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Analysis of Laser Phase Noise Effect in Direct-Detection Optical OFDM Transmission

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Analysis of Laser Phase Noise Effect in

Direct-Detection Optical OFDM Transmission

Wei-Ren Peng

Abstract—In this paper, we characterize the impact of laser phase noise (PN) in direct-detection optical OFDM (DDO-OFDM) and identify its many differences from those in coherent optical OFDM (CO-OFDM). The analytical models for the diverse PN effects, including power degradation, phase rotation term (PRT), and inter-carrier interference (ICI), are given in terms of critical system parameters with or without the small PN assumption. In particular, the analytical upper-bound of the ICI power with a simple form is also provided. We also present a bit error rate (BER) estimation approach which is proven to be reliable for an optical signal-to-noise-ratio (OSNR) penalty lower than 2 dB. In addition, the PN tolerances, in terms of OSNR penalty, are also numerically analyzed and discussed with different QAM formats, data rates, laser linewdiths, and subcarrier numbers.

Index Terms—Direct detection, optical fiber communication, or-thogonal frequency division multiplexing (OFDM), optical modu-lation, phase noise.

I. INTRODUCTION

O

PTICAL orthogonal-frequency-division-multiplexing (OFDM) has recently received lots of attention due to its high spectral efficiency and superior resilience against fiber chromatic dispersion (CD) [1]–[4]. To date, the OFDM systems have included the coherent and direct detection approaches. The direct-detection optical OFDM (DDO-OFDM) [1], which uses a simpler receiver at a price of worse sensitivity when compared with coherent optical OFDM (CO-OFDM) [2]–[4], could be considered as an alternative modulation format for next-gener-ation metropolitan and long-haul terrestrial transmissions.

One claimed benefit of DDO-OFDM systems is the relaxed requirement for the laser linewidth: contrary to the high-cost external cavity laser (ECL) in CO-OFDM, a low-priced dis-tributed feedback (DFB) laser with a MHz-level linewidth, in general, is considerably acceptable in DDO-OFDM because of its better phase coherency between the carrier and sideband [21]. However, as depicted in Fig. 1, due to fiber CD, the carrier and the sideband would gradually walk off with the increased transmission length and eventually loss their phase coherency and result in significant phase noise (PN) in detection. The laser linewidth effect has been firstly identified in [5] with 12.5 Gbps Manuscript received December 18, 2009; revised June 20, 2010; accepted June 25, 2010. Date of publication July 01, 2010; date of current version August 18, 2010.

The author is with Department of Photonics and Institute of Electro-Optical Engineering, National Chiao Tung University, HsinChu 300, Taiwan (e-mail: pwr.eo92g@nctu.edu.tw).

Color versions of one or more of the figures in this paper are available online at http://ieeexplore.ieee.org.

Digital Object Identifier 10.1109/JLT.2010.2055834

Fig. 1. Origin of phase noise (PN) in DDO-OFDM transmission.

(32-quadrature-amplitude modulation, QAM) data rate and 320-km standard single mode fiber (SSMF) transmission. How-ever, the PN characteristics in DDO-OFDM systems, which are found to be quite different from that in CO-OFDM, should be clarified and characterized. In addition, the PN impact, in terms of its analytical forms with critical system parameters, should be provided from a view point of system design.

In this paper, we firstly present a PN model in DDO-OFDM transmission, characterize and emphasize its many unique prop-erties other than those in CO-OFDM. We find that the PN in DDO-OFDM has the following two significant differences from those in CO-OFDM: 1) the power and bandwidth, i.e., power spectral density (PSD), of PN in DDO-OFDM are functions of the subcarrier frequency and transmission length. Typically, a high-frequency subcarrier or a long-distant transmission would result in a larger PN power and a smaller PN bandwidth. 2) The PN bandwidth could range in MHz which is independent of the laser linewidth. Such a broad spectrum will inevitably in-troduce significant inter-carrier interference (ICI), making the PN compensator more difficult to design.

In addition to the PN characterization, we also analyze the PN effects on the received symbol, derive the PN power in terms of the system parameters, and present a simple BER estimator which is proven to be reliable provided the OSNR penalty is smaller than 2 dB. Furthermore, the numerical results demon-strate that, 1) with the same data rate, the lower QAM format would exhibit a better PN tolerance even though it suffers more CD and more PN power, 2) the PN tolerance, in terms of the maximum achievable fiber distance, could be easily scaled to different data rates and laser linewidths, which could help sim-plify the system design, and 3) the PN tolerance could be en-hanced by increasing the subcarrier number, which indicates 0733-8724/$26.00 © 2010 IEEE

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that a longer OFDM symbol duration would yield a better per-formance in the presence of PN.

The rest of this paper is organized as follows. In Section II, the linear system model in the presence of laser PN is provided. In Section III, we analyze the PN effects, derive the closed-form PN power, and offer a semi-analytical BER estimator evalu-ating the PN-induced OSNR penalty. In Section IV, numerical results and discussions are given with different data rates, laser linewidths, and subcarrier numbers. Finally, Section V concludes this paper.

