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An IFU for diffraction-limited 3-D spectroscopic imaging: laboratoryand on-site tests

机译:用于衍射限制3-D光谱成像的IFU:实验室和现场测试

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We have developed a state-of-the-art image slicer Integral Field Unit (IFU) for the McMath-Pierce Solar Telescope (McMP) located at Kitt Peak National Solar Observatory. The IFU will be used for high-resolution 3-dimensional spectroscopy and polarimetry over a small field of view that is well corrected by adaptive optics. It consists of 19 effective slices that correspond to a field of view of 6.27" x 7". The IFU delivers a 152" long slit to an existing spectrograph producing diffraction-limited 3-dimensional spectroscopy. The 3-D instrument is being used for high-spatial and high-temporal resolution imaging of the Sun, which is crucial for the magnetic field and spectroscopic studies of 2-dimensional solar fine structures. We discuss the instrument construction, laboratory test and on-site trial observations with the McMP.
机译:我们为位于Kitt Peak国家太阳天文台的McMath-Pierce Solar Telescope(MCMP)开发了一个最先进的图像切片机整体单元(IFU)。 IFU将用于高分辨率三维光谱和偏振基,通过自适应光学良好校正的小视野。它由19个有效切片组成,该切片对应于6.27“x 7”的视野。 IFU向现有的光谱仪提供152英寸的长缝,产生衍射限制的三维光谱。3-D仪器用于太阳的高空间和高时间分辨率成像,这对于磁场至关重要和二维太阳能细结构的光谱研究。我们与MCMP讨论仪器施工,实验室试验和现场试验观察。

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