High power compatible internally sensed optical phased array

被引:34
作者
Roberts, Lyle E. [1 ,2 ]
Ward, Robert L. [1 ,2 ]
Francis, Samuel P. [1 ,2 ]
Sibley, Paul G. [1 ,2 ]
Fleddermann, Roland [1 ]
Sutton, Andrew J. [1 ]
Smith, Craig [2 ,3 ]
McClelland, David E. [1 ]
Shaddock, Daniel A. [1 ,2 ]
机构
[1] Australian Natl Univ, Res Sch Phys & Engn, Dept Quantum Sci, GPO Box 4, Canberra, ACT 2601, Australia
[2] Mt Stromlo & Siding Spring Observ, Adv Instrumentat & Technol Ctr, SERC, Weston, ACT 2611, Australia
[3] Mt Stromlo & Siding Spring Observ, EOS Space Syst Pty Ltd, EOS House, Weston, ACT 2611, Australia
来源
OPTICS EXPRESS | 2016年 / 24卷 / 12期
基金
澳大利亚研究理事会;
关键词
ENHANCED HETERODYNE INTERFEROMETRY; BRILLOUIN-SCATTERING; FIBER AMPLIFIERS; LOCKING; MODULATION; KW;
D O I
10.1364/OE.24.013467
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The technical embodiment of the Huygens-Fresnel principle, an optical phased array (OPA) is an arrangement of optical emitters with relative phases controlled to create a desired beam profile after propagation. One important application of an OPA is coherent beam combining (CBC), which can be used to create beams of higher power than is possible with a single laser source, especially for narrow linewidth sources. Here we present an all-fiber architecture that stabilizes the relative output phase by inferring the relative path length differences between lasers using the small fraction of light that is back-reflected into the fiber at the OPA's glass-air interface, without the need for any external sampling optics. This architecture is compatible with high power continuous wave laser sources (e.g., fiber amplifiers) up to 100 W per channel. The high-power compatible internally sensed OPA was implemented experimentally using commercial 15 W fiber amplifiers, demonstrating an output RMS phase stability of lambda/194, and the ability to steer the beam at up to 10 kHz. (C) 2016 Optical Society of America
引用
收藏
页码:13467 / 13479
页数:13
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