Notably this paper will focus on the linear PN effect which is mainly comes from the interaction between the laser PN and the fiber CD, and all the presented results and conclusions are obtained without using any PN compensation technique, which currently for DDO-OFDM is still under explored.

II. SYSTEMMODEL

Throughout this paper we will consider the typical single polarization DDO-OFDM signal [7]–[9], which inserts a fre-quency gap with the same width as the data sideband and can be modeled by [8]

(1)

where is the imaginary unit, and are the complex am-plitudes of the carrier and the modulated symbol on th subcar-rier, respectively, is the number of data subcarriers, is the carrier’s baseband frequency, and is the subcarrier fre-quency spacing. We emphasize that the signal model (1) is com-patible with the following DDO-OFDM transmitters with each having different carrier frequency: i) optical-filtering transmitter [7], which retains the laser carrier and removes one of the sidebands with an optical filter. ii) Digital-carrier transmitter [8], which suppresses the laser carrier and in-serts a digital carrier by virtual of the digital signal processor (DSP). iii) Analog-carrier transmitter [9], which suppresses the laser carrier and inserts an analog carrier with an external radio frequency (RF) local oscillator. Since the carrier’s baseband frequency will not take any effect in de-riving the PN model, for simplicity we set its value to be zero, i.e., , for the following analysis.

The phase fluctuation of a laser , which is often quanti-fied by the laser linewidth , can generally be modeled by the Wiener process [6], [10], [12], [15], i.e.,

(2) where is a zero-mean stationary white Gaussian random process with a variance of . As a result, the phase fluctu-ation is a normal process with a zero mean and a variance of . To introduce this phase fluctuation to the typical DDO-OFDM signal (1), we simply multiply (1) with the noisy

carrier , which by definition is the laser PN. Thus, the signal model with PN can be given as

(3) For simplicity in (3) we leave out the pulse waveform term, which is typically a rectangular function with a duration defining the period of one OFDM symbol. From the viewpoint of fast Fourier transform (FFT), which presumes that each OFDM symbol extends periodically in the time domain, the above assumption would be still reasonable in the absence of the inter-symbol interference (ISI).

Based on the transmitter’s output signal , because of the power-detection nature of the photodiode, the laser PN will not appear in the converted electrical signal and thus will do no harm to the system performance. However, if after transmission, the signal with a certain amount of CD will have the different subcarriers experiencing different timing offset, which can be expressed as

(4) where * denotes the convolution operator,

is the impulse response of fiber CD with

, of which is the dispersion parameter, is the fiber length, is the operating wavelength, and is the light speed in vacuum. In deriving (4) we assume that the laser linewidth is relatively smaller than the subcarrier frequency spacing and ignore its finite bandwidth effect. Thus, the fiber CD only contributes a relative time delay between the th subcarrier and the optical carrier.

After the photodiode, the converted electrical signal will include the desired signal, the direct current (DC), and the sideband-sideband beat interference (SSBI) [8], which are expressed in sequence as follows:

(5)

where is the converted phase

fluc-tuation on th subcarrier and therefore stands for the converted PN (CPN) on th subcarrier,

(3)

is the CD-induced phase rotation on th subcar-rier, takes the real part of , and the superscript “*’ is the complex conjugator. Before the signal is sampled to the digital domain, we should firstly discuss the PSD of the CPN: , which is found to be quite different from that of the coherent PN: . The PSD of CPN, denoted as , had been previously derived in [10] and for convenience we have rewritten it with the herein presented parameters

(6) where is defined as the PN power on th sub-carrier. Contrary to the PN in CO-OFDM systems, the CPN in DDO-OFDM is a function of the subcarrier index (or subcar-rier frequency). Independent of the laser linewidth, the band-width of CPN is also found to be a function of the time delay and might range in the order of MHz, which will not simply pollute the th subcarrier itself but also corrupt its many adjacent subcarriers. Thus, after the signal is sampled and FFT demodulated, the th subcarrier symbol can be rep-resented as

(7)

where is the FFT size, is the th

sub-carrier symbol in the absence of PN, is the discrete-time converted phase fluctuation, and is the FFT of , rep-resenting the frequency-dependent interferences from th sub-carrier

(8) From (7) we found that the received th subcarrier symbol in-cludes not only the transmitted symbol , which is corrupted by , but also the ICI terms from adjacent symbols

where .

It is worth noting that (7) has a similar form as the conven-tional PN model in CO-OFDM systems [6], [10], [12], [15], ex-cept for the specific natures of CPN: 1) the subcarrier frequency dependency and 2) the much-broader bandwidth. In particular, the variance of the 0th-order interference , conventionally called the common phase error (CPE) in CO-OFDM systems [6], [11], [12], [14], would vary with the subcarrier frequency and would be no longer “common” to all subcarriers, Hence, for

Fig. 2. Effects of the PN on the received subcarrier signal: (1) power degrada-tion , (2) phase rotation term (PRT), and (3) inter-carrier interference (ICI).

