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Calhoun: The NPS Institutional Archive Theses and Dissertations Thesis Collection 1994-06 A simple analytical model for dense WDM/OOK systems Tso-Chuan Chou. Chou, Tso-Chuan Monterey, California. Naval Postgraduate School http://hdl.handle.net/10945/42887

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Page 1: A simple analytical model for dense WDM/OOK systems Tso-Chuan … · 2016. 7. 4. · Tso-Chuan Chou LCDR, Taiwan Navy B.S, Chinese Naval Academy, November 1983 Submitted in partial

Calhoun: The NPS Institutional Archive

Theses and Dissertations Thesis Collection

1994-06

A simple analytical model for dense WDM/OOK

systems Tso-Chuan Chou.

Chou, Tso-Chuan

Monterey, California. Naval Postgraduate School

http://hdl.handle.net/10945/42887

Page 2: A simple analytical model for dense WDM/OOK systems Tso-Chuan … · 2016. 7. 4. · Tso-Chuan Chou LCDR, Taiwan Navy B.S, Chinese Naval Academy, November 1983 Submitted in partial

AD-A283 229

NAVAL POSTGRADUATE SCHOOL

Monterey, California

A R A DD 10 DT I c94-25527

ELECTE

TSS AUG 15 19943

A SIMPLE ANALYTICAL MODEL FOR DENSE WDM/OOK SYSTEMS

by

Tso-Chuan, Chou

June 1994

Thesis Advisor: Th T. Ha

Thesis Co-Advisor: Randy L. Borchardt

Approved for public release; distribution is unlimited.

9428h12049

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REPORT DOCUMENTATION PAGE From Approved OMB No. 0704

Public repoingm burden for tha colltaim ofidnfemrAion is edimatad to avage I hour per reqome. induding tutme for reviewfn iA&Wtiw, sdhgexisting data sources gpat md imammioaig dat needed, a.d conwkig and reviewing the c on of ifonatn Sed cmmenws rerdmg thisburdn etim a or any othe apet of thu collemtiom o(daonation. including susgatio for reducn ths burd to Waston Headuawn Sevics anBmuge. Paework Reduction Proj (070oo4.01) Wahinso DC 20503

1. AGENCY USE ONLY 2. REPORT DATE 3. REPORT TYPE AND DATES COVERED(Leave Blank) IJune 1994 Masters Thesis

4. TITLE AND SUBTITLE S. FUNDING NUMBERS

A SIMPLE ANALYTICAL MODEL FOR DENSE WDM/OOKSYSTEMS

6. AUTHOR(S) TSO-CHUAN. CHOU

7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) 8. PERFORMING ORGANIZATIONNaval Postgraduate School REPORT NUMBERMonterey. CA 93943-5000

9. SPONSORING/MONITORING AGENCY NAME(S) AND 10. SPONSORING/MONITORINGADDRESS(ES) AGENCY REPORT NUMBER

11. SUPPLEMENTARY NOTESThe views expressed in this thesis are those of the author and do not reflect the official policy or position of theDepartment of Defense or the U.S. Goverment.

12a. DISTRIBUTION/AVAILABILITY STATEMENT 12b. DISTRIBUTION CODEApproved for public release; distribution is unlimited. *A

13. ABSTRACT (maximum 200 words)We derive the closed form expression for the bit error probability of dense WDM systems employing an external OOK

modulator. Our model is based upon a close approximation of the optical Fabry-Perot filter in the receiver as a single-poleRC filter for the signals that are bandlimuted to a frequency band approximately equal to one sixtieth of the Fabry-Perotfilter's free spectral range. Our model can handle bit rates up to 2.5 Gb/s for a free spectral range of 3800 GHz and up to 5Gb/s when the power penalty is I dB or less.

14. SUBJECT TERMS 15. NUMBER OF PAGES69

16. PRICE CODE

17. SECURITY CLASSIF- 18. SECURITY CLASSIF- 19. SECURITY CLASSIFIC- 20. LIMITATION OFICATION REPORT ICATION OF THIS ATION OF ABSTRACT ABSTRACTUnclassified PAGE Unclassified UL

Unclassified

NSN 7540-01-280-5500 Standard Form 298 (Rev. 2-89)

Panraibed by ANSI SUd. 239-13

Page 4: A simple analytical model for dense WDM/OOK systems Tso-Chuan … · 2016. 7. 4. · Tso-Chuan Chou LCDR, Taiwan Navy B.S, Chinese Naval Academy, November 1983 Submitted in partial

Approved for public release; distribution is unlimited.

A SIMPLE ANALYTICAL MODEL FOR DENSE WDM/OOK SYSTEMS

by

Tso-Chuan ChouLCDR, Taiwan Navy

B.S, Chinese Naval Academy, November 1983

Submitted in partial fulfillment

of the requirements for the degree of

MASTER OF SCIENCE IN ELECTRICAL ENGINEERING

from the

NAVAL POSTGRADUATE SCHOOLJune, 1994

Author: Tso-Chuan Chou

Approved By:

Tri T. Thesis Advisor

R•dy L. Borchardt, Co-Advisor

Michael A. Morgan, ChaidanDepartment of Electrical and Computer Engineering

ii

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ABSTRACT

We derive the closed form expression for the bit error probability of dense WDM

systems employing an external OOK modulator. Our model is based upon a close

approximation of the optical Fabry-Perot filter in the receiver as a single-pole RC filter for

signals that are bandlimited to a frequency band approximately equal to one sixtieth of the

Fabry-Perot filter's free spectral range. Our model can handle bit rates up to 2.5 Gb/s for

a free spectral range of 3800 GHz and up to 5 Gb/s when the power penalty is 1 dB or

less.

Accesion Fof

NTIS CRA&IDTIC TABUnannounced 0Justification .................

Distribution I

Availability CodesAvail and / or

Dist Special

dPI

iii°o

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TABLE OF CONTENTS

I. INTRODUCTION ..................................................................... 1

IL ANALYSIS ........................................... ...................................................... .......... 4

A. INPUT SIGNAL. ............................ ....................... .............................. ......... 4

B. FABRY-PEROT FILTERED OUTPUT SIGNAL ........................................ 6

C. DECISION VARIABLES ............................................................................... 12

D. BIT ERROR PROBABILITY ........................................................................ 14

II. NUMERICAL RESULTS ................................................................................... 16

IV. CONCLUSIONS .................................................................................................. 27

APPENDIX A - DERIVATION OF FORMULA FOR DECISION VARIABLES...23

APPENDIX B - MATLAB COMPUTER PROGRAMS ........................................ 55

LIST OF REFERENCES ........................................................................................... 60

INITIAL DISTRIBUTION ........................................................................................ 62

iv

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LIST OF FIGURES

Figure 1: OOK receiver structure ............................................................................... $

Figure 2: Spectral characteristics of the Fabry-Perot fidter and the approximatedsingle-pole RC lowpass filter .................................................................. 9

Figure 3: Normalized impulse response of the Fabry-Perot filter and theapproximated single-pole RC lowpuass ilter ....................................... 10

Figure 4: Probability of bit error versus signal-to-noise ratio as a function ofnormalized channel spacing for cT - ................................................ 17

Figure 5: Probability of bit error versus signal-to-noise ratio as a function ofnormalized channel spacing for cT =10 ............................................... is

Figure 6: Power penalty versus normalized channel spacing as a function ofFabry-Perot fidter parameter cT ........................................................ 20

Figure 7: Power penalty versus normalized channel spacing as a function ofFabry-Perot fdter parameter cT with a fixed threshold a -0.5 ............... 22

Figure 8: Worst-case power penalty versus normalized channel spacing as afunction of Fabry-Perot fdter parameter cT with optimal thresholda = (X*+XI)/2 ................................................................................. .23

Figure 9: Worst-case power penalty versus normalized channel spacing as afunction of Fabry-Perot filter parameter cT with fixed thresholda = 0.5 ............................................................................................ 24

Figure 10: The normalized optimal threshold versus normalized channel spacing asa function of Fabry-Perot filter parameter cT .............. ............ 26

V

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L INTRODUCTION

Wavelength division multiplexing (WDM) systems have been increasingly proposed

as an attractive alternative to coherent optical frequency division multiplexing (FDM)

systems [Ref 1-5]. Although WDM systems with direct detection do not have the

channel capacity of coherent optical FDM systems, they are much less costly to

implement. Furthermore, present filter technology enables the designers to tightly pack

the channel, resulting in dense WDM systems that can provide aggregate bit rates of many

terabits per second (1 TbIs = 1•' b/s). Dense WDM systems are particularly attractive in

the area of undersea surveillance where hundreds of sensors and data collection sites are

envisioned being merged onto single-fiber superhighways through massive data fuision.

