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

机译:用于衍射极限3D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"× 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:我们已经为位于基特峰国家太阳能天文台的麦克马斯·皮尔斯太阳望远镜(McMP)开发了最先进的图像切片器积分场单元(IFU)。 IFU将用于高分辨率的3D光谱学和偏振计,可通过自适应光学器件很好地校正。它由19个有效切片组成,对应于6.27“×7”的视场。 IFU向现有的光谱仪提供152英寸长的狭缝,从而产生衍射受限的3维光谱。3D仪器用于对太阳进行高空间和高时间分辨率成像,这对于磁场至关重要二维太阳精细结构的光谱学和光谱学研究,我们将与McMP讨论仪器的构造,实验室测试和现场试验观察。

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