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Study on Spectrograph for Ionosphere: a Broadband Imaging Instrument Prototype for Far-Ultraviolet

机译:电离层光谱仪的研究:一种用于远紫外线的宽带成像仪器原型

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Current research on space-based exploration for the ionosphere needs more advanced technologies. Because the spectral signals in the ionosphere distributing basically in the far-ultraviolet waveband are very weak. Usual spectrometer structures and detectors such as CCD can't receive enough information. Based on this principle of atmospheric sounding, the imaging spectrometer prototype for ionosphere detection application was designed to solve the problem. This prototype consists of the telescope and the imaging spectrometer. The simple structure and small number of mirrors can help higher transmission efficiency be achieved and weak signals detection be implemented. The telescope is an off-axis parabolic mirror and the spectrometer is a modified Czerny-Turner spectral imaging system. Modified Czerny-Turner spectrometer contains a spherical mirror, a fixed plane grating and a toroidal mirror. By adjusting the incident angle to the collimating mirror and using toroidal mirror, coma and astigmatism were corrected well. We also optimize distances between the grating to the focusing mirror and the focusing mirror to the image plane to improve disadvantages of traditional Czerny-Turner structure. Designed results demonstrate that aberrations are substantially corrected, and high image quality can be obtained in broad waveband. The photon counting Wedge-Strip-Anode detector with micro-channel planes as the receiving plane is accepted for the instrument prototype. The other photon counting 2-D detector responding well for weak light such as Cross-Delay line detector and MAMA detector can also be used for detection. The calibration and performances testing system is made of a vacuum system, a deuterium lamp, a monochrometer and the instrument prototype. Results obtained from the experiment show that the spectral resolution is 2.4 nm and the spatial resolution is 80 μm. The other calibration experiments are running. The technology of the spectrometer prototype is important for the research and applications of ionosphere remote sensing.
机译:当前对电离层进行天基探测的研究需要更先进的技术。由于电离层中的光谱信号基本上分布在远紫外线波段,因此非常微弱。常规的光谱仪结构和检测器(如CCD)无法接收到足够的信息。基于大气探测的这一原理,设计了用于电离层探测应用的成像光谱仪原型来解决该问题。该原型机由望远镜和成像光谱仪组成。简单的结构和少量的反射镜可以帮助实现更高的传输效率,并实现微弱的信号检测。望远镜是离轴抛物面镜,光谱仪是经过改进的Czerny-Turner光谱成像系统。修改后的Czerny-Turner光谱仪包含一个球面镜,一个固定平面光栅和一个环形镜。通过调节准直镜的入射角并使用环形镜,可以很好地矫正昏迷和散光。我们还优化了光栅到聚焦镜的距离以及聚焦镜到像平面的距离,以改善传统的Czerny-Turner结构的缺点。设计结果表明,像差已得到基本校正,并且可以在宽波段获得高图像质量。仪器原型接受以微通道平面作为接收平面的光子计数楔形条阳极检测器。其他对弱光响应良好的光子计数二维检测器(如Cross-Delay线检测器和MAMA检测器)也可以用于检测。校准和性能测试系统由真空系统,氘灯,单色仪和仪器原型组成。从实验中获得的结果表明,光谱分辨率为2.4 nm,空间分辨率为80μm。其他校准实验正在运行。光谱仪原型技术对电离层遥感的研究和应用具有重要意义。

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