DDO-OFDM we rename as “phase rotation term (PRT)” to distinguish it from its conventional name of CPE.

III. PERFORMANCEANALYSIS A. Phase Noise Effects

The PN effects on the received symbol can be mainly cate-gorized as the power degradation, PRT, and ICI, which can be intuitively understood via Fig. 2. Even though their power, for evaluating the electrical SNR or BER, can be obtained using the numerical approach with the PSD given in (6), we provide their analytical solutions which more clearly identify the direct rela-tions between the PN power and the system parameters.

a) Power Degradation: Since, under the corruption of

PN, part of the subcarrier power will leak to the PRT and ICI, the original transmitted subcarrier would inevitably suffer some power loss. The power degradation , defined as the power ratio between the th subcarrier with PN to the th subcarrier without PN can be obtained under the small PN assumption, i.e., , which in general is true for most practical trans-missions. Following the procedures described in Appendix I,

can be expressed as

(9) where takes the expectation of is the sampling time, and is the number of delay samples for th sub-carrier w.r.t the optical sub-carrier. From (9) we found , indicating that the power loss of the th subcarrier will turn to the PN power of th subcarrier.

b) Phase Rotation Term (PRT): According to the previous

definition, PRT is the 0th-order interference . Then, using (8) and the small PN assumption, PRT can be manipulated as follows:

(10) We found PRT will only disturb the signal’s imaginary part, and therefore results in a phase rotation. Because is a zero-mean Gaussian random variable, the PRT will also follow Gaussian random process with a zero mean and a variance of

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(11) where is the PN variance within a sample duration. The detailed derivation is in Appendix II. Notably in (11) we have not specifically denoted a subscript for ; however, the readers should know that the PRT power would always be a function of . In general, because the CP duration is typically longer than the subcarrier’ time delay , the PRT power (11) could be further simplified as , which is in proportion to . Therefore, the PRT power will enlarge with an increasing fiber length or/and a decreasing subcarrier number.

c) Inter-Carrier Interference (ICI): The noise behavior of

ICI has long been considered as a zero-mean complex Gaussian random variable [6], [12]. The ICI power is also a function of the subcarrier index and its variance, when normalized to the subcarrier symbol power, can be exactly obtained without using the small PN assumption

(12)

with (13), shown at the bottom of the page, where is the subcarrier symbol power in the absence of

PN, , and . The

exact derivation of (13) is provided in Appendix III. Similar to the PRT power, we also ignore the subscript for the ICI power denotation while the readers should know that the ICI power will always be a function of . Note that for deriving (12) the following assumption is applied

(14) which is true as long as the subcarrier symbols are

mutually-independent, i.e., where .

To simplify (12) and (13), we ignore the PSD difference of CPN for adjacent subcarriers, i.e.,

. Therefore, (12) can be approximated as

(15) where the upper-bound is achieved when . However, if the sideband bandwidth is larger than the CPN’s band-width, as is usual the case after a long-distant transmission, the ICI power would mostly come from the adjacent subcarriers and thus its value would be very close to this bound.

If we further use the small PN assumption for (15), with which can be simply approximated as the sum of the power degradation and PRT power, i.e.,

, then the bound in (15) can be re-expressed as

(16) which provides a very simple form for the upper-bound of the ICI power.

B. Bit Error Rate Estimation

In general, if the PN interferences of PRT and ICI, as well as the ASE beat noise, are mutually independent and follow the complex Gaussian distribution, then the BER can be simply es-timated via (12) and (13) in [13]. However, since the PRT will only rotate the subcarrier symbol phase and may not be simply assumed as complex Gaussian noise, an alternate BER estimator would be needed. For deriving the BER estimator, we mainly follow the procedures in [11] and assume that the PRT and ICI are mutually independent so that the conditional BER of th subcarrier, given a PRT-induced phase rotation , can be written as:

(17) with

(18)

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where the subscript of stands for the QAM size, i.e., 4 QAM, is the complement error function, is the th-subcarrier’s electrical signal-to-noise-ratio (ESNR) excluding the PRT power, and represents the th-subcarrier’s ESNR with the consideration of only ASE. The numerical method for has been well documented in [13] and thus is omitted here. Thus, the ensemble BER of th subcarrier, with the consideration of all possible PRT phase rotation, can be expressed as [11]

(19) where is the probability density function (PDF) of PRT, which follows the Gaussian distribution with a zero-mean and a variance of

(20) The system BER can then be obtained by taking the average of over all subcarriers [13]. Notably the BER with higher QAM formats can be easily derived with a similar form of (26) in [15].

It is worth noting that, given a fixed PN power (which implies that the total power of PRT and ICI is fixed), because the phase rotation would have a greater impact on BER, the system performance would be worse if the relative power of PRT is higher than that of ICI.

