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Optical fiber communication solution manual

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Optical fiber communication solution manual

1 Problem Solutions for Chapter 2 2-1. E = 100cos 2 π 10 8 t + 30 ° ( ) e x + 20cos 2 π 10 8 t − 50 ° ( ) e y + 40cos 2 π 10 8 t + 210 ° ( ) e z 2-2. The general form is: y = (amplitude) cos(ωt - kz) = A cos [2π(νt - z/λ)]. Therefore (a) amplitude = 8 µm (b) wavelength: 1/λ = 0.8 µm -1 so that λ = 1.25 µm (c) ω = 2πν = 2π(2) = 4π (d) At t = 0 and z = 4 µm we have y = 8 cos [2π(-0.8 µm -1 )(4 µm)] = 8 cos [2π(-3.2)] = 2.472 2-3. For E in electron volts and λ in µm we have E = 1 .240 λ (a) At 0.82 µm, E = 1.240/0.82 = 1.512 eV At 1.32 µm, E = 1.240/1.32 = 0.939 eV At 1.55 µm, E = 1.240/1.55 = 0.800 eV (b) At 0.82 µm, k = 2π/λ = 7.662 µm -1 At 1.32 µm, k = 2π/λ = 4.760 µm -1 At 1.55 µm, k = 2π/λ = 4.054 µm -1 2-4. x 1 = a 1 cos (ωt - δ 1 ) and x 2 = a 2 cos (ωt - δ 2 ) Adding x 1 and x 2 yields x 1 + x 2 = a 1 [cos ωt cos δ 1 + sin ωt sin δ 1 ] + a 2 [cos ωt cos δ 2 + sin ωt sin δ 2 ] = [a 1 cos δ 1 + a 2 cos δ 2 ] cos ωt + [a 1 sin δ 1 + a 2 sin δ 2 ] sin ωt Since the a's and the δ's are constants, we can set a 1 cos δ 1 + a 2 cos δ 2 = A cos φ (1) 2 a 1 sin δ 1 + a 2 sin δ 2 = A sin φ (2) provided that constant values of A and φ exist which satisfy these equations. To verify this, first square both sides and add: A 2 (sin 2 φ + cos 2 φ) = a 1 2 sin 2 δ 1 + cos 2 δ 1 ( ) + a 2 2 sin 2 δ 2 + cos 2 δ 2 ( ) + 2a 1 a 2 (sin δ 1 sin δ 2 + cos δ 1 cos δ 2 ) or A 2 = a 1 2 + a 2 2 + 2a 1 a 2 cos (δ 1 - δ 2 ) Dividing (2) by (1) gives tan φ = a 1 sin δ 1 + a 2 sin δ 2 a 1 cosδ 1 + a 2 cosδ 2 Thus we can write x = x 1 + x 2 = A cos φ cos ωt + A sin φ sin ωt = A cos(ωt - φ) 2-5. First expand Eq. (2-3) as E y E 0 y = cos (ωt - kz) cos δ - sin (ωt - kz) sin δ (2.5-1) Subtract from this the expression E x E 0 x cos δ = cos (ωt - kz) cos δ to yield E y E 0 y - E x E 0x cos δ = - sin (ωt - kz) sin δ (2.5-2) Using the relation cos 2 α + sin 2 α = 1, we use Eq. (2-2) to write 3 sin 2 (ωt - kz) = [1 - cos 2 (ωt - kz)] = 1 − E x E 0x       2       (2.5-3) Squaring both sides of Eq. (2.5-2) and substituting it into Eq. (2.5-3) yields E y E 0 y − E x E 0x cos δ       2 = 1 − E x E 0x       2       sin 2 δ Expanding the left-hand side and rearranging terms yields E x E 0x       2 + E y E 0y       2 - 2 E x E 0x       E y E 0y       cos δ = sin 2 δ 2-6. Plot of Eq. (2-7). 2-7. Linearly polarized wave. 2-8. 33 ° 33 ° 90 ° Glass Air: n = 1.0 (a) Apply Snell's law n 1 cos θ 1 = n 2 cos θ 2 where n 1 = 1, θ 1 = 33°, and θ 2 = 90° - 33° = 57° ∴ n 2 = cos 33 ° cos 57 ° = 1.540 (b) The critical angle is found from n glass sin φ glass = n air sin φ air 4 with φ air = 90° and n air = 1.0 ∴ φ critical = arcsin 1 n glass = arcsin 1 1 .540 = 40.5° 2-9 Air Water 12 cm r θ Find θ c from Snell's law n 1 sin θ 1 = n 2 sin θ c = 1 When n 2 = 1.33, then θ c = 48.75° Find r from tan θ c = r 12 cm , which yields r = 13.7 cm. 2-10. 