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Comparative study of mid-infrared fibers for modal filtering

机译:中红外光纤模态滤波的比较研究

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We compare the filtering capabilities of two infrared fibers developed to achieve a high rejection ratio of the higher order modes in order to obtain compact modal filters devoted to stellar interferometry. Two types of double-clad fibers are studied: a fiber with a second thin absorbing cladding and a fiber with a second thick absorbing cladding closer to the fiber core; both are single mode around the CO_(2) band (10.6 (mu)m). We present the single-mode spectral domain and the nulling capabilities of both fibers for different fiber lengths, comparing simulations with experimental results. We show that the filtering capabilities are improved when the absorbing clad is closer to the fiber core, as the propagation distance needed to filter out these modes is shorter. Thus, to obtain high rejection ratios in compact devices, an absorbing cladding close to the core of the fiber is compulsory in order to suppress cladding modes that could eventually recouple into the waveguide. We present an empirical model that allows determining the minimum filter length, considering only one effective leaky mode with low attenuation, which considerably simplifies the theoretical studies.
机译:我们比较了为获得高阶模的高抑制比而开发的两种红外光纤的滤波能力,以获得用于恒星干涉测量的紧凑型模态滤波器。研究了两种类型的双包层光纤:具有第二薄吸收包层的光纤和具有靠近纤维纤芯的第二厚吸收包层的光纤。两者都是CO_(2)频带(10.6μm)附近的单模。我们将单模光谱域和两种光纤针对不同光纤长度的归零能力进行了比较,并将仿真结果与实验结果进行了比较。我们表明,当吸收包层靠近光纤纤芯时,滤波能力会得到改善,因为滤除这些模式所需的传播距离更短。因此,为了在紧凑的设备中获得高拒绝率,必须抑制靠近光纤纤芯的吸收包层,以抑制最终可能重新耦合到波导中的包层模式。我们提出了一种经验模型,该模型可以确定最小滤波器长度,仅考虑一种低衰减的有效泄漏模式,从而大大简化了理论研究。

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