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A daylight experiment for teaching stellar interferometry

机译:教授恒星干涉法的日光实验

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We discuss the design of a simple experiment that reproduces the operation of the Michelson stellar interferometer. The emission of stellar sources has been simulated using light emerging from circular end-faces of step-index polymer optical fibers and from diffuse reflections of laser beams. Interference fringes have been acquired using a digital camera, coupled to a telescope obscured by a double aperture lid. The experiment is analogous to the classical determination of stellar sizes by Michelson and can be used during the day. Using this experimental set-up, we can determine the size of extended sources, located at a distance of about 75m from our telescope, with errors less than 25%.
机译:我们讨论了一个简单实验的设计,该实验再现了迈克尔逊恒星干涉仪的操作。已使用阶跃折射率聚合物光纤的圆形端面和激光束的漫反射发出的光模拟了恒星源的发射。干涉条纹已经使用数码相机获取,并与双孔盖遮盖的望远镜连接。该实验类似于迈克尔逊(Michaelson)对恒星大小的经典确定,可以在白天使用。使用此实验设置,我们可以确定距望远镜约75m的扩展源的尺寸,误差小于25%。

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