Length dependency of modal noise and scrambling effect of fibers under incoherent light

Zhenyu Ma, Yuchen Pang, Kangquan Sun, Han Liu, Weimin Sun, Yunxiang Yan
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Abstract

Fiber scrambling is important in high-precision calibration systems for radial velocity measurement for searching for exoplanets. As for laser frequency combs, the modal noise of significant laser speckles can occur due to the strong coherence of the light source, which can be effectively suppressed by vibrating the fiber. However, the fibers used for scientific target detection are coupled with polychromatic light from the celestial body. This study focuses on the fiber mode noise and length dependency under white light conditions, and proposes a new fiber scrambling method of combining different types of fiber to achieve high scrambling gain. The results show that the fiber mode noise increases with decreasing length, and that there is also significant mode noise when the fiber is less than 2m, resulting in a speckle-like pattern as the modal pattern in the near field. The combination of non-circular fibers and graded index fibers can effectively reduce mode noise and improve the scrambling gain.
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非相干光下光纤模态噪声和扰频效应的长度依赖性
光纤扰频在用于搜索系外行星的径向速度测量的高精度校准系统中非常重要。至于激光频率梳,由于光源的强相干性,可能会出现明显的激光斑点模态噪声,这可以通过振动光纤来有效抑制。然而,用于科学目标探测的光纤是与来自天体的多色光耦合的。本研究重点研究了白光条件下的光纤模式噪声和长度依赖性,并提出了一种结合不同类型光纤的新型光纤扰频方法,以获得较高的扰频增益。研究结果表明,光纤模式噪声随长度的减小而增大,当光纤长度小于 2m 时,也会出现明显的模式噪声,导致近场模态模式出现斑点状。非圆形光纤和分级索引光纤的组合可有效降低模式噪声,提高扰频增益。
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