Dual-channel common-path prism dispersion broadband imaging spectrometer optical system
An imaging spectrometer and optical system technology, applied in the field of space optics, can solve the problems of large volume and weight, complex structure of broadband imaging spectrometer, etc., and achieve the effect of compact system layout and high spectral transmission efficiency
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specific Embodiment approach 1
[0010] Specific implementation mode 1. Combination figure 1 with figure 2 Describe this embodiment, the optical system of a dual-channel common optical path prism dispersion broadband imaging spectrometer, the optical system includes a first aperture stop 1, a second aperture stop 2, a telescope 5, an entrance slit 6, and a first collimating mirror 7 , the second collimating mirror 8, the dispersion prism 9, the first imaging mirror 10, the second imaging mirror 11 and the detector image plane 12; The first channel 3 and the second channel 4 are respectively incident on the same telescope 5, imaged on the incident slit 6 by the telescope 5, and after exiting from the incident slit 6, pass through the first collimating mirror 7 and the second collimating mirror respectively 8, incident on the dispersion prism 9, incident on the first imaging mirror 10 after being dispersed by the dispersion prism 9, incident on the second imaging mirror 11 after being reflected by the first i...
specific Embodiment approach 2
[0013] Specific embodiment two, this embodiment is the application of the dual-channel co-optical path prism dispersion wide-band imaging spectrometer optical system described in specific embodiment one, this embodiment detects the atmospheric ozone profile in a limbo observation mode, and the orbital height H =833km, the distance from the instrument to the limb observation point is 3365km, the spectral resolution is 1.5nm-40nm, and the spatial resolution is 3km. The focal length of the optical system of the imaging spectrometer is 69mm, the field of view is 2.3°×0.034°, and the working band is 280-1000nm. Atmospheric limb scenes are incident on the same telescope 5 through the first aperture stop 1 and the second aperture stop 2 into a first channel 3 and a second channel 4 . The aperture of the first aperture stop 1 is 6mm, and the aperture of the second aperture stop 2 is 10mm. The large aperture is used for weak signal detection, and the small aperture is used for strong s...
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