Other applications call for relatively low-bandwidth data collection over many months to

be dumped quickly to a remote recording site in a matter of minutes. This

"collection-and-dumped" compression can demand total data rates on the order of

hundreds of Gb/s. Long distance between data collection sites and a remote recording site

requires the use of optical amplifiers. Therefore, it is necessary to pack all channels within

the optical amplifier bandwidth.

A dense WDM receiver with on-off-keying (OOK) modulation can be modeled as

shown in Fig. 1. Conceptually, the analysis involves two main operations: 1) a

convolution operation to evaluate the signal at the output of the optical filter, a

1

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Fabry-Perot (FP) filter in our investigation, and 2) the integration of the output of the

photodetector. Evaluation of bit error probability by the numerical analysis of these two

operations has been carried out in [Ref 6], with a number of approximations made to

reduce the computational complexity. In this investigation the FP filter is shown to be

well approximated by an RC filter within the frequency range I f-f. I < FSR / 207c, where

FSR is the free spectral range of the FP filter [Ref 7] andfo is the FP filter center

frequency. For example, given FSR = 3800 GHz, the approximation works very well for

I f-f 0 I < 60.5 GHz; that is, the effects of adjacent channels within a 121 GHz bandwidth

centered at fo must be included, while all others can be neglected. This simple model

agrees well with [Ref 6] as demonstrated in Section III. Furthermore, this model enables

us to obtain a closed form analytical expression for the bit error probability for which

numerical results can be obtained with little effort. Our investigation shows that this

simple model provides accurate results as compared to those in [Ref 6] for bit rates up to

2.5 Gb/s when the effects of four adjacent channels are included with FSR = 3800 GHz.

Actually, when the power penalty relative to single channel operation is I dB or less, there

is virtually no difference in the effect of four or two adjacent channels. Thus, for this

power penalty criterion, this simple model can handle bit rates up to 5 Gb/s for a FP filter's

FSR = 3800 GHz.

In Section II the closed form expression for the decision variable, and consequently,

the bit error probability assuming all channels are bit synchronous as in [Ref 6] is derived.

Section III presents the numerical results which include the bit error probability versus the

2

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signal-to-noise ratio as function of the FP filter bandwidth and channel spacing, and the

power penalty (relative to single channel operation without filtering or with filtering but no

intersymbol interference) versus the channel spacing as a function of the bandwidth.

Finally, a summary of results appears in Section IV.

3

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IL ANALYSIS

The receiver model for the dense WDM system is shown in Fig. I. The desired

signal is filtered by a Fabry-Perot (FP) filter that rejects adjacent channels. The

photodetector is assumed to have a responsivity f (A/W). The detected current is

amplified by a low noise amplifier that contributes a postdetection thermal noise n() with

spectral density No (A2/Hz). The decision variable at the output of the integration is

compared to a threshold a to determine whether a bit zero or bit one was present.

A. INPUT SIGNAL

For convenience, we designate channel 0 as the desired channel, and channel k as

an adjacent channel where k = -M/2, ..., -1, 1, ... , M2 with M an even integer. We

consider the equivalent lowpass (complex envelope) data signal in channel 0 and channel k

as follows:

bo() = bo,,pT -T- (15=-Lo

bk(t) = Y bk, 'eiok pT(tO-17) (2)I=-L

where

T." bit duration

b,,, ={0,1 ): bit in channel 0 in the time interval (iT, (i+1)7)

b,, =(O,e''*)is the ' bit in channel k in the time interval (IT,(l+I)7)

4

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0E--)

E-4

I E-

-H-

E-4 b.

0

E- U0 w-U

I.-'

C4 z0

Cf)

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a phase offset between channel k and channel 0 and is assumed to be uniformly

distributed in (0, 2n) radians

Wk 'radian frequency spacing between channel k and channel 0 with (ok -- -0-k

The function prl - il ) is defined as

1, iT<t<(i+l)T(3pr(t- iT) = { o, odmurise()

In both (1) and (2), the non-negative integers Lo and L represent the number of bits in

channel 0 and k, respectively, that proceed the detected bits bo.o. The received dense

WDM equivalent lowpass signal at the input of the FP filter is given by

M12r(t) = FPboXW+ M: FP NO (4)

k=-M12k*-

where P is the received optical power.

B. FABRY-PEROT FILTERED OUTPUT SIGNAL

The FP filter can be characterized by the following equivalent lowpass transfer

function [Ref 1,7]

H(f) I-p I-A-p

6

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I-p l-A-pI-p COS(2)+jp sin(,!) i-p

where p is the power reflectivity, A is the power absorption loss (zero for an ideal FP

filter) and FSR is the free spectral range. For If! < FSR/20it and assuming A = 0, we can

approximate H (f) as follow:l-p _ 1

H(f) -Plp)+j1 • fi +j 21

2sj2, If I < FSR/0I2O (6a)

where

FSR(I-p)C = p (6b)

The free spectral range FSR can be related to the full width at half maximum (FWHM)

bandwidth B and the finess F of the FP filter as

FSR = -P--- = BF (7)

Thus if the signal is bandlimited to If I < FSR/20x, we can truly approximate (5) with a

single-pole RC filter with the following transfer function and impulse response

H(f ) = ---. (--1+j29 (8)

7

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h(t) = ce' , t > 0 (9)

Figures 2a-b show the magnitude and phase (radians) of H(f) of the FP filter in (5) and

its single-pole RC filter approximation given in (8) for p = 0.99, F = 312,6, B = 12.1 GHz

and FSR = 3800 GHz. Note that as the frequency increases, the phases of the FP filter

and the RC filter differ markedly, but the magnitudes of their transfer functions remain

identical and attenuate rapidly. When I f I > FSR/20, the magnitude of H(f) is very

small, and therefore, the effect of adjacent channel interference beyond this frequency

range is negligible. Figure. 3 shows the normalized impulse response of both FP and

single-pole RC filters. In summary, the above approximation is valid for dense WDM

analysis when the filter finess F is large or equivalently the FWHM bandwidth B is small

since the equivalent lowpass signal must be bandlimited to about I f I < FSR/20n.

This approximation has been used in [Ref 5] to study spectral efficiency of optical

FDM/ASK systems, which involves the evaluation of the decision variable for worst-case

analysis using the eye diagram technique. Since we are interested in the detected bit b 0.0

in the time interval ( 0, T), we consider the output filtered signal s(t), t< V < T given by

s(t) = SB(t) + SISI(t) + SAC(t), 0 < t < T (10)

where

s. (1): desired signal

.. , (t): intersymbol interference signal

8

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___FPflMw

IW03dxmate RC MWteA=O (ideal

~0.5- FSR-3800 0HzB (bandwidth of FP) : 12.160GHz

01 0 . . .. ,, aW I I - .

