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首页> 外文期刊>Sensors and Actuators, A. Physical >MAGNETO-OPTICAL POSITION-RESOLVING SENSOR FOR DISPLACEMENT MEASUREMENTS BETWEEN LIGHT BEAMS
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MAGNETO-OPTICAL POSITION-RESOLVING SENSOR FOR DISPLACEMENT MEASUREMENTS BETWEEN LIGHT BEAMS

机译:用于光束之间位移测量的磁光位置分辨传感器

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The dispersion of the refractive index of the atmosphere leads to small angles (delta beta approximate to 1 mu rad) between light beams of different wavelengths (e.g., red and green) and therefore the images of these beams in the focal plane of a telescope are displaced by a few micrometres. According to this fact, geodetical refraction measurements can be accomplished by a position-resolving sensor. The magneto-optical transversal Kerr effect of a 40 nm thin iron film is used to modulate the light beams up to 100 kHz. Separating the beams by a colour-sensitive beamsplitter, the displacement between the two focal points is measured by the time difference of the corresponding photodiode signals. The relation between the time and a locally defined magnetization reversal of the film is achieved by a ferrite C-yoke with gradient pole shoes and the rectangular hysteresis of the iron film. Simulating the conditions of refraction measurements in the atmosphere at a total light power of 5 mu W on the front end of the telescope (focal length 1.5 m), a resolution of 35 nm is achieved, which corresponds to an angular resolution for delta beta of 23 nrad. [References: 7]
机译:大气折射率的分散会导致不同波长(例如红色和绿色)的光束之间的角度较小(δbeta近似于1μrad),因此这些光束在望远镜焦平面中的像是位移了几微米。根据这一事实,大地折射测量可以通过位置分辨传感器来完成。 40 nm铁薄膜的磁光横向Kerr效应用于调制高达100 kHz的光束。用色敏分束器将光束分开,通过相应光电二极管信号的时间差来测量两个焦点之间的位移。时间与薄膜的局部磁化反转之间的关系是通过带有梯度极靴的铁氧体C形磁轭和铁薄膜的矩形磁滞实现的。在望远镜前端(焦距1.5 m)上以5μW的总光功率模拟大气中的折射测量条件,可获得35 nm的分辨率,这对应于δβ的角分辨率23拉德[参考:7]

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