication , 2008, paper OMQ6.
–
13
O. Vassilieva, T. Hoshida, J. C. Rasmussen, and T. Naito, “Symbol rate dependency of XPM phase noise penalty on QPSK-based modulation formats” in Tech. Digest of the European Conference on Optical Communication
, 2008, paper We.1.E.4. [CrossRef]
] separately. With the proposed model, the complex XPM may be estimated from system configurations easily.