Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group
  • 2013 Conference on Lasers and Electro-Optics - International Quantum Electronics Conference
  • (Optica Publishing Group, 2013),
  • paper CJ_1_6

Fundamental Gaussian mode content measurements on active large core CCC fibers

Not Accessible

Your library or personal account may give you access

Abstract

Applications in gravitational wave detectors [1] require high power lasers with approximately 200 W of single-frequency output in linearly polarized TEM00-mode. Single-frequency signals have been amplified to more than 500 W in master oscillator power amplifier (MOPA) configurations, employing photonic crystal fibers (PCF) [2] as well as chirally coupled core (CCC) fibers [3]. For a PCF amplifier system, a fundamental Gaussian mode power of 203 W was demonstrated in linear polarization [4]. In this contribution we report for the first time measurements of the overlap of high power CCC fiber amplifiers output beam with the TEM00-mode of a scanning non-confocal ring cavity [5].

© 2013 IEEE

PDF Article
More Like This
Single-frequency Yb-doped PCF MOPA with 294 W of output power for gravitational wave detection

M. Karow, C. Basu, D. Kracht, J. Neumann, and P. Wessels
CJ7_4 The European Conference on Lasers and Electro-Optics (CLEO/Europe) 2011

Fiber Amplifiers for Gravitational Wave Detection

P. Weßels, M. Karow, V. Kuhn, M. Steinke, H. Tünnermann, D. Kracht, and J. Neumann
MA1_1 Conference on Lasers and Electro-Optics/Pacific Rim (CLEO/PR) 2013

Fiber integrated Ytterbium single frequency amplifier with a measured fundamental mode power content of 91% at 215 W

T. Theeg, H. Sayinc, J. Neumann, L. Overmeyer, and D. Kracht
W3.33 Workshop on Specialty Optical Fibers and their Applications (WSOF) 2013

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.