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A Laser Frequency Comb System for Absolute Calibration of the VTT Echelle Spectrograph

机译:激光频率梳系统,用于绝对校准VTT艾歇尔光谱仪

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A wavelength calibration system based on a laser frequency comb (LFC) was developed in a co-operation between the Kiepenheuer-Institut für Sonnenphysik, Freiburg, Germany and the Max-Planck-Institut für Quantenoptik, Garching, Germany for permanent installation at the German Vacuum Tower Telescope (VTT) on Tenerife, Canary Islands. The system was installed successfully in October 2011. By simultaneously recording the spectra from the Sun and the LFC, for each exposure a calibration curve can be derived from the known frequencies of the comb modes that is suitable for absolute calibration at the meters per second level. We briefly summarize some topics in solar physics that benefit from absolute spectroscopy and point out the advantages of LFC compared to traditional calibration techniques. We also sketch the basic setup of the VTT calibration system and its integration with the existing echelle spectrograph.
机译:在德国弗赖堡的Siennphysik研究所和德国Garching的Max-Planck研究所的合作下开发了基于激光频率梳(LFC)的波长校准系统,以便在德国永久安装加那利群岛特内里费岛的真空塔望远镜(VTT)。该系统于2011年10月成功安装。通过同时记录来自太阳和LFC的光谱,对于每次曝光,可以从已知的梳形模式频率得出校准曲线,该曲线适用于每秒米级的绝对校准。 。我们简要总结了太阳物理学中受益于绝对光谱的一些主题,并指出了LFC与传统校准技术相比的优势。我们还概述了VTT校准系统的基本设置及其与现有echelle光谱仪的集成。

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