A Two-Stage S-Band Erbium-Doped Fiber Amplifier Based on W-type Erbium-Doped Fiber

  • Received Date: March 02, 2010
  • Published Date: August 31, 2010
  • An S-band erbium-doped fiber (EDF) amplifier based on a W-type EDF designed by ourselves is demonstrated by employing a two-stage double-pass configuration. The amplifier provides a bandwidth of 34 nm (1486-1520 nm) for the gain over 20 dB. The maximal gain of 32.8 dB is achieved at 1501 nm and the corresponding noise figure is 6.0 dB. The proposed amplifier has a promising foreground in extending the current network to the S band.
  • Article Text

  • [1] Kasamatsu T et al 1999 Proc. OAA 30 46
    [2] Kasamatsu T et al 2002 J. Lightwave Technol. 20 1826
    [3] Aozasa S, Masuda H and Shimizu M 2006 J. Lightwave Technol. 24 3842
    [4] Bromage J, Bouteiller J C, Thiele H J, Brar K, Park H J, Headlefl C, Nelson L E et al 2001 Optical Fiber Communications Conference 70 PD1
    [5] Arbore M, Zhou Y, Thiele H, Bromage J and Nelson L 2003 Optical Fiber Communications Conference l 374
    [6] Rosolem J B, Juriollo A A, Arradi R, Coral A D, Oliverira J C F and Romero A 2005 IEEE Photon. Technol. Lett. 17 1399
    [7] Harun S W, Saat N K and Ahmad H 2005 Chin. Phys. Lett. 22 3080
    [8] Wang L A and Chen C D 1997 IEEE Photon. Technol. Lett. 9 446
    [9] Wang L A and Chen C D 1997 Electron. Lett. 33 703
    [10] Sun J J, Ding L and Lu K C 2009 OFCIO 15 62
    [11] Zhang Z Q, Ding L, Xing J B, Wang S M and Lu K C 2009 Acta Opt. Sin. 7 1885
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