Highly stable fiber lasers for satellite-based gravitational measurements

被引:2
|
作者
Fitzau, O. [1 ]
Betz, P. [1 ]
Cebeci, P. [1 ]
Giesberts, M. [1 ]
Hoffmann, H-D [1 ]
Schiemangk, M. [2 ]
Wicht, A. [2 ]
Sanjuan, J. [3 ]
Dahl, K. [4 ]
Pyka, S. Amairi [5 ]
Kovalchuk, E. [5 ]
Peters, A. [5 ]
机构
[1] Fraunhofer Inst Laser Technol ILT, Aachen, Germany
[2] Ferdinand Braun Inst, Leibniz Inst Hochstfrequenztech FBH, Berlin, Germany
[3] Deutsch Zentrum Luft & Raumfahrt DLR, Inst Raumfahrtsyst, Cologne, Germany
[4] SpaceTech GmbH STI, Bodensee, Germany
[5] Humboldt Univ, Inst Phys, Berlin, Germany
来源
FIBER LASERS XVI: TECHNOLOGY AND SYSTEMS | 2019年 / 10897卷
关键词
Fiber Laser; Fiber Amplifier; Semiconductor Amplifier; Low-Noise; Relative Intensity Noise; Narrow Linewidth; LISA; NGGM;
D O I
10.1117/12.2509950
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
For studies of the European Space Agency ESA, Fraunhofer ILT develops and builds narrowband, power-stabilized fundamental mode fiber amplifiers especially for future space-based gravitational-wave detectors, e.g. LISA, and for Earth gravity field missions. In this paper, we present the status of our ongoing work, based on a highly stable fiber amplifier designed for a Next Generation Gravity field Mission (NGGM) pre-study, towards power scaling as well as enhancement of the Technology Readiness Level (TRL). Our amplifier has already demonstrated to meet the requirements for future gravity field missions. It features a design that is free of stimulated Brillouin scattering (SBS) and a feedback loop for power stabilization.
引用
收藏
页数:11
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