10 101 102 10 10Frequency in GHz

(a)I I"" "1. . . I . .. I

Z.1

I.-2100 10' 102 10

Frequency In GHz(b)

Figure 2: Spectral characteristics of the Fabry-Perot filter and the approximatedsingle-pole RC lowpass filter

9

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1

0.9 - FP filter

0.8* approximate RC filter

0.7

0.6

•0.5

0.4-

0.3-

0.2-

0.1-

00 0.05 0.1 0.15 0.2 0.25

time (ns)

Figure 3: Normalized impulse response of the Fabry-Perot filter and the approximatedsingle-pole RC iowpass filter

10

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t

SB() = #'bo, o f h(t- r)dr0

= JPbo,o(l -el'), 0 < t < T (Ii)

P ý (i+l)TsjsI(t)= 4T": - bo,, j h(t- r)d

iT

= e-ct bo, (e('+l)cT--eicT), 0 < t < T (12)j=-Lo

(l+)T

SAC,(t) = 1 T f2 { bk,, h(t- T)eDkdr]k=-M12 I=-L IT

k*O

+bk, of h(t-r)ejdk"dt}, 0 < t < T0

T+ cell 2 { bk'I(e(c+J(ok)(+l)Tk--M12 CJOlk j=-.

-e(C+jiOk)IT)] + bko(e(c+ilk)f - 1)}, 0 < t < T (13)

The FP filtered output s(t) is detected by the photodetector which produces a

current of A' I s() 12 Amps. This current plus additive white postdetection thermal noise

current from the amplifier is integrated by the integrator to obtain a decision variable for

the threshold detector.

11

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C. DECISION VARIABLES

The decision variable Y appearing at the integrator output consists of the signal

component X and noise component N

Y=X+N (14)

where

TX=f X ls(t)I 2dt (15)

0T

N=f n(t)dt (16)0

We note that N is a zero mean Gaussian random variable with variance NOT Substituting

(I 0)-(103) into (15) we obtain the signal component X as a function of the two parameters

cT and o)kT, which represent the effect of intersymbol interference and adjacent channel

interference, respectively.

+ dfLT( +ee-T)( ]

X= f ePrboTo +1 -Tk.U

+ W LLTP (I - e'-2cT[ bo, .(ei+l)cT- eicT)]2

2cT / -i=-Lo 1

PT ecr M1•2 .-1 bk. IU'T•'( k=-M/2 1=4z t+j, okT/cT

k*O

(e(cT+jwT11( (+l ) _ +-ot 7) 2

12

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P 2 AT bk.ob.*ocT k=-M12 m,-M12 (1+JwkTlcT)(1-ftouTlcT)

kseO M*O

C T, d ( okT Uc + ec(cT-Ik?')-XmkT--SmT)-lT 1-jwkTIcT

e-(cT+J~1+ -eT

2 PT~e 72 A~ btb*,0k-=_M/2 m=-M 12=-L (1±ftokT/cT)(1-fto .TlcT)

k:*O n,*O

(e(cT+i~okT)l+l) - (CT+JrIokl)I) [..f~C..-e I 1±jco.T/ cT

bo, i(e(l+l )cT - eacT) + -P--e{ ( +e ecT

-2'e-T) bk., (e cT+jwkT)(I+1

k-M12 l=-L 1+I~kTIcTek*eO

-e(CT+iODkT)I) +2 ( - + -2k=--M/2 I~~k~TwTI cTk#O

13

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1-,- PT "76 bo,j(e(i+l)cT2 2 + .jkC)+C-~~~~ ~ - eiW~T c =-L.

--eICT)Re { 2 l bkl (1 -e2CTk=-M/2 I=-L I+jkakT/cT

k*O

(e(cT+jwkTXI+l) - e(cT+jikT) 1)

+ ( bko 2(1---<cTr-wkT)) _ (2cT17)k---MI2 l+jPkTlcT( 1-jwkT/cT - -)1

k*O

D. BIT ERROR PROBABILITY

For a detection threshold a and an ISIACI bit pattern b = (b, bo., ;i=-Lo, ..- 1

= -L, ..., 0; k- -M12, ..., M/2, k;e 0, the conditional bit error probability of the OOK

signal represented by the Gaussian random variable Yin (14)-(16) is given by [Ref 8]

1 = ,--,X b)-a'z 1 , Q-XO(b)('ely kC ) + j =(8

where Q (X) is defined as

Q(x) = J e-'/2dy (19)

and Xo and X are the values of X in (17) for bko = 0 and b0o0 = 1, respectively. The

average bit error probability P. is obtained by taking the expected value of P, (b) in (18)

14

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over all bit patterns b. The minimum bit error probability is obtained by optimizing over

the threshold a. In summary, given a, we calculate the following expectations:

Pe =E {Pe(b)} (20)b

Pe,.mm = minE {P,(b)} =min = p(b)a b a 2M(L+I•-Lo 2patterns

where

2 n 2 x 4 -W 2 ..O V

11 ")M( If... f -X°p(b) = M,0 o o4,MI 2 ... d4MI 2

2x 2xSf (0 4... M2 - - 2... dM/2

(21)

15

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UIL NUMERICAL RESULTS

In this section we present the numerical results for a) bit error probability versus

signal-to-noise ratio Z =,eP T/10 as a function of the normalized channel spacing

(normalized to the bit rate)

I=OT = (Af) T (22)

where Af= o,/2xk is the equal channel spacing in GHz, and b) power penalty versus

normalized channel spacing I as a function of the FP filter parameter cT= (r,//Wp)BT

where B is the filter full width at half maximum bandwidth(FWH-M).

Figures 4-5 show the minimum bit error probability versus signal-to-noise ratio

(Z ) for cT- 5 and 10, respectively, and that of a single channel (SC) operation without

filtering or with filtering but without ISI. In Fig. 4 we observe that a large degradation

occurs due to ISI for cT = 5 which represents a narrowband filter. As the FP filter

bandwidth is made larger as in Fig. 5 with cT = 10, the ISI is reduced but the ACI

increases.

In our model, we are constrained to M =4 for the case under consideration. We set

a FP filter with free spectral range, FWHM Bi21-.6 GHz, FSR = 3800 GHz, fness F

FSR/B = 312.6, and c = 38.4 GHz, 1/T= 2.56 Gb/s, thencT= 15.

