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MATISSE selection mechanism development

机译:MATISSE选择机制的发展

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MATISSE (Multi AperTure mid-Infrared SpectroScopic Experiment) will be a mid-infrared spectro-interferometercombining the beams of up to four telescopes of the European Southern Observatory Very Large TelescopeInterferometer (ESO VLTI), providing phase closure and image reconstruction. MATISSE will produce interferometricspectra in the LM and in the N band (3.0 to 13.0 micron) and is as such a successor of MIDI. Beams pass the warm preopticsand in the cold optics all beams recombine on the detector where they create a spectral interference pattern.Instruments with a large wavelength bandwidth like MATISSE usually comprise mechanisms for selection ofobservation mode, filters, dispersing elements, pinholes or slits. The cryogenic operating environment poses severalchallenges to these cryogenic mechanisms like differential thermal shrinkage, physical property change of materials andlubrication. For the MATISSE instrument two concepts of selection mechanisms can be distinguished: linear selectionmechanisms (sliders) and rotating selection mechanisms (wheels). Both mechanisms provide high accuracy andrepeatability. The feature density is high in a limited space envelope. Cryogenic electric motors are used as the actuatorfor all these mechanisms. This paper describes the design and realization of these linear and rotating selectionmechanisms.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:MATISSE(Multi AperTure中红外光谱实验)将是一种中红外光谱干涉仪,它将欧洲南部天文台超大型望远镜干涉仪(ESO VLTI)的多达四台望远镜的光束组合在一起,提供相封闭和图像重建功能。 MATISSE将在LM和N波段(3.0到13.0微米)产生干涉光谱,并以此作为MIDI的后继者。光束通过温暖的光学元件,然后在冷光学元件中所有光束重新组合在检测器上,从而在光谱仪上产生光谱干涉图样。诸如MATISSE之类的大波长带宽的仪器通常包括用于选择观察模式的机制,滤光片,色散元件,针孔或狭缝。低温运行环境对这些低温机理提出了若干挑战,例如差异热收缩,材料物理性能变化和润滑。对于MATISSE仪器,可以区分选择机制的两个概念:线性选择机制(滑块)和旋转选择机制(轮)。两种机制均提供高精度和可重复性。在有限的空间包络中,特征密度很高。低温电动机被用作所有这些机构的致动器。本文介绍了这些线性和旋转选择机制的设计和实现。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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