45 ° Using Snell's law n glass sin θ c = n alcohol sin 90° where θ c = 45° we have n glass = 1 . 45 sin 45 ° = 2.05 2-11. (a) Use either NA = n 1 2 − n 2 2 ( ) 1 / 2 = 0.242 or 5 NA ≈ n 1 2 ∆ = n 1 2(n 1 − n 2 ) n 1 = 0.243 (b) θ 0,max = arcsin (NA/n) = arcsin 0 . 242 1.0     = 14° 2-13. NA = n 1 2 − n 2 2 ( ) 1 / 2 = n 1 2 − n 1 2 (1 − ∆ ) 2 [ ] 1 / 2 = n 1 2 ∆ − ∆ 2 ( ) 1 / 2 Since ∆ << 1, ∆ 2 << ∆; ∴ NA ≈ n 1 2 ∆ 2-14. (a) Solve Eq. (2-34a) for jH φ : jH φ = j εω β E r - 1 β r ∂ H z ∂φ Substituting into Eq. (2-33b) we have j β E r + ∂ E z ∂ r = ωµ j εω β E r − 1 β r ∂ H z ∂φ       Solve for E r and let q 2 = ω 2 εµ - β 2 to obtain Eq. (2-35a). (b) Solve Eq. (2-34b) for jH r : jH r = -j εω β E φ - 1 β ∂ H z ∂r Substituting into Eq. (2-33a) we have j β E φ + 1 r ∂ E z ∂φ = -ωµ −j εω β E φ − 1 β ∂ H z ∂ r       Solve for E φ and let q 2 = ω 2 εµ - β 2 to obtain Eq. (2-35b). (c) Solve Eq. (2-34a) for jE r : 6 jE r = 1 εω 1 r ∂ H z ∂φ + jr β H φ      Substituting into Eq. (2-33b) we have β εω 1 r ∂ H z ∂φ + jr β H φ      + ∂ E z ∂ r = jωµ H φ Solve for H φ and let q 2 = ω 2 εµ - β 2 to obtain Eq. (2-35d). (d) Solve Eq. (2-34b) for jE φ jE φ = - 1 εω j β H r + ∂ H z ∂ r     Substituting into Eq. (2-33a) we have 1 r ∂ E z ∂φ - β εω j β H r + ∂ H z ∂ r     = -jωµ H r Solve for H r to obtain Eq. (2-35c). (e) Substitute Eqs. (2-35c) and (2-35d) into Eq. (2-34c) - j q 2 1 r ∂ ∂ r β ∂ H z ∂φ + εω r ∂ E z ∂ r      − ∂ ∂φ β ∂ H z ∂ r − εω r ∂ E z ∂φ            = jεωE z Upon differentiating and multiplying by jq 2 /εω we obtain Eq. (2-36). (f) Substitute Eqs. (2-35a) and (2-35b) into Eq. (2-33c) - j q 2 1 r ∂ ∂ r β ∂ E z ∂φ − µω r ∂ H z ∂ r      − ∂ ∂φ β ∂ E z ∂ r + µω r ∂ H z ∂φ            = -jµωH z Upon differentiating and multiplying by jq 2 /εω we obtain Eq. (2-37). 2-15. For ν = 0, from Eqs. (2-42) and (2-43) we have 7 E z = AJ 0 (ur) e j( ω t − β z) and H z = BJ 0 (ur) e j( ω t − β z) We want to find the coefficients A and B. From Eqs. (2-47) and (2-51), respectively, we have C = J ν ( ua ) K ν (wa) A and D = J ν ( ua ) K ν (wa) B Substitute these into Eq. (2-50) to find B in terms of A: A j βν a     1 u 2 + 1 w 2     = Bωµ J' ν (ua) uJ ν (ua) + K' ν (wa) wK ν (wa)       For ν = 0, the right-hand side must be zero. Also for ν = 0, either Eq. (2-55a) or (2-56a) holds. Suppose Eq. (2-56a) holds, so that the term in square brackets on the right-hand side in the above equation is not zero. Then we must have that B = 0, which from Eq. (2- 43) means that H z = 0. Thus Eq. (2-56) corresponds to TM 0m modes. For the other case, substitute Eqs. (2-47) and (2-51) into Eq. (2-52): 0 = 1 u 2 B j βν a J ν (ua) + A ωε 1 uJ' ν (ua)     + 1 w 2 B j βν a J ν (ua) + A ωε 2 w K' ν (wa)J ν (ua) K ν (wa)       With k 1 2 = ω 2 µε 1 and k 2 2 = ω 2 µε 2 rewrite this as Bν = ja βωµ 1 1 u 2 + 1 w 2         k 1 2 J ν + k 2 2 K ν [ ] A 8 where J ν and K ν are defined in Eq. (2-54). If for ν = 0 the term in square brackets on the right-hand side is non-zero, that is, if Eq. (2-56a) does not hold, then we must have that A = 0, which from Eq. (2-42) means that E z = 0. Thus Eq. (2-55) corresponds to TE 0m modes. 