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Instrument for Setting Radio Telescope Surfaces

机译:设置射电望远镜表面的仪器

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摘要

The Green Bnak Telescope (GBT) (1) is a 100-meter radio telescope under construction by The National Radio Astronomy Observantory in Green Bank, WV. The GBT incorporates a first-of-its-kind active surface that will be adjusted under a closed-loop laser metrology system (2) to correct surface deflections. The goal is to maintain a reflector surfae accuracy of 0.220-mm rms in order to operate down to 3-mm wavelengths. (100 GHz). The reflector is made up of 2004 individual panels, each of which is manufactured to a section of a 60-meter focal length paraboloid surface to an accuracy of 0.075-mm rms. The panels rest on 2209 motor-driven actuators that adjust the surface to correct for deflections in the telescope backup structure. A bracket on each actuator joints the corners of four panels, so each actuator moves the four adjacent panel corers as a signle unit and thus the relative location of the four corners remains fixed.
机译:Green Bnak望远镜(GBT)(1)是西弗吉尼亚州格林班克的国家射电天文台正在建造的100米射电望远镜。 GBT包含首创的主动表面,可在闭环激光计量系统(2)下对其进行调整以校正表面变形。目的是保持反射器表面精度为0.220 mm rms,以便在3 mm的波长下工作。 (100 GHz)。该反射器由2004个单独的面板组成,每个面板都制造为60米焦距抛物面的一部分,精度为0.075-mm rms。面板靠在2209个电动执行器上,该执行器调整表面以校正望远镜备用结构中的挠度。每个执行器上的支架连接四个面板的角,因此每个执行器将四个相邻的面板去芯器作为信号单元移动,因此四个角的相对位置保持固定。

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