IV. NUMERICALRESULTS ANDDISCUSSIONS

Unless specified otherwise, the system parameters used in simulations are given as follows: 16-QAM format, 20-Gbps data rate, 20% cyclic prefix (CP), 160 data subcarriers , 256 FFT size , 2-MHz laser linewidth, and 16 ps/(nm.km) dispersion parameter. (1024 ) is chosen as the simulation bandwidth so that the broadband PN impact can be accurately evaluated. The fiber channel used in simulations considers only the linear chro-matic dispersion and at the receiver a 2nd-order Gaussian op-tical filter is applied with a -dB bandwidth equal to 1.2 ( ). No optical dispersion management is deployed in the link, and OSNR is evaluated in a noise bandwidth of 0.1 nm whenever ASE is considered.

A. Phase Noise Characteristics

To emphasize the uniqueness of PN in DDO-OFDM systems, in Figs. 3 and 4 we compare the PN characteristics of the CO-and DDO-OFDM systems. For Figs. 3(a) CO-and 4 we use Monte Carlo (MC) simulations while for Fig. 3(b) we use the analytical PSD given in (6). The ASE noise is ignored to focus on the PN behaviors. In Fig. 3(a) we show the phase fluctuations of 10 con-secutive OFDM symbols for the CO- and DDO-OFDM systems with a fiber length of 1600 km. For CO-OFDM we only draw the results of the central subcarrier since the phase fluctuation

Fig. 3. (a) (Converted) Phase fluctuations versus OFDM symbols for CO-and DDO-OFDM systems. (b) Power spectral density (PSD) of PN. Top: CO-OFDM, Center: DDO-OFDM, with 800-km SSMF,

Bottom: DDO-OFDM, with 1600-km SSMF. For all cases the ASE noise

is not considered.

Fig. 4. The effects of phase rotation term (PRT) and ICI on 16-QAM format in both CO- and DDO-OFDM systems. = 2 MHz., L = 1600 km. No ASE noise is considered.

will behave similarly among all subcarriers1; while for DDO-OFDM we show both the results of 1st and -th subcarrier to identify its subcarrier-dependent phase fluctua-tion characteristic. In CO-OFDM, the larger phase variance

1In CO-OFDM, due to the fiber CD, there will also be some relative time

delay among the transmitted subcarriers. However, because of the independency between the transmitter laser and the local oscillator, the overall PNs of each subcarrier will behave correlatedly with the same PSD following the Lorenzian shape.

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can be observed because of the random walk nature of the Wiener process, which allows the phase travels unlimitedly with increasing time. On the other hand, the phase variance of DDO-OFDM will be constrained by 2 and thus, unlike that in CO-OFDM, the phase will not go unbound-edly. Because in DDO-OFDM system the frequency spacing of between the carrier and the -th subcarrier is doubled than that of between the carrier and the 1st subcarrier, the expe-rienced time delay of -th subcarrier will also be doubled than that of 1st subcarrier, i.e., , thus resulting in an

doubled PN power, .

Fig. 3(b) shows the PSD of PN in CO-OFDM and DDO-OFDM systems. The PSD of PN in CO-OFDM is essentially follows the Lorentzian shape [10], which has a two-sided 3-dB bandwidth equal to the laser linewidth, i.e., 2 MHz in this demonstration. For DDO-OFDM, we show both the results of 1st and -th subcarrier with different fiber lengths of 800-km (center) and 1600-km (bottom). Compared with the PN in CO-OFDM, the PN in DDO-OFDM shows an relatively broader bandwidth (two-sided 3-dB bandwidth = 350 MHz for 160th subcarrier with 1600 km transmission), and be functions of both the subcarrier frequency and fiber length. Note that the first frequency null is located at around Hz2, which will cover its many adjacent subcarriers as long as the delay time is shorter than the cyclic-prefix (CP), i.e., , where is the CP duration. Such a broad PN spectrum will result in a high ICI power and thus the previously proposed CPE compensator [6], [14] would help limitedly for PN-corrupted DDO-OFDM systems.

In Fig. 4 we show that how the PN will affect the received constellations in both CO-OFDM and DDO-OFDM systems. For CO-OFDM, the PRT (previously CPE) strongly rotates the subcarrier symbol phase so that a digital CPE compensator is a must at the receiver [6]; while for DDO-OFDM, although the PRT also degrade the signal’s quality by introducing some phase deviations, the ICI has a more significant impact on the signal’s quality. The larger PN power of -th subcarrier can be clearly observed compared with that of 1st subcarrier.

Discussions: Contrary to the CO-OFDM, the power and

bandwidth of PN in DDO-OFDM are found to be functions of both the subcarrier frequency and transmission distance. Moreover, in a practical link the PN bandwidth might vary around MHz leading to a significant ICI power. Thus, based on these observations in this section, the previously pro-posed CPE compensator in CO-OFDM [6], [14], which doesn’t take care of the ICI, would inefficiently assist in recovering the PN-corrupted signals in DDO-OFDM3. On the other hand, the huge bandwidth of PN in DDO-OFDM would make the previous monitoring-tone compensator [15], [16], which needs an empty frequency band with a width approximately equal to the PN bandwidth, less spectrally-efficient. Therefore, these

2Based on (2), the converted phase fluctuation (t) is the integration of the

white Gaussian noisen(t) from (t 0 T k) to t, which equivalently filters this while Gaussian noise with a sinc-in-frequency filter with nulls at the multiples of(1=T k). With the small PN assumption where CPN 1 + j (t), the PSD of CPN will include the DC carrier and the PSD of (t), therefore resulting in the spectra in Fig. 3(b).