16

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IlOe

~10.1 -

10 t 11\1 4 5 1 17 8 19 2

(

L~174

L low

\SC

10 11 12 13 14 15 16 17 is 19 20Z (dB)

Figure 4: Probability of bit error versus signal-to-noise ratio as a fiuntion of normnalized

channel spacing for c2"-5

17

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107

-1 0

1, 4

10

'SC

10 11 12 13 14 15 16 17 18 19 20Z (dM)

Figure 5: Probability of bit error versus signal-to-noise ratio as a function of normalized

channel spacing for c T= 10

18

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(i.e. channel spacing is 12 times the bit rate or 30-4 GHz). In this model the farthest

adajcent channel for M = 4 is twice the channel spacing which is 60. 8 GHz. This verifies

the assumption I f-f, I < FSR/207 = 60.5 GHz, where f. is the FP filter center frequency

This result agrees well with that in [Ref 6; Figs. 6,9, MIF = 0.4, a = 0.2]. Thus we

incorporate the degradation caused by the four nearest adjacent channels. We observe

that for bit rates of I Gb/s or less, our model is valid up to M = 10, and very little

difference is observed between M = 4 and M = 10. Also, we observe that there is little

difference between M = 2 and M = 4 when I > = 10 for bit rates up to 3 Gb/s. In all results

we set Lo = 2 and L = 0,

Figure 6 also shows the power penalty for a dense WDM system relative to a single

channel operation at the minimum bit error probability of 10" . This is the required

additional signal power (dBW) for the dense WDM system to be able to operate at the

10`5 bit error probability achieved in the single channel system with a SNR=12dB. The

dense WDM system is ISf-limited at 2.2 dB, I dB, 0.5 dB, and 0.4 dB in power penalty

for cT = 5, 10, 15, and 20, respectively. It is seen that for a 2.3 dB power penalty, the

normalized channel spacing can be as close as I = 6 (i.e., a channel spacing of six times the

bit rate) for cT = 5. If the power penalty criterion is 1 dB, the normalized channel spacing

is I=12 for cT-= 10, 15, 20. We remark that although the exact transfer functions of the

FP filter is used in [Ref. 6], a number of approximation have been made to obtain

numerical results. The approximations are 1) the ISI is obtained by modeling FP filter as

a single-pole RC filter [Ref 6, Eqs. (4) and (36)], 2) approximating the finite integration

19

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12

x CT-20

10x.

+ CT-15

+

0 o CT=IO

ii

Sx CT=54 " +

4-4

S'' " • .. " 'i ... ... ...,,, ..I ...................... , .............2 -

S '.. . ...-.: . . .... ....... .

Oc I I I I

2 4 6 8 10 12 14 16 18 20I

Figure 6: Power penalty versus normalized channel spacing as a finction of Fabry-Perotfilter parameter cT

20

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with an infinite integration in the calculation ofACI [Ref. 6, Eq. (15)], and 3) the beat

interference is ignored. On the other hand, the ISI and ACI in our investigation are

obtained by modeling the FP filter as a single-pole RC filter, using finite integration and

including the beat interference. Since the results in our investigation and in [Ref 6] agree

well, we conclude that approximations are quite valid. We also note that our resuits also

agree well with the simulation carried out in [Ref. 1, Fig. 17].

The above numerical results shown in Figs. 4-6 are obtained with an optimized

threshold setting. Figure 7 shows the power penalty for fixed threshold a = d'PT/2 which

is the same optimum threshold for single channel operation (midpoint between the

received power for bit zero and bit one). It is seen that the performance of a dense WDM

system is quite sensitive to a for a narrow band filter. An additional 1.8 d3 is observed

for cT = 5 for I > 8, and 0.5 dB for cT = 10 for I > 12. Negligible degradation is observed

forcT= 15, 20 forI> 16.

Figures 8-9 show the power penalty versus normalized channel spacing as a function

of FP filter parameter cT for the worst-case analysis with optimal threshold and fixed

threshold, respectively. The worst-case bit pattern is fixed to produce the minimum X,

and maximum X0 where X, and X0 are the values to X in Appendix-A equation (9) with

b0.0 = I and b0.0 = 0 respectively.

21

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10 I

9- x CT-20

08 + CT-15

7 + 0 CTI0

xS6 " *CT,,5

4 - . .+ x

3-X

x2-+

' o . .o .. ." ... o.... : ..-..-. ....... ............ 0

"0 2 4 6 8 10 12 14 16 18 201

Figure 7: Power penalty versus normalized channel spacing as a function of Fabry-Perotfilter parameter cTwith a fixed threshold a=0.5

22

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12 x x CT=20

+

10- + CT=15

So CT=10

C0". 6- "•cTr--

0

CL-

"

S X.4 -"

"0 .• . " . ~ ~~.................. .. '. . . . . .2 ' .+ x.2 ..............."" " • .. ..

0 -I I I I I II

0 2 4 6 8 10 12 14 16 18 20

Figure 8: Worst-case power penalty versus normalized channel spacing as a function ofFabry-Perot filter parameter cT with optimal threshold oL=(Xo+XI)12

23

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12 Q x CT=20

10- + CT=15

o 8- oCT=10

0 4 - .. . . . . .. . . . . .. . .. . .

"X.

2- o + ...O 0 .. 0 • .. .0 *. .i . .. . . . . . . •...... .. v ..0 . ... .. . . .. .. 0

. . . . . . . . . . . . . . . *X+':.• : ::... . . . . .•

O t I I I- I2 4 6 8 10 12 14 16 18 20

1

Figure 9: Worst-case power penalty versus normalized channel spacing as a function ofFabry-Perot filter parameter cT with fixed threshold ax=0.-5

24

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We observe that the power penalty for the worst-case analysis is only slightly larger

than that of the exact analysis for I > 10 shown in Fig. 6. Similarly the power penalty for

the worst-case analysis with fixed threshold is only slightly larger than that of the exact

analysis with fixed threshold for I > 10 shown is Fig. 7. The reason for this is that for

large channel spacing (I > 10), the ACI effect is small, so the ACI bit pattern has a small

influence on the power penalty.

Figure 10 shows the normalized optimal threshold for the exact analysis shown in

Fig. 6. It is observed that a =0.4 for I > 10. Note that the normalized optimal threshold

for the single channel operation is a = 0.5.

25

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* CT,5

0.9× o CT,1O

0.7 "÷0.8 x CT-20

0.

0.6- 0 ..

1044"*E*.. '.

0.. .. . ... .......... ...... ....

'o5 -+ '0-0 -0 . +0 - ............ ......... 0 ............ 0

0.!• .'° " "° o O -o ...................... o ............ o

10.4

0.3

0.2

0.1,

0 2 4 6 8 10 12 14 16 18 20

Figure 10: The normalized optimal threshold versus normalized channel spacing as afunction of Fabry-Perot filter parameter cT

26

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IV. CONCLUSIONS

We have presented a simple model for the analysis of dense WDM systems

employing an external OOK modulator. The only approximation that we use involves the

modeling of the Fabry-Perot filter by a single-pole RC filter assuming the equivalent

lowpass signal is bandlimited to the frequency range IfI < FSR / 20z. This model

enables us to obtain a closed form expression for the bit error probability which previously

can only be obtained via numerical analysis [Ref 6]. For FP filter with an FSR around

3800 GHz, our model can include the ACI effects of four adjacent channels for bit rates

up to 2.5 Gb/s. Our numerical results show that this model agrees well with that in

[Ref. 6].

27

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"APPENDIX A

DERIVATION OF FORMULA FOR DECISION VARIABLES

DESIRED CHANNEL: CHANNEL 0

ADJACENT CHANNEL. k,k = -M/2,...,-1, 1,...,M2;M: even

BIT IN CHANNEL IN ith TnI lEVAL (iT, Q + 1)7)

bo,•{0,1}, boo DETECTEDBiTIN(0,7)

BIT IN CHANNEL k IIhTIINTERVAL (IT, (I + 1)T)

bk, e { 0, ei*k } WHEREj - 4 • IMAGINARY NUMBLER

a, FREQUENCY SPACING BETWEEN CHANNEL k AND CHANNEL 0,

(ok ---- "•k

4'" PHASE OFFSET BETWEEN CHANNELS k AND CHANNEL 0,

UNIFORMLY DISTRIBUTED BETWEEN (0, 2w)

DATA SIGNAL IN CHANNEL 0

bo(t) = bo,,p(t- iT)-Lo

28

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DATA SIGNAL IN CHANNEL k:

bk(t) = i bkjejlk'pT(t- IT)l=-L

Lo , L: INTEGERSS1, O<t<T

P 2(t) = 0 o, otherwise

pT(t " I, iT<t<4+l)TP O- i 7)= {0 o, otherwise

THE RECEIVED SIGNAL AT THE INPUT OF THE FP FILTER OF

CHANNEL 0 IS:

FPt b ibo (t)+_TFPbktk /2

k*O

P: RECEIVED OPTICAL POWER.

