Lightwave Technology

Chapter 9.5.4 - Use of DPSK Format

9.5.4 Use of DPSK Format

Similar to the case of phase-alternation technique discussed in Section 8.5.2 for suppressing the intrachannel nonlinear effects, one may ask whether pulse phases can be adjusted to reduce the interchannel nonlinear effects. The answer turns out to be yes. The modulation format that has proved quite successful in this respect is the RZ-DPSK format (see Section 2.3.4) in which an optical pulse is present in all bit slots and the information is encoded in the phase of these pulses through DPSK [128]-[132]. Figure 9.25 shows schematically how the field amplitude and optical power vary with time for a DPSK-coded channel in which the phase of pulses is shifted by π whenever a bit transition occurs.

It is easy to understand qualitatively why XPM-induced penalties are reduced for systems designed with the RZ-DPSK format. The main reason why interchannel XPM leads to the amplitude and timing jitter is related to the randomness of bit patterns in two neighboring channels. It is easy to see that the XPM will be totally harmless if channel powers were constant in time because all XPM-induced phase shifts will be time-independent, producing no frequency and temporal shifts. However, this is not the case for the RZ-DPSK systems because, even though information is coded through phase shifts, an optical pulse is present in all bit slots. As seen in Figure 9.25, channel powers vary in a periodic fashion under such conditions. Nevertheless, the XPM effects are considerably reduced because all bits experience the same bit patterns in the neighboring channels and undergo nearly identical collision histories, especially if the average channel power does not vary too much along the link. Since all bits are shifted in time by nearly the same amount, little timing jitter is induced by interchannel collisions.

09_05_04_Lightwave_Technology-1.jpg

Figure 9.25: Temporal variations of the electric field and optical power for a 10-Gb/s channel coded using the RZ-DPSK format. (After Ref. [129]; ©2002 IEEE.)


For a more quantitative analysis, we should include the walk-off effects through Eqs. (9.4.3) and (9.4.4) since pulses in two channels travel at different speeds. If we ignore pulse broadening induced by GVD in these equations, the XPM-induced phase shift on a pulse in channel 1 depends on power variations in channel 2 as

09_05_04_Lightwave_Technology-2.jpg

where P2(t) = P0U(0,t)2 governs power variations in channel 2 and δ = β2Ωch depends on the channel spacing. If lumped amplifiers are used to compensate for fiber losses, p(z) = exp(-αz) in each fiber section between two amplifiers. By taking the Fourier transform of Eq. (9.5.1), we obtain [129]

09_05_04_Lightwave_Technology-3.jpg

where we used L = NALAand assumed that the link is made of NAamplifiers spaced apart by LAsuch that αLA>> 1.

Equation (9.5.2) shows that the fiber link acts as a low-pass filter of bandwidth fb = α / (2πβ2Ωch) as far as the transfer of power variations into phase variations is concerned [129]. Using typical parameter values for a WDM system designed with standard fibers, α = 0.2 dB/km, D = 17 ps/(km-nm), and 100-GHz channel spacing, this frequency is found to be around 540 MHz, a value much smaller than typical channel bit rates. Since the spectrum2(ω) of a periodic pulse train consists of discrete frequency components separated by the bit rate B, only the zero-frequency (dc) component is passed by the low-pass filter. As a result, the XPM-induced phase shift is nearly constant in time even for RZ pulses, and no frequency and temporal shifts occur during interchannel collisions.

Numerical simulations performed for an eight-channel WDM system confirm this simple analysis [129]. Figure 9.26 compares the calculated eye-opening penalty for the fourth channel in the case of standard RZ-ASK and RZ-DPSK formats, when channels operate at 10 Gb/s and are spaced 100 GHz apart. Each span between two amplifiers consists of 100 km of standard fiber, followed with a DCF of suitable length. Each channel carries chirp-free RZ pulses with 8-mW peak power. Residual dispersion of each channel is compensated at the receiver end to optimize the eye opening, measured in a 20-ps time window. As seen in Figure 9.26, penalty increases rapidly for the standard RZ format but does not exceed even 1 dB at a distance of 3000 km when the DPSK format is employed.

09_05_04_Lightwave_Technology-4.jpg

Figure 9.26: Eye-opening penalty (EOP) as a function of link length for one of eight channels in the case of RZ-ASK and RZ-DPSK formats. Eye diagrams at a distance of 3,000 km are also shown for the two formats. (After Ref. [129]; ©2002 IEEE.)


It should be mentioned that the reduction of interchannel XPM effects through RZ-DPSK does not come without a penalty, as it is accompanied in practice with the enhanced intrachannel SPM effects [132]. The reason is related to the fact that SPM-induced phase shift depends on the channel power. As a result, any power fluctuations induced by the amplifier noise are converted through SPM into phase [133], which affect the detection of the phase difference between two neighboring bits of that channel. Moreover, interchannel XPM produces additional phase fluctuations [134]. As a result, the use of RZ-DPSK is rarely beneficial for a single-channel system or for WDM systems with a relatively large channel spacing. Nevertheless, this format provides better performance when spectral efficiency is enhanced by reducing the channel spacing. We discuss this issue in the following section.

UNLIMITED FREE
ACCESS
TO THE WORLD'S BEST IDEAS

SUBMIT
Already a GlobalSpec user? Log in.

This is embarrasing...

An error occurred while processing the form. Please try again in a few minutes.

Customize Your GlobalSpec Experience

Category: Optical Linear Encoders
Finish!
Privacy Policy

This is embarrasing...

An error occurred while processing the form. Please try again in a few minutes.