3When the ICI power is much more significant than the PRT power, this

scat-tered-pilot based CPE compensator could even yield a worse performance [20].

Fig. 5. Power of PRT and ICI for each subcarrier with Monte Carlo (MC) and the analytical approaches. UB: upper bound. The format is 4 QAM and the fiber length is 1500 km.

Fig. 6. BER versus OSNR with different transmission distances.

specific characteristics of PN in DDO-OFDM are motivating a new PN compensator for high-capacity transmissions that uses the low-cost DFB lasers.

B. Performance Evaluation

In this subsection, from Figs. 5 to 8 we will firstly demon-strate the effectiveness of the PN and BER models given in Section III, and then, from Fig. 9 to 11, we show that how the system parameters, such as data rates, laser linewidth, and sub-carrier number, will affect the OSNR penalty in the presence of laser PN.

In Fig. 5 we depict the power of PRT and ICI, with both the Monte Carlo (MC) and the presented analytical methods, as a function of subcarrier index in a 4-QAM, 1500-km transmis-sion system. The analytical results, obtained via (11) and (12) for PRT and ICI, respectively, are found to be coincident with the MC results, thus validating our analytical models for PN. On the other hand, except for the ICI power around the edges, the higher PN power can be found for higher-index (or higher-fre-quency) subcarriers, which are in agreement with the obser-vations from Figs. 3 and 4. The abrupt drop of the ICI power around the edges can be attributed to their fewer adjacent sub-carriers which naturally will contribute less ICI power. In par-ticular, the upper-bound (UB) of the ICI power from (16) is also presented and found to be very close to the exact ICI power for most central subcarriers. Therefore, due to the provided accu-racy and its very simple formula, (16) could be directly treated as the ICI power for the future PN-relevant investigations.

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Fig. 7. Constellations of the central (80th) subcarrier signal: (a) with the other 159 subcarriers assigned(1 + i), (b) with 1–79 subcarriers assigned (1 + i) and with 81–160 subcarriers assigned(1 0 i), (c) with all subcarriers assigned random symbols. 4-QAM and 1500-km fiber transmission are considered. The results are obtained using MC approach with no ASE.

Fig. 8. OSNR penalties versus the fiber length for 4-, 16- and 64-QAMs. To test the effectiveness of the presented BER estimator, in Fig. 6 we show the BER performances of 4-QAM format as a function of OSNR with both the MC approach and the BER es-timator (19). With a shorter fiber length (i.e., km), the re-sults from (19) are found to be well matched to the MC rere-sults for a BER down to . With a longer distance, however, the estimator becomes unable to yield an accurate BER. Therefore, the BER estimator only can provide reliable results when PN power is relatively smaller than ASE, i.e., under the conditions of either with a lower OSNR or a shorter transmission length. This BER disagreement mainly comes from the data pattern ef-fect of the subcarriers [17], which is not considered for (19).

The pattern effect on the BER estimator can be easily un-derstood via the received constellations. In Fig. 7, the 4-QAM constellations of the 80th subcarrier after 1500-km fiber trans-mission are shown under different conditions of (a) the rest sub-carriers assigned with the symbol of , (b) the first-half subcarriers (from 1 to 79) assigned with and the second halves (from 81 to 160) assigned with , and (c) the rest subcarriers left random. From Fig. 7(a) and (b) we found that the PN, unlike the regular complex Gaussian noise, scatters in a highly anisotropic manner and exhibits different directivity with different data patterns. However, from Fig. 7(c) the PN would still exhibit the semi-isotropic characteristic since this QAM diagram is assembled from many different data patterns with each contributing its unique directivity. This directly explains why the BER estimator (19) underestimates the exact BER even though the PRT and ICI power, as shown in Fig. 5, can be

accu-rately evaluated. Thus, an accurate BER model should take all possible data patterns and the corresponding noise directivity into account. Nevertheless, the computation effort with such an exhausted approach would increase exponentially with the sub-carrier number, therefore making such an accurate approach al-most prohibitive.

Even though the simple BER model (19) will underestimate the exact BER in the presence of a high PN power, we should discuss the effective range in which (19) could still yield an re-liable result. In Fig. 8 we investigate the OSNR penalties versus transmission length with 4-, 16-, and 64-QAM formats. Note that here the different QAMs are switched with a fixed data sub-carrier number 160. Both the results from the MC approach and the BER estimator (19) are shown for comparisons. If the max-imum estimation error, which is defined as, given a fiber dis-tance , the penalty difference between the MC results and the estimations by (19), is allowed to be 0.2 dB, we found that (19) can offer an acceptable estimation for both 16- and 64-QAM formats when the OSNR penalty is up to 3 dB; while for the 4-QAM format which suffers stronger PN, (19) can still yield an reliable estimation when the OSNR penalty is 2 dB. This demonstrates that (19) can reliably estimate the OSNR penalty when the OSNR penalty is 2 dB for all the considered QAM formats.