THE OUTPUT OF THE FP FILTER IS

ro(t) = J h(t - )r(-)dr

WHERE h() IS THE EQUIVALENT LOWPASS IMPULSE RESPONSE OF

THE FP FILTER OF CHANNEL 0

ro(t) = f- h(t - r)bo(r)dT + FP h( - r)bk(r)dr

= ibo,o I h(t- r)pT@r)dr

+Fp bo,, ' hQt- t)pT@, - ldi2Lo9

29

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k--M12 I=-L

SINCE THE DETECTION INTERVAL IS 0 <1I< T, WE ONLY NEED TO

EVALUATE 0Q < I0 t) 0< T

sQ)= 1b 0 ,0 h-1)dTr~ b0 , J~ h-,r)dr

0o. iT

S (hlI)T+4 f~{_ bk,i f h(t - r)e'k'CdT]

k M12 1-L IT

+bk,o JhQ - r)eJ~ok~dT)0

0< t <T

=SB(t)+SISI~t)+SACAt)(1

SB(t) DESIRED SIGNAL

Ss~,t): INTERSYMBOL INTERFERENCE

s4cXt): ADJACENT CHANNEL INTERFERENCE

LOWPASS EQUIVALENT TRANSFER FUNCTION

30

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--.p I-A--p i-p I-A-pI-PC = J10 lIa• -P I-*Ll-o()+Jp~md±) I-p

p: POWER REFLECTIVITY

A: POWER ABSORPTION LOSS (A= 0 FOR IDEAL FILTER)

FSR: FREE SPECTRAL RANGE

SINCE f<< FSR (FOR OPERATING FREQUENCY RANGE)

WE CAN APPROXIMATE H(f) AS (ASSUME A= 0):

n( f ) = -P I(l-P)+j•. l+j *--xI-p _- )

H(f ): lWHERE C = FSR(I-p)

FOR FP FILTER WE ALSO HAVE

FSR 7B =l-p

B : FULL WIDTH AT HALF MAXIMUM BANDWIDTH (FWHM) OR HALF

POWER BANDWIDTH

THUSc €-, t >0

h(t) = 0. othewse (2)

DERIVATION OF EO.I ON P. 19

1. SB(t):

31

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0 T 0 T

J~ h- T)P T(r)=O0

00 00

-~ ) TTd hQt - r)P T(T)dT

T

JhQt- )dT =fJh(t -T)dT0 0

3,

Page 40: A simple analytical model for dense WDM/OOK systems Tso-Chuan … · 2016. 7. 4. · Tso-Chuan Chou LCDR, Taiwan Navy B.S, Chinese Naval Academy, November 1983 Submitted in partial

SDB(t) = JP-bo,o I hQt- T)dr 0<t (3)0

SUBSTITUTING (2) INTO (3) WE OBTAIN

SBQt) = fP-bo~o f e"(Td Fb~c-fec'tdr

0 0

TP~~~ 4bo.ocle' T ooeI(ect- 1)

b) BITO0:SB.Ot) = 0O< t< T

2.SS, 1 (t)

pT(r- i7)t < iT

iT (i + )T 01iT (i + )T 0

J~ h- c)p T(r - i)dc=0

33

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iT< t <(i+1I)T t >(i +1)T

iT I (i +1)T 10 iT (i + )T 0

00 0

f hQ - r)PT@:- il)dt f h(t -?)PATt - iT)d'r

(i+1)T

=f h(t-t)dT f J ~ h-tr)driT iT

(i+1)TS,()=r- bo,, f h(t-tr)dt O<t<T (5)

SUBSTITUTING (2) INTO (5) WE OBTAIN

-I (i+1)T

Ssis(t) = vr-- bo,, f ce--cI-Tdt

-1= FP b o, ce -t!ZI(+')

i=-Lo ci

s isi W) = *F-ý bo, e~t(e(i+l)cT - eicT)

34

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sst)= FPe bo,i(e(i+l~cT - eicT) 0 <1t < T (6)

WORST-CASE 151: = ,ib- L = oo

3. s~c(t)

PT(@ -)PATt)

IT (I+ )T 00 T

I=-L i-I1=0

So THIS IS THE COMBINATION OF TIE ABOVE 2 CASES

SACJ(t) = liP { k f_ hQ - -T)eJO~k~dT]k=--MI2 1=L IT

k*0

t+bk,o 5 h(t - T)eJwk~d~r} 0 < t < T (7)

0

35

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SUBSTITUTING (2) INTO (7) WE OBTAIN

S (hlI)T

SACJ(t) =FP~? { bkl i Ice--~t?)ej0)k'tdrk=-M12 l=-L IT

t

+bk,O J Ce--Ct-Te1ktdT}0

M1 2 -1(l+1)T (~( )

k-/M2 l=-L ITk"O

+bk,o ce-cl e e(C +ik) ?dt}0

M1 A2 -1 -,cte~ct(k) g (I+1)T1

k-M12 l=-L C+JOt Ik*O

+bk~oce -ceCJ))

SACJ(t) =F 4ce~' T ' [ -1 bk,,(e(C+i'WkXl+l)T - e(c+icwkyT)Jk=-M12 C+J(O k 1=-L

ko0

+bk,o(e (C+J(Ok) -1) 0 < t < T()

WORSE-CASE A :I bkl bk,0 b,L L

36

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ACI k-=-M12 c(1+j4c)k*O

AL1M2 emJ-t

k*O

OUTPUT OF PHOTODETECTOR: 4' I.S(t) 1

T

SIGNAL OUTPUT OF INTEGRATOR: X I' ISQt)j 2dt0

Is(t)12 = ISBWt + SjSQt) + SAC! (t)I12

IsB(t)I' + Iss(t)I 2+ISACI(t)12 + 2Re IsB(t)sIS1 (t)}

+2Ref{s*(t)SACI(t) }+ 2Re {s S~(t)sAcJ(t) }

ISBW)12 = Pb 2,0(1 - e -t2= Pb 2,0(1 - 2e-ct + e-2') 0 < t < T

T T T

fISB(t)I dt = ~~ 0 'o- 2Pbo,0 f e~'dt + Pbo,0 I5-d0 0 0

37

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= PTb:,0 - 2Pbo,0 c e' 0 + Pb 0,oce~ I

= PTbo,o + ~eT12cT)

T 2Tc -c

-~~C#e 2cT~ )Pb e

k=M2 2~= k*0 -7TI-ecT -c)

2) sc (t FPb-e' 0 < 38

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Isj,,,)I2=Plb 12 Af Af0<t<Tk*O h*O

TI.,swAt)I 2dt=P1b2 'f f~ eJ-kWh)tdt0 k=--M I2 h=-M IZ (1+j-~ X --- o

k*O 11*0

=P~bV1A2 AV/2

12 0 1*T

k=--M12 h=--MI2 ck*O 11*0

-~M p2A2 Af2

T o 7' roko

THEN ~~7 !k(~~~)'t {0,0kT_

= s P71t)I A=P IbI2 A0T /-M2 - 2 39 jc-XI-l"-(e c

Page 47: A simple analytical model for dense WDM/OOK systems Tso-Chuan … · 2016. 7. 4. · Tso-Chuan Chou LCDR, Taiwan Navy B.S, Chinese Naval Academy, November 1983 Submitted in partial