2-16. From Eq. (2-23) we have ∆ = n 1 2 − n 2 2 2n 1 2 = 1 2 1 − n 2 2 n 1 2       ∆ << 1 implies n 1 ≈ n 2 Thus using Eq. (2-46), which states that n 2 k = k 2 ≤ β ≤ k 1 = n 1 k, we have n 2 2 k 2 = k 2 2 ≈ n 1 2 k 2 = k 1 2 ≈ β 2 2-17. 2-18. (a) From Eqs. (2-59) and (2-61) we have M ≈ 2 π 2 a 2 λ 2 n 1 2 − n 2 2 ( ) = 2 π 2 a 2 λ 2 NA ( ) 2 a = M 2 π     1 / 2 λ NA = 1000 2     1 / 2 0.85 µ m 0.2 π = 30.25 µ m Therefore, D = 2a =60.5 µm (b) M = 2 π 2 30.25 µ m ( ) 2 1.32 µ m ( ) 2 0.2 ( ) 2 = 414 (c) At 1550 nm, M = 300 2-19. From Eq. (2-58), 9 V = 2 π ( 25 µ m ) 0.82 µm (1.48) 2 − (1.46) 2 [ ] 1/ 2 = 46.5 Using Eq. (2-61) M ≈ V 2 /2 =1081 at 820 nm. Similarly, M = 417 at 1320 nm and M = 303 at 1550 nm. From Eq. (2-72) P clad P     total ≈ 4 3 M -1/2 = 4 × 100 % 3 1080 = 4.1% at 820 nm. Similarly, (P clad /P) total = 6.6% at 1320 nm and 7.8% at 1550 nm. 2-20 (a) At 1320 nm we have from Eqs. (2-23) and (2-57) that V = 25 and M = 312. (b) From Eq. (2-72) the power flow in the cladding is 7.5%. 2-21. (a) For single-mode operation, we need V ≤ 2.40. Solving Eq. (2-58) for the core radius a a = V λ 2 π n 1 2 − n 2 2 ( ) − 1/ 2 = 2 . 40 ( 1 . 32 µ m ) 2 π (1.480) 2 − (1.478) 2 [ ] 1/ 2 = 6.55 µm (b) From Eq. (2-23) NA = n 1 2 − n 2 2 ( ) 1 / 2 = (1.480) 2 − (1.478) 2 [ ] 1 / 2 = 0.077 (c) From Eq. (2-23), NA = n sin θ 0,max . When n = 1.0 then θ 0,max = arcsin NA n     = arcsin 0.077 1 . 0     = 4.4° 2-22. n 2 = n 1 2 − NA 2 = (1.458) 2 − (0.3) 2 = 1.427 a = λ V 2 π NA = ( 1 . 30 )( 75 ) 2 π (0.3) = 52 µm 10 2-23. For small values of ∆ we can write V ≈ 2 π a λ n 1 2 ∆ For a = 5 µm we have ∆ ≈ 0.002, so that at 0.82 µm V ≈ 2 π ( 5 µ m ) 0.82 µ m 1.45 2(0.002) = 3.514 Thus the fiber is no longer single-mode. From Figs. 2-18 and 2-19 we see that the LP 01 and the LP 11 modes exist in the fiber at 0.82 µm. 2-24. 2-25. From Eq. (2-77) L p = 2 π β = λ n y − n x For L p = 10 cm n y - n x = 1.3 × 10 − 6 m 10 −1 m = 1.3×10 -5 For L p = 2 m n y - n x = 1.3 × 10 − 6 m 2 m = 6.5×10 -7 Thus 6.5×10 -7 ≤ n y - n x ≤ 1.3×10 -5 2-26. We want to plot n(r) from n 2 to n 1 . From Eq. (2-78) n(r) = n 1 1 − 2 ∆ (r/a) α [ ] 1 / 2 = 1.48 1 − 0.02(r/25) α [ ] 1 / 2 n 2 is found from Eq. (2-79): n 2 = n 1 (1 - ∆) = 1.465 2-27. From Eq. (2-81) M = α α + 2 a 2 k 2 n 1 2 ∆ = α α + 2 2 π an 1 λ     2 ∆ where ∆ = n 1 − n 2 n 1 = 0.0135 [...]... the volume of the fiber drawn from this section The preform section of length Lpreform is drawn into a fiber of length Lfiber in a time t If S is the preform feed speed, then Lpreform = St Similarly, if s is the fiber drawing speed, then Lfiber = st Thus, if D and d are the preform and fiber diameters, respectively, then Preform volume = Lpreform(D/2)2 = St (D/2)2 Fiber volume = Lfiber (d/2)2 = st... geometries of the preform and its corresponding fiber: 25 µm R 4 mm 62.5 3 mm µm FIBER PREFORM We want to find the thickness of the deposited layer (3 mm - R) This can be done by comparing the ratios of the preform core-to-cladding