Although in Fig. 8 we have obtained the PN tolerances, in terms of the fiber length, for different QAM formats with a fixed 20-Gbps data rate and a 2-MHz laser linewidth. However, ques-tions would arise whether this PN-tolerance could be scaled to a different data rate or a different laser linewidth. Therefore, in Fig. 9 we discuss the data rate and linewidth scalability of the PN-tolerance in terms of the fiber length. Note that in Figs. 9–11, the results are obtained using MC approach with each point having at least bit errors. For simplicity, here we only dis-cuss the 16-QAM format while the other QAMs would yield the similar conclusions. Fig. 9(a) shows the OSNR penalties as a function of fiber length with different data rates -, 20-and 40 Gbps. With a certain OSNR penalty (ex. 3 dB), we de-note the corresponding fiber length as for data rate. Then the product of is found to be approximately a constant, i.e., . Thus, provided the QAM is hold un-changed, the PN-tolerance shown in Fig. 8 could be easily scaled to a different data rate with the rule of . Fur-thermore, in Fig. 9(b) we show the OSNR penalties as a func-tion of fiber length with different linewidths of , and MHz. Similarly we define the 3-dB fiber length to be , then the product of is found to vary implicitly with different

, that is, . Therefore, the

PN-tolerance could also be scaled to a different laser linewidth with the relation of . The above data rate and linewidth scalability can be clearly understood via the factors of the PN power, . For the same QAM format, the data rate is roughly in proportion to the subcarrier frequency , which can be further related to the time delay via

where is a constant. Therefore, given a fixed laser linewidth and a QAM format, a constant value will result in a con-stant , and thus a constant which implies a constant PN power. Therefore, the data-rate scalability simply suggests the

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Fig. 9. OSNR penalties versus fiber length for (a) different data rates, and (b) different laser linewidths.

Fig. 10. OSNR penalties versus the fiber length given a fixed L product of 1 600 (MHz.km) yielding a fixed PN power. This emphasizes that the power ratio between PRT and ICI is also important to the OSNR performance. system would perform similarly provided that the same PN power is given. Likewise, the linewidth scalability can also be realized with a similar manner.

Based on the above discussions, it appears that the OSNR penalty could be easily predicted by the PN power. However, the

Fig. 11. OSNR penalties versus the subcarrier number with two different trans-mission lengths. A larger subcarrier number, or alonger symbol duration, is found to have a better performance in the presence of laser PN.

derived data-rate and linewidth scalabilities are simply approx-imations and the performance would still change even under the same PN power. Shown in Fig. 10 is the OSNR penalty as a function of given a fixed linewidth and length product of (MHz km), which yields a fixed PN power. Two different subcarrier numbers and , which corre-spond to FFT sizes of 64 and 256, respectively, are investigated for comparisons. With both the subcarrier numbers we found the performance would continuously become worse as the length in-creases, which is more evident especially with the smaller sub-carrier number. These observations stems from the following reasons: given a PN power , 1) a longer distance would yield a larger through the relation of , which indicates that the PRT power would increase with the fiber length and decrease with the subcarrier number. 2) Subsequently, a larger PRT power would lead to a greater OSNR penalty since PRT, rotating randomly the subcarrier symbol phase, typically has a more severe impact than ICI. Thus, even given a fixed PN power, the longer fiber length , or a smaller subcarrier number N, would have a rela-tively larger OSNR penalty.

Now we investigate how the subcarrier number, i.e., symbol duration, will affect the system performance in the presence of PN. Shown in Fig. 11 are the OSNR penalties versus the subcar-rier number with two distinct fiber lengths. Note for Fig. 11 we have removed the constraint of a constant PN power, which is put on Fig. 10. We found 1) the OSNR penalty is more sensitive to the subcarrier number in the case with a longer fiber length, and 2) the greater subcarrier number would yield a lower OSNR penalty for both the considered fiber lengths. In particular, the OSNR improvement brought by the subcarrier number is found to be almost diminished when the subcarrier number is beyond some threshold which depends on the fiber length. As a con-clusion for Fig. 11, the longer OFDM symbol duration is more attractive for the better PN tolerance in DDO-OFDM transmis-sions under the condition of no PN management.