4) 2Resat S BWS,(t)} 2Re IF ~fb 0 0( 1 - e-ct)F/ b-e-' I

J2Re(SB(t)ssj (t)}dt =2Pbo,ob-t { 0 - 1

= 2c

_PTboob-( -2eT e 2cT)

5) 2Re{4;(t)SACJ(t) = 2Re{ f~bo,o)(1-ec)~ !Lk-- M12 (akk*0

=2Pbo,oRe Ib eoe--Jk~k=--M12 i-I-

k-*O

f 2Rels*(t)SAC,(t)}Idt =2Pbo,oRelb _

0 k---M12 l+jLL-

T 0

(0 k I [NTEGER>O

40

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JeJOtdt ±(elOkI 1)0

j e-l`:OkTtjt_ I -j ~t~JkT Ij

0 -(C-J; k) c -

f 2Re{4*(t)sAci(t)} dt =2Pb o,oRe (b ,, c-~-4~

2F~ho~oRe(b) e-c)

- CT (1(Ik))k*0

6) 2Ref Sl~(t)sACI(t)} )=2Re(J.Yb-e-'.1Pb 2: sko

=2Pb-Reb I~ bFk=M2I+j-'-

k*O

S2Re~s*,(t)SACI(t)}= 2Pb-Rec b}o k---M12 (1-j- -I jc-

k=-M12&0O

41

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5Lq~hdR FWOMT-CASE ANALYSIS

0) Lzd I- NTEGER>O0

T

X=, 4f JisQt)l 2d0

-4 PTb', 0 [I -3-L - e--T) + jTT<1 -e~TJ+1 L( e-2T)

+PllbI12 f PTbo~ob i- 2 ecT+e-2CT)k---M/2 1jt')2

k*O

2P~bo~oRefbI 1e-cT) I- ~k---MI2 c)

k*O

P.h..Re(b)(~T) ~ L

cT k_-My k2

+b2[-L - e-2T)] + bo.ob-[3<1I 2-T + e-2cT)]

+[1b 12 + _LI ~e-T)Re (b) (b- -bo,o)1

42

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wHERE b e (0, eh) sRe Ib) e 0, cos*,b1 0, O1}

EXACT ANALYSI

uf sat) dt= ~b[ 0 I - -LIe-T + -T(10

2) sim~t) = JPe bo,,(e(II)tcT - e~cT) 0 < t < Ti=-Lo

Iss(t)12 = pe bo,1(e(i+lWcT - elTj 0 < t < T

T -

MI~ j lsj)2d,= Xj(I ~e-2 T)[_i bo,i(e(i+U'~iT]

kM12 c1-J

k:*O

-(c + bk.o(e(I±~' - 1)) 0 < t < T

43

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SAC~t) = .f-e-c' +16k bk~(+

k*OO

SACIQt)I2=peI -2c, b~ -b (e~ 1+j-*Xl(+I)cT I e(+jA)IcTI2k=-M121---L I+j~c

ksO

A~2 A~2 bk.0b* 0 (Pk

+2Pe f~ !k 440 .bkjb, 0 - -(e-Jm -I4JxI cf)~k--MI2 m=--M1 0 =- (lj c X-jc

k*O m*O

bkjb

TEVALUATE fIS~ct)I12dt:

0

a) T Isc 2tIdt PT I( -e- c T )I T120 AMII tT k=-M~2 I=-L I +j4t

(e (I I+jt-i~lT - k

44

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SPECIAL CASE.- W1k = 2xkI 1J INTEGER > 0

-PT 1 e -c) I 'f2 bkl Z((I+l)cT -e'cT)1 2

2cT' =1 l=_L l~jP7%"ks0

b) 1 O IA,) 2dtO jeimk-m)d0 k=--M/ F/M2 (I~lc-x)l-j-oC-) 0

k*O moo

T T T

-1 e-ý`Jrkydt-f e-(c+i-)tdt+f e-2'dt}0 0 0

Sbk.ob,,o T, 64=0).

k=--M12 m=--M12 (1+j+)(1-Al-)j/e-e)

e -(p Jk)T -1 e -<pm -)T -I 1 2c )C-jCD k C+JO.

__~ Ak2 b~ ______ cT Ci~k=CO

-cT ~M~iM2(I+jlkXl-j) ~½--~k*iO m*O4 a

+ _ e-(14 1 + ~ 2cT)}

SPECIAL CASE: 0) k = 2WkI 1= INTEGER> 0T

(JmT

45

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T IT, Wkk=m eTk=W

fc 0

eJOwkT = e J~kT-1

Wbklot. 1 7Z A2 bkob*.

-PT{ k-M1 (=M/ + 1. cT

k*O kCO w M*O c r

C) I SAC]~)d =2PRe I Af2 A0 ~k=--M2 m=M2 1-L I1+jlX1-j) I-m)

ksO M*O

-e(l+ij)IcT)[J e-(1+ij)tdt-f e-2cdt] }0 0

2= Re{_I

k*O n,*O

(e (I+lc-XI+l)c~T e c Iie)IcT)( )]

SPECIAL CASE. (Ok Ti I INTEGER> 0

46

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btjb2 7-Q -I )c IcT ~r

Off Re( T L 2ý -,,(,(IeI''cT k--Ml2nt~i,-2 1=L (+~X

k*O m*O

T t =2d LcT Ie-2cT) l lk- ~L(1+jtk)l+)cTf ISAC1 2Yj~ _eM21- 14j-r0 kso

-e(1+jc)ICT)12 +la 0~ Af2 ko0-e . Tk=-MI2m=-M/2 (1+j c X1-Ajl)

ko0 moo

cT =o, wi c tIJ!-WTr-Ok G~ o) I+ w

I j c +(10 e cT)

+2PT L 2 Af2 -m.

+2jRe{2jZ~Zk*O m$O

47

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T 1A2A.d.&I(- e 2cT)I _Ajl (e11c __e__)JISACIK ,A- ''_ 11-

A.:T + ± A1 2 1=-L bk+oba

0~ k*0 m*0

+2PRe T~ If2 -3b.,ý e()t

ksO m*Os *Oc

T -I

= 2Pbo~ J-e c boeI+I - e-cT)]J(~ ~td

00

T (i~l cT e CT)48

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f 2Re({SBQt)S;~sJQ) } dt0

= 2bo0 ~bo,((i+l)cT - eicT)[!lI T e-2 T3~

2P~bo,o -i ,( Ti0=2i=-Lo22

2PT o~o - I i+ )cT - cT)(1 -7tT -

- 1T =ec - 2oi e(' T) -e -oe(I+ l e 2

-2 PJhe{[,/ho o(1 -e')]T iT( e-c-2-T

fPebo' -2cT (.Le1 irX+l)cT -ei

(I+e-M12,I-LT I~h ebl~ieT)

