Ultraviolet, visible and ultraviolet prism chromatic dispersion imaging spectrometer
An imaging spectrometer and near-infrared technology, applied in the field of space remote sensing imaging spectroscopy, can solve the problems of short wavelength band and small dynamic range of detectable signals, and achieve the effect of light weight and small size
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specific Embodiment approach 1
[0010] Specific implementation mode 1. Combination figure 1 and figure 2 Describe this embodiment, ultraviolet, visible, near-infrared prism dispersive imaging spectrometer, this spectrometer includes optical system, CCD detector 9 and electronic system 10, optical system includes telescopic system and spectral imaging system, telescopic system includes aperture stop 2 and a telescope 2, the spectral imaging system includes an incident slit 3, a plane folding mirror 4, a collimating mirror 5, a dispersion prism 6, an imaging mirror 7 and a sub-band attenuation filter 8. The beams of ultraviolet, visible, and near-infrared bands emitted by the target are first imaged on the incident slit 3 through the aperture stop 1 and the telescope 2, and then pass through the plane folding mirror 4, collimating mirror 5, and dispersion The prism 6, the imaging mirror 7 and the sub-band attenuation filter 8 are imaged on the CCD detector 8, and the two-dimensional spectral image is obtaine...
specific Embodiment approach 2
[0014] Specific embodiment two, combine figure 1 and figure 2 Describe this embodiment. This embodiment is the application of the ultraviolet, visible, and near-infrared prism dispersive imaging spectrometer described in Embodiment 1. The spectrometer described in Embodiment 1 is applied to ultraviolet-visible-near-infrared atmospheric remote sensing, and the working band 250-1000nm, the telescope is a single off-axis parabolic mirror, the focal length of the telescope is 120mm, the field of view is 2.4°×0.024°, the size of the entrance slit is 5mm×0.05mm, and the size of the aperture stop is Φ30mm. Atmospheric astigmatism in the ultraviolet-visible-near-infrared band is imaged on the entrance slit through the aperture diaphragm and the telescope. Both the collimating mirror and the imaging mirror are six-time off-axis aspheric mirrors, the radius of curvature of the collimating mirror is 573.51, the coefficient of the second order is -0.21077, and the coefficient of the six...
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