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Fig. 12-1: Network topologies

Fig. 12-1: Network topologies. Fig. 12-2: Bus-coupler losses. Fig. 12-3: Linear bus topology. Fig. 12-4: Liner bus versus star coupler. Fig. 12-5: Basic STS-1 SONET frame. Fig. 12-6: Basic STS-N SONET frame. Fig. 12-7a: 2-fiber UPSR. Fig. 12-7b: 2-fiber UPSR.

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Fig. 12-1: Network topologies

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  1. Fig. 12-1: Network topologies

  2. Fig. 12-2: Bus-coupler losses

  3. Fig. 12-3: Linear bus topology

  4. Fig. 12-4: Liner bus versus star coupler

  5. Fig. 12-5: Basic STS-1 SONET frame

  6. Fig. 12-6: Basic STS-N SONET frame

  7. Fig. 12-7a: 2-fiber UPSR

  8. Fig. 12-7b: 2-fiber UPSR

  9. Fig. 12-8(varied): BLSR architecture

  10. Fig. 12-9: BLSR reconfiguration

  11. Fig. 12-10: Four-fiber BLSR Reconfiguration

  12. Fig. 12-11: Generic SONET network

  13. Fig. 12-12: SONET ADM

  14. Fig. 12-13: Dense WDM deployment

  15. Fig. 12-14: Two types of WDM LANs

  16. Fig. 12-15: Single-hop network

  17. Fig. 12-16: Multihop architecture

  18. Fig. 12-17: Data packet

  19. Fig. 12-18: ShuffleNet

  20. Fig. 12-19: Wavelength reuse

  21. Fig. 12-20: Optical cross-connect architecture

  22. Fig. 12-21: Optical cross-connect

  23. Fig. 12-22: Wavelength utilization

  24. Fig. 12-23: Wavelength utilization

  25. Fig. 12-24: Increase in utilization

  26. Fig. 12-25: Effective length

  27. Fig. 12-26: SRS effects

  28. Fig. 12-27: Raman gain effects

  29. Fig. 12-28: Allowed power per wavelength

  30. Fig. 12-29: SBS effects

  31. Fig. 12-30: SBS effect on CNR

  32. Fig. 12-31: Spectral broadening due to SPM

  33. Fig. 12-32: 3rd-order sidebands

  34. Fig. 12-33: FWM efficiency

  35. Fig. 12-34: Dispersion & power maps

  36. Fig. 12-35: SNR degradation

  37. Fig. 12-36: Interchannel crosstalk

  38. Fig. 12-37: Intrachannel crosstalk

  39. Fig. 12-38: Crosstalk penalties

  40. Fig. 12-39: Kerr effect

  41. Fig. 12-40: First-order soliton

  42. Fig. 12-41: Hyperbolic secant

  43. Fig. 12-42: Dispersion & nonlinear phase shifts

  44. Fig. 12-43: Soliton pulse width

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