0~

2 -MRe FP A bo( -eJO)]fe']d0~

49k1(~~jkX~~T jIy

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- 2 fJRe{Pbo,o(1 -e-c')e'0

-12 bk(1 +j4)Q+1)CT -~t e(IA.)CT) + Pb0 ,0kM12 =-L I+

bkO

k=M2 I+J7ck*O

= 2Pbo,oRe{_t k (e('iX+ -eT -

k/M21=-L l+J-'-k*O

T 2t:Af2 bk~oe -cl --c~t

f (ei'"t -' c - e - + e-2c)dt}0

-2cT ~ k -1T b k,~~kllc

= 2Pb X~~ (e(I +iý - e W22k---M121=-L 1+J7c

k*0

IjokIC M1 bko ewTl -r I~~ ecT- I -<lJ- XTI

-e1/ T+j+ JOk + C2c + (1-j-c _)C

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_P~bo o 2c2 -c k1 (~t),Ic-- ;;-Re +{ (1 +cT2ecT e=M21- c

k*O

(L2 bkýo e~*kT 1_ -k=-M12 I+

k*O

I-h-

SPECIAL CASE: (0 1=xk FIXED INTEGER >0T

Tf ej 0"'ldt -1 (eiOkT _ 1) =0

0 J(Ok

THAEN

J2Re {s*(t)SACJ(t) }dt0

-P Tbo.O o 1 + 2 cT -k~ 2e+T1Ac2

"(I-jR)lcT+ 0~ + ~ e-T - _ecT 12 Ti,-e cT

(e(e1

-eM1 'cJc 22l 2 jLO

k*O

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6) f 2Re {Sj*S(t)SACl(t) }dt0

-2Re f [4Te"` ý 4 bo,,i(e(il -Te'cT)1

[.f~eý bk2 -I~4((+jt4 )(I+1)cT e(I+jtk)IcT)

ITM21- e It(e(-k*0

k---M/2 I+J ck*0

2PRe{ /2 - .,, bok(e(i+l)cT - e'cT)k---M12 I=-L i=-Lo +j -c-

k*0

6t1+.-k(+1 (I+j-k)lC T\rz d M/2 -1 bo,,bko--el~lcT ec ) j e-2t+0 k---M12 i=-Lo l+Ji -

(e(i+l)cT - e icT) fJ (e-(1 -m)ct - ecdt0

-2PRe{ 1:2: bob2:,ilc _ icT)k---M12 1=-L i=-Lo 1 A--

k*0

(e(I+~l+ 1)cTe 0+j 4) lcT)-1(1 ~e 2 cT)

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+ ~ bo.bk~o(i+l)cT iecT)[ I -I-4j-J-k)cT I.(~T 1J

k--- cTL, k=-M12 l=Lc jk*Oe

(I~j L Xj+ )cT c2 bko 2 (1lI('J ck)CT)

(e ce(I+P~k)IcT)+ i-jk +e- 2cT~1)

2icklSPECIAL CASE: (Ok = T I= MNEGER.>O0

J2Rel{S;S(t)SAcJ(t)dt0

_PT bi(e(i+l)cT eiT)Re{_j bk,_~(1 -e2cT)

-cT i- k-M12 =-L l+JL--k*O c

(e~ljL'-)(+I~T I~l!,)I Aj2 bk~o[(2-.2e e -- 2IT t ,,') +e- 2 cT 1

w~e(1+jt"-I+1)c~T - (C+irx k )I+ I)T - (CT+i(OkTX+I)

-ecT(I+1)eftiokT(l+1) =-cx''

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sBMILARLY=* e(l+i-r)IcT = -(t~Y ecIT

=:>j 2Re({sI*S,(t)SACJQt) }dt0

PT ý bo,i(e(1+I)cT - ecT)Re{ f/2 bk7T i=Lk--M12 l=-L Itj~lý

0 ~k*O c

(1-e-2cT)(ecT(I+1) - ecTI)+__2 ko 22ec) -2T 1 }/--j2 I tj~ ;T -j-;x.

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APPENDIX B

MATLAB COMPUTER PROGRAMS

exact analysis with optimal threshold signal out of the integrator, the signal X contains desiredsignal and ACI & ISI and postdetect noise ,The formula for the BER is:

S 12 p(b)2M(L+I)$LO 2Mpanern

where p(b) = .() O A ,) d0-MI2 ...dOMr2

2x2*f ( .""OTZ)' )d4-Ma ...dDM/2 }

M is number of adjacent channels. Since we assume upper and lower channels are synchronizedindividually, i.e. for our model the power of(l/2x) is fixed to 2, also we only have twointegrations and two arguments.

M=4; k=[-M/2:-I I:M/2];m--k,% produce the controlled matrix b to control 64 different bit patternsml=[ zeros(l,32) ones(l,32) ];m2=[ zeros(l,16) ones(l,16) zeros(l,16) ones(l,16)];m3=[];

for i=1:4m3=[m3 [zeros(l,S) ones(1,8)));

endm4-[];

for i=l -8m4=[m4 [zeros(1,4) ones(l,4)]];

endm5=zeros(1,64);m6=[];for i= 1:16

m6n[m6 [zeros(1,2) ones(1,2)]];end

m7=[),for i=1:32

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m7in[m7 zeros(l, 1) ones(l, 1)];

end

b-[m 1,,n2;m3;m4;mS;m6;m7)];

% signal to noise ratio range in dBRPTNDB=[1OO.5:25]; O/.RPTN-dBppp IO N.ýO. 1 *RPTNDB);lenlI=Iength(ppp);

% solaiph fimction is provided by Professor Randy L. Borchardt

n=10;[bpx~wfxl-grule(n), 6'/obpx~bpy ,w&i=wfy

% single channelBERO0. 5*erfc(Ppp/8A0.S);

pp=[]; thresh=[]; */thresh is not normalized threshold

for CT=[5 10 15 20] % cT is Fabry-Perot filter parameterif CT==5

qqq{(2:12 17 20];elseif CT=10

qqq=[3:12 17 20];elseif CTlS1

qqq=[4:12 17 20];-elseif CT-20

qqc=[5:12 17 20];end

pe=[J, thresh 1=[];

for I=qqqBER=[]; thresh2=[];

for RPTN~pppap=linspace(0, 182,11); /.approximated thresholdsx3=0; % first few loops to find out the threshold which make the

% BER minimun dont care about the scalefor i=1:64 x3-x3+...

solaph(xx00,0,2*pi,2,bpx,wfx,0,2*pi,2,bpx,wfx,ap,b,CT,iI,k,m,RPTN)+...solalph(W 'xII,0,2*pi,2,bpxwfx,0,2*pi,2,bpx~wecap,b,CT,L,~knmRPTN);

end[val,ind]-mn~x3);

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lef..ap(ind)-16.6,

if lef<O ,lef-; end % to aviod the threshold go beyond the negative side

ap=linspacele~ap(ind)+l6.6,1 1);% two more time to find alpha

x3=0;

for i=1:64 x3=x3+...so~aph('xxOO',O,2*pi,2,bpx,wflc,O,2*pi2,bpx,wflC,ap,bCT,iI,k,IU,RPTN)+..solaiph(xxll ,O,2*pi,2,bpx~wfxcO,2*pi,2,bpx~wfxcap~b,CT,i,I,knmRPTN),

end

[val,ind]-min(x3);lef--ap~ind)-3. 1,

if lef<O ,lefO; end

ap=linspace(lef,ap(ind)+3. 1,11);%three more time to find alpha

xc30,

for i1:64x3-x3+..

solaph(xxOO,O,2*pi,2,bpx,wflc,O,2*pi,2,bpx,wfx,ap,b,CT,i,I,k,n',RPTN)+..solalph('xxll ',O,2*pi,2,bpx~wfx,O,2*'pi,2,bpx~wftxap~bCT,i,l,k,IflRPTN);

end

[val,indj=min(x3),

if lef<O ,Ief=O; end

ap=Iinspace~lef~ap(ind)+O. 57,8);% four more time to find alpha

x30-;

for i=1: 64x3=x3+...solalph('xxOWt,,2*pi,2,bpx,wfx,O,2*pi,2,bpx,wflC,ap,b,CT,i,I,k~nl,RPTN)+..

soph('xxcl .O02*p,2,bpxwfx,O2*pi,2bpx~wftxap,b,CT,i,I,kI.RPTN);end

[vai,ind]=rniin(x3);

ap=ap(ind);