Discussions: Even though the DDO-OFDM signal has long

been considered to be immune to fiber CD and suitable for long-distant transmission, however, this would not be definitely true

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if a low-cost DFB laser is applied in the transmitter. Considering a 16-QAM, 20-Gbps single-band DDO-OFDM transmission [18], a commercial DFB laser with 2-MHz linewidth will limit the 3-dB fiber length to be -km, which would constrain the high-capacity DDO-OFDM signals to the local access and metropolitan networks. To increase the PN-limited fiber length, possible strategies might include: 1) Low-QAM format, which, as indicated in this paper, provides a larger PN margin at a price of a lower spectral efficiency. 2) Digital compensators, which, to date, has not been extensively studied for DDO-OFDM. 3) Multi-band transmissions (including the polarization-division multiplexing, PDM), which transmits one carrier for each band to reduce the frequency spacing between the carrier and side-band. 4) Virtual SSB-OFDM, which naturally exhibits a higher PN tolerance with the halved signal bandwidth [19]. 5) ECL, which, although with a high price presently, could greatly in-crease the 3-dB fiber length with its typical linewidth of only 100 kHz. However, among the presented strategies here, if a specified transmission format is given, only (2) and (5) could improve the PN-limited distance, which might lead to a fight between the cost of ECL and the complexity of a digital com-pensator. Since the aim of this paper is mainly to analyze the PN characteristics and its impact on the system performance, further discussion on the PN compensation is out-of-scope of this paper and should appear in an alternate publication.

V. CONCLUSION

We have characterized the PN impact in DDO-OFDM systems and identified its many differences from those in CO-OFDM. The PN effects, categorized as the power degrada-tion, PRT, and ICI, are analyzed in detail and their powers, in terms of critical system parameters, are given with closed-form expressions. Via the numerical results, we have verified the presented PN models and demonstrated that the given BER estimator could be reliable provided that the OSNR penalty is dB. We have also investigated the PN tolerances, in terms of achievable fiber length given a certain OSNR penalty, with diverse system parameters, such as QAM formats, data rates, laser linewidths, and subcarrier numbers and showed that the PN tolerance could be roughly scaled to a different data rate and laser linewidth which could help simplify the link design process in the future. Finally, for DDO-OFDM a longer OFDM symbol duration is found to have a more robust tolerance against laser PN in the absence of PN management.

APPENDIXI

For the th subcarrier, the delayed samples with respect to the optical carrier is denoted as , that is, where

is the relative time delay w. r. t. the carrier and is the sample duration. Then the discrete-time converted phase fluc-tuation can be expressed as the summation of mutu-ally-independent Gaussian random variables starting from

to

(A1) Note that each single represents the phase fluctuation within one sample duration with a zero-mean and a variance of

, where is the laser linewidth.

To derive the power degradation, where is the expectation of , we will firstly obtain the expecta-tion of the 0th-order interference, , and then the power degradation will be derived by simply taking the square of it. With small PN assumption, i.e.,

can be manipulated as follows:

(A2)

where for is used. The power

degra-dation is then obtained via

(A3) APPENDIXII

The PRT power is the variance of (0), which can be derived following the below procedures

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(A6)

(A7)

(A4)

APPENDIXIII

The power of the th interference bin from th subcarrier, , can be expressed as: Depending on the range of , (A5) will be separately manipulated with the proce-dures similar to [14]. Here we firstly consider the case for

where takes the real part of and . Similar to the procedures deriving (A6), we can

manipulate (A5) for where

.

REFERENCES

[1] B. J. C. Schmidt, Z. Zan, L. B. Du, and A. J. Lowery, “100 Gbit/s trans-mission using single-band direct-detection optical OFDM,” in Proc.

OFC, San Diego, CA, Mar. 2009, Paper PDPC3.

[2] Y. Ma, Q. Yang, Y. Tang, S. Chen, and W. Shieh, “1-Tbps per channel coherent optical OFDM transmission with sub-wavelength bandwidth access,” in Proc. OFC, San Diego, CA, Mar. 2009, paper PDPC1. [3] H. Takahashi, A. Amin, S. L. Jansen, I. Morita, and H. Tanaka,

“DWDM transmission with 7.0-bit/s/Hz spectral efficiency using 82 65.1-Gb/s coherent PDM-OFDM signals,” in Proc. Optical Fiber

Commun. Conf., San Diego, CA, Mar. 2009, paper PDPB7.

[4] S. L. Jansen, A. Amin, H. Takahashi, I. Morita, and H. Tanaka, “132.2-Gb/s PDM-8QAM-OFDM transmission at 4-b/s/Hz spectral efficiency,” IEEE Photon. Technol. Lett., vol. 21, no. 12, pp. 802–804, Jun. 2009.

[5] Z. Zan, M. Premaratne, and A. J. Lowery, “Laser RIN and linewidth requirements for direct detection optical OFDM,” CLEO’08 Paper CWN2.

[6] X. Yi, W. Shieh, and Y. Ma, “Phase noise effects on high spectral effi-ciency coherent optical OFDM systems,” J. Lightw. Technol., vol. 26, no. 10, pp. 1309–1316, May 2008.

[7] A. J. Lowery, L. B. Du, and J. Armstrong, “Performance of optical OFDM in ultra long haul WDM lightwave systems,” J. Lightw.

Technol., vol. 25, no. 1, pp. 131–138, Jan. 2007, OWM4.

