Publikationen

973 nm wavelength stabilized hybrid ns-MOPA diode laser system with 15.5 W peak power and a spectral line width below 10 pm

T.N. Vua,b, A. Klehra, B. Sumpfa, H. Wenzela, G. Erberta, G. Tränklea

Published in:

Proc. SPIE, vol. 9134, Photonics Europe, Brussels, Belgium, Apr. 14-17, 91340T (2014).

Abstract:

A master oscillator power amplifier (MOPA) system for the generation of ns-pulses with high peak power, narrow spectral line width, and stabilized emission wavelength will be presented. The master oscillator is a distributed feedback (DFB) ridge waveguide (RW) laser. The tapered amplifier consists of one RW section and one flared gain-guided section. The DFB laser is operated in continuous wave mode and emits at 973.5 nm with a spectral line width below 10 pm. The RW section of the amplifier acts as an optical gate. The tapered section amplifies the generated optical pulse. An optical peak power of 15.5 W for a pulse width of 8 ns is obtained. The emission wavelength remains constant at all output power levels of the MOPA system for a fixed current into the DFB laser. The spectral power density of the ASE is 37 dB smaller than the lasing spectral power density. The spectral line width is smaller than 10 pm, limited by the resolution of the optical spectrum analyzer.

a Ferdinand-Braun-Institut, Leibniz-Institut für Höchstfrequenztechnik, Gustav-Kirchhoff-Straße 4, 12489 Berlin, Germany
b Institute of Materials Science, Vietnam Academy of Science and Technology, 18 Hoang Quoc Viet rd., Cau Giay, Hanoi, Vietnam

Keywords:

ns-pulses, semiconductor lasers, narrow spectral line width, master oscillator power amplifier (MOPA), distributed feedback (DFB) laser, tapered power amplifier.

© 2014 COPYRIGHT SPIE--The International Society for Optical Engineering. Personal use of this material is permitted. However, permission to reprint/republish this material for advertising or promotional purposes or for creating new collective works for resale or redistribution to servers or lists, or to reuse any copyrighted component of this work in other works must be obtained from the SPIE.

Full version in pdf-format.