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% after find optmal alpha use double integrationqq3=0;

for i-1: 64qq3=qq3+( dbgquadm(ýocO,O,2*pi,2,bpx~wfic,O,2*pi2,...

bpx,wfx,ap,b,CT~i,I,k~mRPTN4)+...dbgquadn('xxl I ',O,2*p0,,bpx~wfx,O,2*pi,2,...bpx,wfic,ap,b,CT,i,IlkmRPTN) /( 1024*piA2);

end

BER=[BER qq3J; thresh2j[thresh2 ap];

if qq3< I O(-15) %for save timec only interesting in IOA'(-l5)ufl-fnd(ppp-RPTN);

BER(ii+l :lerl)-5* 1OA(-lI 16)*ones( l,length(ii+l:leni))thresh2(ii+1lclnl)=(ap+2)*ones(I,length(ii+l:lenl))break

endend

pe[pe;BERJ; threshl=[threshl ;thresh2];end

pp=[pp;pe], thresh--[tbresh~thresh 1],end

time2--toc,-

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% worse case form appendix setting optimal threshold equal (xO-sx 1)/2M-41=linspace(0,6. 10 1), % set I value in linspceinteger to find minimum IRPTNDB 0:2.2:0, % x-axis dB rangeRPTN=10 "(0. I *RPTNJ)B); % change to ratio% single channelBERO=0O. 5 *erfc(RPTN/SAO. 5);%find optimal alphapp=01

for CThIIS 10 15 20]x3=0-for k=1:0.5*M

x3-x3+2./( 1+(2*pi*k*L/CT).A2);end

x0=( I exp(-2*CT))I(2*CT)+x3*(1I+2*( I-exp(-CT))ICT)-;xl =1-2 *( I-exp(-CT))/CT+( I-exp(-2 *CT))/(2*CT);[val..ind]-min(abs(xO-xl ));I~ceil(I(ind)),1=(I(ind)); % our minimum I value

% set different I and to find the BERss=I+l:1+10;BER4[];

for I=ssx3=0;

for k=1: 0. 5*Mx3=x3+2/( I+(2*pi*k*I/CT)A 2);

endx0=( I exp(-2*CT))/(2*CT)+x3 *(1I+2*( I-exp(-CT))/CT);xl=1-2 *( I-exp(-CT))/CT+( I exp(-2*CT))/(2*CT);BER([BER;0. 5 *erfc( RPTN*(x I -xO)/8A0. 5)]

endpp=[pp;BER];

end

seniilogy(RPTNDB,BERO.'-',RPTNDB,pp(::))

axis([ 10 19 10'(- 15) 1]

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LIST OF REFERENCES

[1] C.S. Li, F.F. Tong, K. Liu, andD.G Messerscmitt, "Channelcapacityoptimization of chirp-limited dense WDM/WDMA systems using OOK/FSKmodulation and optical fibers," Journal Lightwave Technol., Vol. 10, No. 8,pp. 1148-1161, Aug. 1992.

[2] PA. Humblet and W.M. Hamdy, "Crosstalk analysis and filteroptimization for single-and double-cavity Fabry-Perot filtersm" IEEE journalSelect. Area Commun., Vol. 8, No. 6, Aug. 1990.

[3] C.A. Brachkett, "Dense wavelength division multiplexing: Principles andapplications," IEEE Journal Select Area Commun., Vol. 8, pp. 948-964,1990.

[4] I.P. Kaminow, "FSK with direct detection in optical multiple access FDMnetworks," IEEE Journal Select. Area Commun., Vol. 8, pp. 1005-1114,1990.

[5] L.J. Cimini and G.J. Foschini, "Can multilevel signaling improve thespectral efficiency of ASK optical FDM systems?," IEEE Trans. Commun.,Vol. 41, No. 7, 1084-1090, July 1993.

[6] W.M. Hamdy and P.A. Humblet, "Sensitivity analysis of direct detectionoptical FDMA networks with OOK modulation," Journal Lightwave Technol.,Vol. 11, pp. 783-794, May/June 1993.

[7] P.E. Green, Jr., Fiber Optic Networks, Englewood Cliffs, New Jersey:Prenticeh-Hall, 1993.

[8] L.W. Cough, Ill, Digital and Analog Communication Systems, 4th Ed., NewYork. McMillan, 1993.

[9] J.G. Proakis, Digital Communications, 2nd Ed., New York: McGraw-Hill,1989.

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[101 I.P. Kaminow, P.P. lannone, J. Stone, and LW. Stulz, "FDMA-FSKstar network with a tunable optical filter demultiplexer," Journal LightwaveTechnol., Vol. 6, No. 9, pp. 1406-1414, 1988.

[l1] J.P. Powers, An Introduction to Fiber Optics Systems, Aksen Associate,Inc., Publishers, 1993.

[12] G.K. Keiser, Optical Fiber Communications, 2nd Ed., New YorkMaGraw-Hill, 1991.

[13] G. P. Agrawal, Fiber-Optic Communications Systems, New York WileyInter-Science, 1992.

[14] A.E Willner, "Simplified model of an FSK-to-ASK direct-detection systemusing a Fabry-Perot demodulator," IEEE Photon. Technol. Lett., Vol. 2,No. 5, pp. 363-366, May 1990.

[15] A.E. Willner, "SNR analysis of crosstalk and filtering effects in anamplified multichannel direct-detection dense-WDM system," IEEE Ph'-on.Technol. Lett., Vol. 4, No. 2, pp. 186-189, Feb. 1992.

[16] P.E. Green and R. Ramaswazni, "Direct detection lightwave systems ý Whypay more?," IEEE LCSMag., Vol. 1, pp. 50-56, 1990.

[17] A.A.M. Saleh and J. Stone, "Two-stage Fabry-Perot filters a demultiplexers inoptical FDMA LANs," Journal Lightwave Technol., Vol. 7, pp. 323-330,1989.

[18] P.A. Humblet and W.M. Hamdy, "Crosstalk analysis and filter optimization ofsingle-and double-stage Fabry-Perot filters," Journal Select. Areas Commun.,

Vol. 9, No. 8, pp. 1095-1107, 1990.

[19] P.A. Rosher and A.R. Hunwicks, "The analysis of crosstalk in multichannelwavelength division multiplexed optical transmission systems and it- impact onmultiplexer design," IEEE Journal Select. Areas Commun. Vol. 9, pp.1108-1115, 1990.

[20] W.M. Hamdy, "Crosstalk in optical direct detection optical FDMAnetworks," Ph.D. Thesis, Massachusetts Institute of Technology, 1991.LIDS-TH-2053.

[21] James L. Buchanan and Peter R. Turner, Numerical Methods and Analysispp. 473-477, 1992.

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EqrrlAL DISTRIBUTION LIST

1. Defense Technical Information Center 2Cameron StationAlexandria, VA 22304-6145

2. Library, Code 52 2Naval Postgraduate SchoolMonterey, CA 93943-5 101

3 Department Chairman, Code ECDepartment of Electrical and Computer EngineerNaval Postgraduate SchoolMonterey, CA 93943-5121

4. Tri T. Ha, Code EC/Ha 3Department of Electrical and Computer EngineerNaval Postgraduate SchoolMonterey, CA 93943-5121

5. Randy L. Borchardt, Code EC/Bt 2Department of Electrical and Computer EngineerNaval Postgraduate SchoolMonterey, CA 93943-5121

6. Chou, Tso-Chuan 5LCDR, Taiwan NavyIF #13 Lane 161 Chung-Hua Ist RD. Ku-Shan Dist.Kaohsiung, Taiwan, R. 0. C.

62