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Wide field imaging spectroscopy using aberration-corrected holography

机译:使用像差校正全息术的宽场成像光谱

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The most powerful diagnostics of hot gas in the universe are well understood, but there are few instruments capable of making measurements at the wavelengths of the most important lines (103 nm, 123 nm, and 155 nm, the lithium-like series of O, N, and C). No complete survey has been done with moderate spatial resolution in emission even though virtually all measurements capable of detecting the presence of lithium-like oxygen do so. We present a type of imaging spectrograph that takes advantage of the large, well-corrected field of view from a three-mirror anastigmat (TMA) in conjunction with aberration-corrected holography applied to the tertiary. The combination of a TMA and aberration-corrected holography allows a large well-corrected field of view in diffracted light, potentially providing an excellent basis for an instrument capable of the first large scale survey from 100 nm to 150 nm.
机译:宇宙中热气体最强大的诊断得很好,但是有很少的仪器能够在最重要的线条的波长下进行测量(103nm,123nm和155nm,锂样系列O, n,c)。 即使几乎所有能够检测锂状氧气的存在,也没有在发射中进行中等空间分辨率进行完整的调查。 我们介绍了一种成像光谱仪,其与三镜子Anastigmat(TMA)结合使用施加到第三镜的像差校正全息术来利用大型良好校正的视野。 TMA和像差校正全息术的组合允许在衍射光中进行大的良好校正的视野,潜在地为能够从100nm至150nm的第一大规模调查的仪器提供优异的基础。

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