cross-sectional areas and the fiber core-to-cladding cross-sectional areas: A preform core A fiber core = Apreform clad A fiber clad or π(32 − R2 ) π (25)2 = π(42 − 32 )... two fiber samples, F1 = F2, or   σ m L   σ m L  1c 1 2  2c  1 - exp −   = 1 - exp −  σ  L  0  0   σ0  L0   which implies that m m  σ1c  L1  σ 2c  L 2    =  σ 0  L 0  σ0  L0 or σ1c  L 2  =   σ 2c  L1  1/m If L1 = 20 m, then σ1c= 4.8 GN/m2 If L2 = 1 km, then σ2c= 3.9 GN/m2 Thus m 1000  4.8  = = 50  3.9  20 gives m= log 50 = 18.8 log(4.8/ 3.9) 16 Problem Solutions... π(42 − 32 ) π [(62.5)2 − (25)2 ] from which we have   7(25)2 R = 9 − 2 2  (62.5) − (25)  1/ 2 = 2.77 mm Thus, thickness = 3 mm - 2.77 mm = 0.23 mm 2-31 (a) The volume of a 1-km-long 50-µm diameter fiber core is V = πr2L = π (2.5×10-3 cm)2 (105 cm) = 1.96 cm3 The mass M equals the density ρ times the volume V: M = ρV = (2.6 gm/cm3)(1.96 cm3) = 5.1 gm 12 (b) If R is the deposition rate, then the deposition... ] which is Eq (2-87) When a static stress σs is applied after proof testing, the time to failure is found from Eq (2-86): χs ∫ χ −b / 2 dχ = AYb σ b s χp ts ∫ dt 0 where χ s is the crack depth at the fiber failure point Integrating (as above) we get Eq (289): [ ] B σ b−2 − σsb−2 = σ b ts p s Adding Eqs (2-87) and (2-89) yields Eq (2-90) 14 2-35 (a) Substituting Ns as given by Eq (2-92) and Np as given...At λ = 820 nm, M = 543 and at λ = 1300 nm, M = 216 For a step index fiber we can use Eq (2-61) V2 1  2πa  2 2 n n2 Mstep ≈ =   ( 1 − 2) 2 2 λ At λ = 820 nm, Mstep = 1078 and at λ = 1300 nm, Mstep = 429 Alternatively, we can let α = ∞ in Eq (2-81): 2  2πan1  ∆= Mstep... opt ) 0.05 = =− = −170% (0.015)(1.95) σ int er (α = α opt ) ∆(α + 2) For α = 1.05αopt , we have σ int er (α ≠ αopt ) (α − α opt ) 0.05 = =+ = +163% (0.015)(2.05) σ int er (α = αopt ) ∆(α + 2) 12 Problem Solutions for Chapter 4 4-1 3/4 2πkBT3/2  Eg  From Eq (4-1), ni = 2  2  (memh) exp - 2k T B    h   2π(1.38 × 10−23 J / K)  =2  −34 2  (6.63 × 10 J.s)   3/ 2 T 3 /2 [(.068)(.56)(9.11×... Plot of Eq (4-18) Some representative values of P/P0 are given in the table: f in MHz 1 10 20 40 60 80 100 4-8 1 2 26 mW = 0.37 mW 3.5(3.5 + 1) P/P0 0.999 0.954 0.847 0.623 0.469 0.370 0.303 The 3-dB optical bandwidth is found from Eq (4-21) It is the frequency f at which the expression is equal to -3; that is,  1 10 log 2  1 + (2πfτ ) [  1/ 2  = −3  ] 3 With a 5-ns lifetime, we find f = 4-9 . the fiber drawing speed, then L fiber = st. Thus, if D and d are the preform and fiber diameters, respectively, then Preform volume = L preform (D/2) 2 = St (D/2) 2 and Fiber volume = L fiber . cross-sectional area A must equal the volume of the fiber drawn from this section. The preform section of length L preform is drawn into a fiber of length L fiber in a time t. If S is the preform feed. core-to-cladding cross-sectional areas and the fiber core-to-cladding cross-sectional areas: A preform core A preform clad = A fiber core A fiber clad or π (3 2 − R 2 ) π (4 2 − 3 2 ) =

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