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Measurement of the mutual coherence function of an incoherent infrared field with a gold nano-wire dipole antenna array

机译:用金纳米线偶极子天线阵测量非相干红外场的互相干函数

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The first direct measurement of the mutual coherence function of a spatially incoherent infrared beam was performed at 10.6 mu m using a pair of infrared dipole nano-wire antennas that were connected to a common bolometer in the center of the pair by short lengths of coplanar strip transmission line. A spatially incoherent source was constructed by dithering a BaF2 diffuser near the focus of a CO2 laser beam. The distance from the diffuser to the nano-wire antenna pair was held constant while the distance from the focus of the laser beam to the diffuser was varied to control the effective diameter of the source. The measured bolometer signal was proportional to the magnitude of the mutual coherence function at the plane of the antennas. The experimental results were found to match the predicted performance closely. If this technology can be extended to large arrays, a form of synthetic aperture optical imaging based on the Van Cittert-Zernike theorem is possible, similar to that performed at microwave frequencies now by astronomers. This has the potential to greatly increase the angular resolution attainable with optical instruments.
机译:使用一对红外偶极纳米线天线,在10.6微米处对空间不相干红外光束的互相干函数进行首次直接测量,该对偶极纳米线天线通过短共平面带连接到该对中心的公共辐射热测量计传输线。通过使BaF2扩散器在CO2激光束焦点附近抖动来构造空间不相干的光源。从扩散器到纳米线天线对的距离保持恒定,而从激光束焦点到扩散器的距离则变化以控制源的有效直径。测得的辐射热计信号与天线平面处的互相关函数的大小成比例。实验结果与预测的性能非常接近。如果这项技术可以扩展到大阵列,那么基于Van Cittert-Zernike定理的合成孔径光学成像的形式就可能成为可能,类似于现在天文学家在微波频率下进行的成像。这有可能大大提高光学仪器可达到的角分辨率。

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