[8] W.-R. Peng, X. Wu, V. R. Arbab, K.-M. Feng, B. Shamee, L. C. Christen, J.-Y. Yang, A. E. Willner, and S. Chi, “Theoretical and experimental investigations of direct-detected RF-tone assisted optical OFDM systems,” J. Lightw. Technol., vol. 27, no. 10, pp. 1332–1339, May 2009.

[9] B. J. C. Schmidt, A. J. Lowery, and L. B. Du, “Low sampling rate transmitter for direct-detection optical OFDM system,” in Proc.

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[10] G. Qi, J. Yao, J. Seregelyi, S. Paquet, C. Belisle, X. Zhang, K. Wu, and R. Kashyap, “Phase-noise analysis of optically generated millimeter-wave signals with external optical modulation techniques,” J. Lightw.

Technol., vol. 24, no. 12, pp. 4861–4875, Dec. 2006.

[11] P. Liu and Y. Bar-Ness, “Closed-form expressions for BER perfor-mance in OFDM systems with phase noise,” in IEEE Proc. ICC, 2006, pp. 5366–5370.

[12] L. Tomba, “On the effect of Wiener phase noise in OFDM systems,”

IEEE Trans. Commun., vol. 46, no. 5, pp. 580–583, May 1998.

[13] W.-R. Peng, K.-M. Feng, A. E. Willner, and S. Chi, “Estimation of the bit error rate for direct-detected OFDM signals with optically pre-am-plified receivers,” J. Lightw. Technol., vol. 27, no. 10, pp. 1340–1346, May 2009.

[14] S. Wu and Y. Bar-Ness, “OFDM systems in the presence of phase noise: Consequences and solutions,” IEEE Trans. Commun., vol. 52, no. 11, pp. 1988–1996, Nov. 2004.

[15] M. S. El-Tanany, Y. Wu, and L. Hazy, “Analytical modeling and sim-ulation of phase noise interference in OFDM-based digital television terrestrial broadcasting systems,” IEEE Trans. Broadcast., vol. 47, no. 1, pp. 20–31, Mar. 2001.

[16] S. L. Jansen, I. Morita, T. C. W. Schenk, N. Takeda, and H. Tanaka, “Coherent optical 25.8 Gb/s OFDM transmission over 4160-km SSMF,” J. Lightw. Technol., vol. 26, no. 1, pp. 6–15, Jan. 2008. [17] R. Corvaja and S. Puolin, “Phase noise spectral limits in OFDM

sys-tems,” Wireless Pers. Commun., vol. 36, pp. 229–244, 2006. [18] A. Amin, H. Takahashi, I. Morita, and H. Tanaka, “Polarization

multi-plexed 100-Gbps direct detection OFDM transmission without MIMO processing,” in Proc. ECOC’09, Paper 1.3.1..

[19] W.-R. Peng, B. Zhang, K.-M. Feng, X. Wu, A. E. Willner, and S. Chi, “Spectrally efficient direct-detected optical OFDM transmission using a tunable gap and an iterative detection schemes,” J. Lightw. Technol., vol. 27, no. 24, pp. 5723–5735, Dec. 2009.

[20] A. G. Armada and M. Calvo, “Phase noise and subcarrier spacing ef-fects on the performance of an OFDM communication system,” IEEE

Commun. Lett., vol. 2, no. 1, pp. 11–13, Jan. 1998.

[21] D. Qian, J. Yu, J. Hu, L. Zong, L. Xu, and T. Wang, “10 Gb/s WDM-SSB-OFDM transmission over 1000 km SSMF using conven-tional DFB lasers and direct-detection,” Electron. Lett., vol. 44, no. 3, pp. 223–225, Jan. 2008.

Wei-Ren Peng received the B.S.E.E. degree from National Taiwan University,

Taiwan, in 2001, and the M.S. and Ph.D. degrees in electro-optical engineering from National Chiao Tung University, Taiwan, in 2003 and 2008, respectively. In 2007, he was a visiting researcher at Optical Communications Labora-tory at University of Southern California, US, under the supervision of Prof. Alan Willner, working on optical orthogonal frequency division multiplexing (O-OFDM) experiments. In 2009 he worked as a postdoctoral fellow at National Chiao Tung University, Taiwan, focusing on the performance analysis of op-tical OFDM transmissions. Currently he engages some opop-tical OFDM projects in KDDI R Laboratories, Japan, under contract.

Dr. Peng has authored or coauthored more than 65 papers in prestigious inter-national journals and conferences. He also serves as a paper reviewer for IEEE and OSA journals. His current interest is the impairment compensation using digital signal processing (DSP) for optical long-haul transmissions.

數據

Fig. 1. Origin of phase noise (PN) in DDO-OFDM transmission.
Fig. 2. Effects of the PN on the received subcarrier signal: (1) power degrada- degrada-tion , (2) phase rotation term (PRT), and (3) inter-carrier interference (ICI).
Fig. 3. (a) (Converted) Phase fluctuations versus OFDM symbols for CO-and DDO-OFDM systems
Fig. 5. Power of PRT and ICI for each subcarrier with Monte Carlo (MC) and the analytical approaches
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